From 8d7f724ee43a8485608ac9a2e1fb654c19e33614 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Tue, 20 Jun 2023 15:59:05 +0200 Subject: [PATCH 01/48] created hidden photon files and started work --- .gitignore | 1 + inc/TRestAxionSolarHiddenPhotonFlux.h | 125 +++++ src/TRestAxionSolarHiddenPhotonFlux.cxx | 700 ++++++++++++++++++++++++ 3 files changed, 826 insertions(+) create mode 100644 inc/TRestAxionSolarHiddenPhotonFlux.h create mode 100644 src/TRestAxionSolarHiddenPhotonFlux.cxx diff --git a/.gitignore b/.gitignore index f57a1172..58ad2261 100644 --- a/.gitignore +++ b/.gitignore @@ -1,3 +1,4 @@ build *.root **/.DS_Store +*.json \ No newline at end of file diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h new file mode 100644 index 00000000..3a31e634 --- /dev/null +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -0,0 +1,125 @@ +/************************************************************************* + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +#ifndef _TRestAxionSolarQCDFlux +#define _TRestAxionSolarQCDFlux + +#include +#include + + +//! A metadata class to load tabulated solar hidden photon fluxes. Mass and coupling set to 1. +class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { + private: + /// The filename containing the solar flux table with continuum spectrum + std::string fFluxDataFile = ""; //< + + /// The filename containing the resonance width (wGamma) + std::string fWGammaDataFile = ""; //< + + /// The filename containing the plasma freqency (wp) table + std::string fWpDataFile = ""; //< + + /// It will be used when loading `.flux` files to define the input file energy binsize in eV. + Double_t fBinSize = 0; //< + + /// It will be used when loading `.flux` files to define the threshold for peak identification + Double_t fPeakSigma = 0; //< + + /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFluxTable; //! + + /// The tabulated resonance width TH1F(200,0,20)keV in eV2 versus solar radius + std::vector fWGammaTable; //! + + /// The solar plasma frequency vector in eV versus solar radius + std::vector fWpTable; //! + + /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) + std::vector fFluxTableIntegrals; //! + + /// A pointer to the continuum spectrum histogram + TH1F* fContinuumHist = nullptr; //! + + /// A pointer to the superposed monochromatic and continuum spectrum histogram + TH1F* fTotalHist = nullptr; //! + + void ReadFluxFile(); + void LoadContinuumFluxTable(); + void LoadMonoChromaticFluxTable(); + void IntegrateSolarFluxes(); + + public: + /// It returns true if continuum flux spectra was loaded + Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } + + /// It returns true if width table was loaded + Bool_t isWidthTableLoaded() { return fWGammaTable.size() > 0; } + + /// It returns true if plasma frequency table was loaded + Bool_t isPlasmaFreqLoaded() { return fWpTable.size() > 0; } + + /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range + Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; + + /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), + Double_t mass = 0) override; + + /// It defines how to read the solar tables at the inhereted class + Bool_t LoadTables() override; + + /// It returns the total integrated flux at earth in cm-2 s-1 + Double_t GetTotalFlux(Double_t mass = 0) override { + return fTotalContinuumFlux + fTotalMonochromaticFlux; + } + + /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 + TH1F* GetEnergySpectrum(Double_t m = 0) override { return GetTotalSpectrum(); } + + TH1F* GetContinuumSpectrum(); + TH1F* GetMonochromaticSpectrum(); + TH1F* GetTotalSpectrum(); + + virtual TCanvas* DrawSolarFlux() override; + + /// Tables might be loaded using a solar model description by TRestAxionSolarModel + void InitializeSolarTable(TRestAxionSolarModel* model) { + // TOBE implemented + // This method should initialize the tables fFluxTable and fFluxLines + } + + void ExportTables(Bool_t ascii = false) override; + + void PrintMetadata() override; + + void PrintContinuumSolarTable(); + void PrintIntegratedRingFlux(); + void PrintMonoChromaticFlux(); + + TRestAxionSolarQCDFlux(); + TRestAxionSolarQCDFlux(const char* cfgFileName, std::string name = ""); + ~TRestAxionSolarQCDFlux(); + + ClassDefOverride(TRestAxionSolarQCDFlux, 1); +}; +#endif diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx new file mode 100644 index 00000000..0140f6fd --- /dev/null +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -0,0 +1,700 @@ +/******************** REST disclaimer *********************************** + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +////////////////////////////////////////////////////////////////////////// +/// TRestAxionSolarQCDFlux will use a file in ASCII or binary format to initialize +/// a solar flux table that will describe the solar flux spectrum as a function +/// of the solar radius. +/// +/// This class may serve to load any generic flux definition that is independent +/// from the axion mass. However, since the design of the class was motivated to +/// reproduce the standard QCD axion flux, therefore the name of the class. +/// +/// Another scenario arises when the axion or an axion-like particle production +/// mechanism depends on its mass, and we may need to introduce a flux description +/// as the given in the class TRestAxionSolarHiddenPhotonFlux. Both classes are +/// prototyped by a pure base class TRestAxionSolarFlux that defines common methods +/// used to evaluate the flux, and generate Monte-Carlo events inside +/// TRestAxionGeneratorProcess. +/// +/// ### Basic use +/// +/// Once the class has been initialized, the main use of this class will be provided +/// by the method TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius. This method will +/// return a random axion energy and position inside the solar radius following the +/// distributions given by the solar flux tables. +/// +/// Description of the specific parameters accepted by this metadata class. +/// - *fluxDataFile:* A table with 100 rows representing the solar ring flux from the +/// center to the corona, and 200 columns representing the flux, measured in cm-2 s-1 keV-1, +/// for the range (0,20)keV in steps of 100eV. The table could be provided in ASCII format, +/// using `.dat` extension, or it might be a binary table using `.N200f` extension. +/// - *fluxSptFile:* A table where each column represents a monochromatic energy. The +/// column contains 101 rows, the first element is the energy of the monochromatic line +/// while the next 100 elements contain the flux, measured in cm-2 s-1, integrated to +/// each solar ring, being the second element the ring in the center of the sun. +/// +/// Additionally this class will be able to read `.flux` files that are the original files +/// produced in 3-columns format (inner radius [solar units] / energy [keV] / +/// flux [cm-2 s-1 keV-1]). The `.flux` files may contain the full information, +/// continuum and spectral components. Those components will be splited into two independent +/// contributions by TRestAxionSolarQCDFlux::ReadFluxFile to be managed internally. Two +/// additional parameters *will be required* to translate the `.flux` files into the tables +/// that are understood by this class. +/// - *binSize:* The energy binning used on the `.flux` file and inside the histogram used +/// for monochromatic lines identification. +/// - *peakSigma:* The ratio between the flux provided at the `.flux` file and the +/// average flux calculated in the peak surroundings. If the flux ratio is higher than +/// this value, the flux at that particular bin will be considered a peak. +/// +/// Optionally, if we want to consider a different binning on the monochromatic/continuum +/// histogram used internally for the calculation we may specify optionally a new parameter. +/// In that case, `fBinSize` will be the binning of the internal histogram, while the new +/// parameter will be the binning given inside the `.flux` file. +/// - *fluxBinSize:* The bin size used on the `.flux` table. +/// +/// Pre-generated solar axion flux tables will be available at the +/// [axionlib-data](https://github.com/rest-for-physics/axionlib-data/tree/master) +/// repository. The different RML flux definitions used to load those tables +/// will be found at the +/// [fluxes.rml](https://github.com/rest-for-physics/axionlib-data/blob/master/solarFlux/fluxes.rml) +/// file found at the axionlib-data repository. +/// +/// Inside a local REST installation, the `fluxes.rml` file will be found at the REST +/// installation directory, and it will be located automatically by the +/// TRestMetadata::SearchFile method. +/// +/// ### A basic RML definition +/// +/// The following definition integrates an axion-photon component with a continuum +/// spectrum using a Primakoff production model, and a dummy spectrum file that +/// includes two monocrhomatic lines at different solar disk radius positions. +/// +/// \code +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// \endcode +/// +/// \warning When the flux is loaded manually inside the `restRoot` interactive +/// shell, or inside a macro or script, after metadata initialization, it is necessary +/// to call the method TRestAxionSolarQCDFlux::LoadTables to trigger the tables +/// initialization. +/// +/// ### Performing MonteCarlo tests using pre-loaded tables +/// +/// In order to test the response of different solar flux definitions we may use the script +/// `solarPlot.py` found at `pipeline/metadata/solarFlux/`. This script will generate a +/// number of particles and it will assign to each particle an energy and solar disk +/// location with the help of the method TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius. +/// +/// \code +/// python3 solarPlotQCD.py --fluxname LennertHoofABC --N 1000000 +/// \endcode +/// +/// By default, it will load the flux definition found at `fluxes.rml` from the +/// `axionlib-data` repository, and generate a `png` image with the resuts from the +/// Monte Carlo execution. +/// +/// \htmlonly \endhtmlonly +/// +/// ![Solar flux distributions MC-generated with TRestAxionSolarQCDFlux.](ABC_flux_MC.png) +/// +/// ### Reading solar flux tables from `.flux` files +/// +/// In a similar way we may initialize the class using a `.flux` file. The `.flux` described +/// previously will contain a high definition flux table measured in `cm-2 s-1 keV-1` as a +/// function of the energy (from 0 to 20keV) and the inner solar radius (from 0 to 1). The +/// binning of this table will be typically between 1eV and 10eV. +/// +/// The class TRestAxionSolarQCDFlux will be initialized directly using the `.flux` file +/// provided under the `fluxDataFile` parameter. During the initialization, the flux will be +/// splitted into two independent flux components. One smooth continuum component integrated +/// in 100 eV steps, and a monochromatic peak components. +/// +/// In order to help with the identification of peaks we need to define the `binSize` used in +/// the `.flux` table and the `peakSigma` defining the number of sigmas over the average for +/// a bin to be considered a peak. +/// +/// \code +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// \endcode +/// +/// We will be able to load this file as usual, using the following recipe inside +/// `restRoot`, +/// +/// \code +/// TRestAxionSolarQCDFlux *sFlux = new TRestAxionSolarQCDFlux("fluxes.rml", "LennertHoofABC") +/// sFlux->Initialize() +/// TCanvas *c = sFlux->DrawSolarFluxes() +/// c->Print("ABC_FluxTable.png" ) +/// \endcode +/// +/// will generate the following figure. +/// +/// \htmlonly \endhtmlonly +/// +/// ![Solar flux distributions generated with TRestAxionSolarQCDFlux::DrawSolarFlux.](ABC_FluxTable.png) +/// +/// ### Exporting the solar flux tables +/// +/// On top of that, we will be able to export those tables to the TRestAxionSolarQCDFlux standard +/// format to be used in later occasions. +/// +/// \code +/// TRestAxionSolarQCDFlux *sFlux = new TRestAxionSolarQCDFlux("fluxes.rml", "LennertHoofABC") +/// sFlux->Initialize() +/// sFlux->ExportTables() +/// \endcode +/// +/// which will produce two files, a binary table `.N200f` with the continuum flux, and an ASCII +/// table containning the `.spt` monochromatic lines. The filename root will be extracted from +/// the original `.flux` file. Optionally we may export the continuum flux to an ASCII file by +/// indicating it at the TRestAxionSolarQCDFlux::ExportTables method call. The files will be placed +/// at the REST user space, at `$HOME/.rest/export/` directory. +/// +/// TODO Implement the method TRestAxionSolarQCDFlux::InitializeSolarTable using +/// a solar model description by TRestAxionSolarModel. +/// +/// TODO Perhaps it would be interesting to replace fFluxTable for a TH2D +/// +///-------------------------------------------------------------------------- +/// +/// RESTsoft - Software for Rare Event Searches with TPCs +/// +/// History of developments: +/// +/// 2023-May: Specific methods extracted from TRestAxionSolarFlux +/// Javier Galan +/// +/// \class TRestAxionSolarQCDFlux +/// \author Javier Galan +/// +///
+/// + +#include "TRestAxionSolarHiddenPhotonFlux.h" +using namespace std; + +ClassImp(TRestAxionSolarHiddenPhotonFlux); + +/////////////////////////////////////////////// +/// \brief Default constructor +/// +TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux() : TRestAxionSolarFlux() {} + +/////////////////////////////////////////////// +/// \brief Constructor loading data from a config file +/// +/// If no configuration path is defined using TRestMetadata::SetConfigFilePath +/// the path to the config file must be specified using full path, absolute or +/// relative. +/// +/// The default behaviour is that the config file must be specified with +/// full path, absolute or relative. +/// +/// \param cfgFileName A const char* giving the path to an RML file. +/// \param name The name of the specific metadata. It will be used to find the +/// corresponding TRestAxionMagneticField section inside the RML. +/// +TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, string name) + : TRestAxionSolarFlux(cfgFileName) { + LoadConfigFromFile(fConfigFileName, name); + + if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Info) PrintMetadata(); +} + +/////////////////////////////////////////////// +/// \brief Default destructor +/// +TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} + +/////////////////////////////////////////////// +/// \brief It will load the tables in memory by using the filename information provided +/// inside the metadata members. +/// +Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { + if (fFluxDataFile == "" && fFluxSptFile == "") return false; + + if (TRestTools::GetFileNameExtension(fFluxDataFile) == "flux") { + ReadFluxFile(); + } else { + LoadContinuumFluxTable(); + LoadMonoChromaticFluxTable(); + } + + IntegrateSolarFluxes(); + + return true; +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing continuum spectra as a +/// function of the solar radius. It will be called by TRestAxionSolarFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { + if (fFluxDataFile == "") { + RESTDebug << "TRestAxionSolarHiddenPhotonflux::LoadContinuumFluxTable. No solar flux table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fFluxDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + std::vector> fluxTable; + if (TRestTools::GetFileNameExtension(fFluxDataFile) == "dat") { + std::vector> doubleTable; + if (!TRestTools::ReadASCIITable(fullPathName, doubleTable)) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. " << RESTendl; + RESTError << "Could not read solar flux table : " << fFluxDataFile << RESTendl; + return; + } + for (const auto& row : doubleTable) { + std::vector floatVec(row.begin(), row.end()); + fluxTable.push_back(floatVec); + } + } else if (TRestTools::IsBinaryFile(fFluxDataFile)) + TRestTools::ReadBinaryTable(fullPathName, fluxTable); + else { + fluxTable.clear(); + RESTError << "Filename extension was not recognized!" << RESTendl; + RESTError << "Solar flux table will not be populated" << RESTendl; + RESTError << "Filename extension: " << TRestTools::GetFileNameExtension(fFluxDataFile) << RESTendl; + } + + if (fluxTable.size() != 1000 && fluxTable[0].size() != 200) { + fluxTable.clear(); + RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows or columns" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1F* h = new TH1F(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); + fFluxTable.push_back(h); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing the plasma frequency as a +/// function of the solar radius. It will be called by TRestAxionPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { + if (fFluxDataFile == "") { + RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fFluxDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + std::vector> fluxTable; + if (TRestTools::GetFileNameExtension(fFluxDataFile) == "dat") { + std::vector> doubleTable; + if (!TRestTools::ReadASCIITable(fullPathName, doubleTable)) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. " << RESTendl; + RESTError << "Could not read solar flux table : " << fFluxDataFile << RESTendl; + return; + } + for (const auto& row : doubleTable) { + fluxTable.push_back(row); + } + } else if (TRestTools::IsBinaryFile(fFluxDataFile)) + TRestTools::ReadBinaryTable(fullPathName, fluxTable); + else { + fluxTable.clear(); + RESTError << "Filename extension was not recognized!" << RESTendl; + RESTError << "Solar flux table will not be populated" << RESTendl; + RESTError << "Filename extension: " << TRestTools::GetFileNameExtension(fFluxDataFile) << RESTendl; + } + + if (fluxTable.size() != 1000) { + fluxTable.clear(); + RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1F* h = new TH1F(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); + h->SetBinContent(1, fluxTable[n][0]); + fWpTable.push_back(h); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containning monochromatic spectral +/// lines as a function of the solar radius. It will be called by TRestAxionSolarQCDFlux::Initialize. +/// +void TRestAxionSolarQCDFlux::LoadMonoChromaticFluxTable() { + if (fFluxSptFile == "") { + RESTDebug << "TRestAxionSolarflux::LoadMonoChromaticFluxTable. No solar flux monochromatic table was " + "defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fFluxSptFile); + + RESTDebug << "Loading monochromatic lines from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + std::vector> doubleTable; + if (!TRestTools::ReadASCIITable(fullPathName, doubleTable)) { + RESTError << "TRestAxionSolarQCDFlux::LoadMonoChromaticFluxTable." << RESTendl; + RESTError << "Could not read solar flux table : " << fFluxSptFile << RESTendl; + return; + } + + std::vector> asciiTable; + for (const auto& row : doubleTable) { + std::vector floatVec(row.begin(), row.end()); + asciiTable.push_back(floatVec); + } + + fFluxLines.clear(); + + if (asciiTable.size() != 101) { + RESTError << "LoadMonoChromaticFluxTable. The table does not contain the right number of rows" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + return; + } + + for (unsigned int en = 0; en < asciiTable[0].size(); en++) { + Float_t energy = asciiTable[0][en]; + TH1F* h = new TH1F(Form("%s_MonochromeFluxAtEnergy%6.4lf", GetName(), energy), "", 100, 0, 1); + for (unsigned int r = 1; r < asciiTable.size(); r++) h->SetBinContent(r, asciiTable[r][en]); + fFluxLines[energy] = h; + } +} + + +/////////////////////////////////////////////// +/// \brief It builds a histogram with the continuum spectrum component. +/// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. +/// +TH1F* TRestAxionSolarQCDFlux::GetContinuumSpectrum() { + if (fContinuumHist != nullptr) { + delete fContinuumHist; + fContinuumHist = nullptr; + } + + fContinuumHist = new TH1F("ContinuumHist", "", 200, 0, 20); + for (const auto& x : fFluxTable) { + fContinuumHist->Add(x); + } + + fContinuumHist->SetStats(0); + fContinuumHist->GetXaxis()->SetTitle("Energy [keV]"); + fContinuumHist->GetXaxis()->SetTitleSize(0.05); + fContinuumHist->GetXaxis()->SetLabelSize(0.05); + fContinuumHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); + fContinuumHist->GetYaxis()->SetTitleSize(0.05); + fContinuumHist->GetYaxis()->SetLabelSize(0.05); + + return fContinuumHist; +} + +/////////////////////////////////////////////// +/// \brief It builds a histogram with the monochromatic spectrum component. +/// The flux will be expressed in cm-2 s-1 eV-1. Binned in 1eV steps. +/// +TH1F* TRestAxionSolarQCDFlux::GetMonochromaticSpectrum() { + if (fMonoHist != nullptr) { + delete fMonoHist; + fMonoHist = nullptr; + } + + fMonoHist = new TH1F("MonochromaticHist", "", 20000, 0, 20); + for (const auto& x : fFluxLines) { + fMonoHist->Fill(x.first, x.second->Integral()); // cm-2 s-1 eV-1 + } + + fMonoHist->SetStats(0); + fMonoHist->GetXaxis()->SetTitle("Energy [keV]"); + fMonoHist->GetXaxis()->SetTitleSize(0.05); + fMonoHist->GetXaxis()->SetLabelSize(0.05); + fMonoHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 eV-1]"); + fMonoHist->GetYaxis()->SetTitleSize(0.05); + fMonoHist->GetYaxis()->SetLabelSize(0.05); + + return fMonoHist; +} + +/////////////////////////////////////////////// +/// \brief It builds a histogram adding the continuum and the monochromatic +/// spectrum component. The flux will be expressed in cm-2 s-1 keV-1. +/// Binned in 1eV steps. +/// +TH1F* TRestAxionSolarQCDFlux::GetTotalSpectrum() { + TH1F* hm = GetMonochromaticSpectrum(); + TH1F* hc = GetContinuumSpectrum(); + + if (fTotalHist != nullptr) { + delete fTotalHist; + fTotalHist = nullptr; + } + + fTotalHist = new TH1F("fTotalHist", "", 20000, 0, 20); + for (int n = 0; n < hc->GetNbinsX(); n++) { + for (int m = 0; m < 100; m++) { + fTotalHist->SetBinContent(n * 100 + 1 + m, hc->GetBinContent(n + 1)); + } + } + + for (int n = 0; n < hm->GetNbinsX(); n++) + // 1e-2 is the renormalization from 20000 bins to 200 bins + fTotalHist->SetBinContent(n + 1, fTotalHist->GetBinContent(n + 1) + 100 * hm->GetBinContent(n + 1)); + + fTotalHist->SetStats(0); + fTotalHist->GetXaxis()->SetTitle("Energy [keV]"); + fTotalHist->GetXaxis()->SetTitleSize(0.05); + fTotalHist->GetXaxis()->SetLabelSize(0.05); + fTotalHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); + fTotalHist->GetYaxis()->SetTitleSize(0.05); + fTotalHist->GetYaxis()->SetLabelSize(0.05); + + return fTotalHist; +} + +/////////////////////////////////////////////// +/// \brief A helper method to initialize the internal class data members with the +/// integrated flux for each solar ring. It will be called by TRestAxionSolarQCDFlux::Initialize. +/// +void TRestAxionSolarQCDFlux::IntegrateSolarFluxes() { + fFluxLineIntegrals.clear(); + fTotalMonochromaticFlux = 0; + + for (const auto& line : fFluxLines) { + fTotalMonochromaticFlux += line.second->Integral(); + fFluxLineIntegrals.push_back(fTotalMonochromaticFlux); + } + + for (unsigned int n = 0; n < fFluxLineIntegrals.size(); n++) + fFluxLineIntegrals[n] /= fTotalMonochromaticFlux; + + fTotalContinuumFlux = 0.0; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + fTotalContinuumFlux += fFluxTable[n]->Integral() * 0.1; // We integrate in 100eV steps + fFluxTableIntegrals.push_back(fTotalContinuumFlux); + } + + for (unsigned int n = 0; n < fFluxTableIntegrals.size(); n++) + fFluxTableIntegrals[n] /= fTotalContinuumFlux; + + fFluxRatio = fTotalMonochromaticFlux / (fTotalContinuumFlux + fTotalMonochromaticFlux); +} + +/////////////////////////////////////////////// +/// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range +/// +Double_t TRestAxionSolarQCDFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { + if (eRange.X() == -1 && eRange.Y() == -1) { + if (GetTotalFlux() == 0) IntegrateSolarFluxes(); + return GetTotalFlux(); + } + + Double_t flux = 0; + for (const auto& line : fFluxLines) + if (line.first > eRange.X() && line.first < eRange.Y()) flux += line.second->Integral(); + + fTotalContinuumFlux = 0.0; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + flux += fFluxTable[n]->Integral(fFluxTable[n]->FindFixBin(eRange.X()), + fFluxTable[n]->FindFixBin(eRange.Y())) * + 0.1; // We integrate in 100eV steps + } + + return flux; +} + +/////////////////////////////////////////////// +/// \brief It returns a random solar radius position and energy according to the +/// flux distributions defined inside the solar tables loaded in the class +/// +std::pair TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius(TVector2 eRange, + Double_t mass) { + std::pair result = {0, 0}; + if (!AreTablesLoaded()) return result; + Double_t rnd = fRandom->Rndm(); + if (fTotalMonochromaticFlux == 0 || fRandom->Rndm() > fFluxRatio) { + // Continuum + for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { + if (rnd < fFluxTableIntegrals[r]) { + Double_t energy = fFluxTable[r]->GetRandom(); + if (eRange.X() != -1 && eRange.Y() != -1) { + if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); + } + Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.01; + std::pair p = {energy, radius}; + return p; + } + } + } else { + // Monochromatic + int n = 0; + for (const auto& line : fFluxLines) { + if (rnd < fFluxLineIntegrals[n]) { + std::pair p = {line.first, line.second->GetRandom()}; + return p; + } + n++; + } + } + return result; +} + +/////////////////////////////////////////////// +/// \brief It prints on screen the table that has been loaded in memory +/// +void TRestAxionSolarQCDFlux::PrintContinuumSolarTable() { + cout << "Continuum solar flux table: " << endl; + cout << "--------------------------- " << endl; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + for (int m = 0; m < fFluxTable[n]->GetNbinsX(); m++) + cout << fFluxTable[n]->GetBinContent(m + 1) << "\t"; + cout << endl; + cout << endl; + } + cout << endl; +} + +/////////////////////////////////////////////// +/// \brief It prints on screen the integrated solar flux per solar ring +/// +void TRestAxionSolarQCDFlux::PrintIntegratedRingFlux() { + cout << "Integrated solar flux per solar ring: " << endl; + cout << "--------------------------- " << endl; + /* + for (int n = 0; n < fFluxPerRadius.size(); n++) + cout << "n : " << n << " flux : " << fFluxPerRadius[n] << endl; + cout << endl; + */ +} + +/////////////////////////////////////////////// +/// \brief It prints on screen the spectral lines loaded in memory +/// +void TRestAxionSolarQCDFlux::PrintMonoChromaticFlux() { + // cout << "Number of monochromatic lines: " << fFluxPerRadius.size() << endl; + cout << "+++++++++++++++++++++++++++++++++++" << endl; + for (auto const& line : fFluxLines) { + cout << "Energy : " << line.first << " keV" << endl; + cout << "-----------------" << endl; + for (int n = 0; n < line.second->GetNbinsX(); n++) + cout << "R : " << line.second->GetBinCenter(n + 1) + << " flux : " << line.second->GetBinContent(n + 1) << " cm-2 s-1" << endl; + } +} + +/////////////////////////////////////////////// +/// \brief Prints on screen the information about the metadata members of TRestAxionSolarQCDFlux +/// +void TRestAxionSolarQCDFlux::PrintMetadata() { + TRestAxionSolarFlux::PrintMetadata(); + + if (fFluxDataFile != "") + RESTMetadata << " - Solar axion flux datafile (continuum) : " << fFluxDataFile << RESTendl; + if (fFluxSptFile != "") + RESTMetadata << " - Solar axion flux datafile (monochromatic) : " << fFluxSptFile << RESTendl; + RESTMetadata << "-------" << RESTendl; + RESTMetadata << " - Total monochromatic flux : " << fTotalMonochromaticFlux << " cm-2 s-1" << RESTendl; + RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; + RESTMetadata << "++++++++++++++++++" << RESTendl; + + if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Debug) { + PrintContinuumSolarTable(); + PrintMonoChromaticFlux(); + PrintIntegratedRingFlux(); + } +} + +/////////////////////////////////////////////// +/// \brief It will create files with the continuum and spectral flux components to be used +/// in a later ocasion. +/// +void TRestAxionSolarQCDFlux::ExportTables(Bool_t ascii) { + string rootFilename = TRestTools::GetFileNameRoot(fFluxDataFile); + + string path = REST_USER_PATH + "/export/"; + + if (!TRestTools::fileExists(path)) { + std::cout << "Creating path: " << path << std::endl; + int z = system(("mkdir -p " + path).c_str()); + if (z != 0) RESTError << "Could not create directory " << path << RESTendl; + } + + if (fFluxTable.size() > 0) { + std::vector> table; + for (const auto& x : fFluxTable) { + std::vector row; + for (int n = 0; n < x->GetNbinsX(); n++) row.push_back(x->GetBinContent(n + 1)); + + table.push_back(row); + } + + if (!ascii) + TRestTools::ExportBinaryTable(path + "/" + rootFilename + ".N200f", table); + else + TRestTools::ExportASCIITable(path + "/" + rootFilename + ".dat", table); + } + + if (fFluxLines.size() > 0) { + std::vector> table; + for (const auto& x : fFluxLines) { + std::vector row; + row.push_back(x.first); + for (int n = 0; n < x.second->GetNbinsX(); n++) row.push_back(x.second->GetBinContent(n + 1)); + + table.push_back(row); + } + + TRestTools::TransposeTable(table); + + TRestTools::ExportASCIITable(path + "/" + rootFilename + ".spt", table); + } +} From f1e5be3c9394e9ba010a533f5c4509491c1265b5 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Thu, 22 Jun 2023 09:53:53 +0200 Subject: [PATCH 02/48] Coded in HP flux calculation --- inc/TRestAxionSolarHiddenPhotonFlux.h | 17 +- src/TRestAxionSolarHiddenPhotonFlux.cxx | 323 ++++++++++++------------ 2 files changed, 170 insertions(+), 170 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 3a31e634..929859a1 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -30,14 +30,20 @@ //! A metadata class to load tabulated solar hidden photon fluxes. Mass and coupling set to 1. class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { private: + /// The hidden photon mass used for calculation + double HiddenPhotonMass; + + /// The value of the kinetic mixing parameter used for calculation + double HiddenPhotonKineticMixing; + /// The filename containing the solar flux table with continuum spectrum std::string fFluxDataFile = ""; //< /// The filename containing the resonance width (wGamma) - std::string fWGammaDataFile = ""; //< + std::string fWidthDataFile = ""; //< /// The filename containing the plasma freqency (wp) table - std::string fWpDataFile = ""; //< + std::string fPlasmaFreqDataFile = ""; //< /// It will be used when loading `.flux` files to define the input file energy binsize in eV. Double_t fBinSize = 0; //< @@ -49,10 +55,13 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { std::vector fFluxTable; //! /// The tabulated resonance width TH1F(200,0,20)keV in eV2 versus solar radius - std::vector fWGammaTable; //! + std::vector fWidthTable; //! /// The solar plasma frequency vector in eV versus solar radius - std::vector fWpTable; //! + std::vector fPlasmaFreqTable; //! + + /// The total solar flux TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFullFluxTable; //! /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) std::vector fFluxTableIntegrals; //! diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 0140f6fd..5f4a00af 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -39,38 +39,22 @@ /// ### Basic use /// /// Once the class has been initialized, the main use of this class will be provided -/// by the method TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius. This method will +/// by the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. This method will /// return a random axion energy and position inside the solar radius following the /// distributions given by the solar flux tables. /// /// Description of the specific parameters accepted by this metadata class. -/// - *fluxDataFile:* A table with 100 rows representing the solar ring flux from the +/// - *fluxDataFile:* A table with 1000 rows representing the solar ring flux from the /// center to the corona, and 200 columns representing the flux, measured in cm-2 s-1 keV-1, -/// for the range (0,20)keV in steps of 100eV. The table could be provided in ASCII format, -/// using `.dat` extension, or it might be a binary table using `.N200f` extension. -/// - *fluxSptFile:* A table where each column represents a monochromatic energy. The -/// column contains 101 rows, the first element is the energy of the monochromatic line -/// while the next 100 elements contain the flux, measured in cm-2 s-1, integrated to -/// each solar ring, being the second element the ring in the center of the sun. -/// -/// Additionally this class will be able to read `.flux` files that are the original files -/// produced in 3-columns format (inner radius [solar units] / energy [keV] / -/// flux [cm-2 s-1 keV-1]). The `.flux` files may contain the full information, -/// continuum and spectral components. Those components will be splited into two independent -/// contributions by TRestAxionSolarQCDFlux::ReadFluxFile to be managed internally. Two -/// additional parameters *will be required* to translate the `.flux` files into the tables -/// that are understood by this class. -/// - *binSize:* The energy binning used on the `.flux` file and inside the histogram used -/// for monochromatic lines identification. -/// - *peakSigma:* The ratio between the flux provided at the `.flux` file and the -/// average flux calculated in the peak surroundings. If the flux ratio is higher than -/// this value, the flux at that particular bin will be considered a peak. -/// -/// Optionally, if we want to consider a different binning on the monochromatic/continuum -/// histogram used internally for the calculation we may specify optionally a new parameter. -/// In that case, `fBinSize` will be the binning of the internal histogram, while the new -/// parameter will be the binning given inside the `.flux` file. -/// - *fluxBinSize:* The bin size used on the `.flux` table. +/// for the range (0,20)keV in steps of 100eV. The table is provided as a binary table using +/// `.N200f` extension. +/// - *widthDataFile:* A table with 1000 rows representing the width of the hidden photon +/// resonant production for each solar ring from the center to the corona, and 200 columns +/// representing the width, measured in eV2, for the range (0,20)keV in steps of 100eV. The +/// table is provided as a binary table using `.N200f` extension. +/// - *plasmaFreqDataFile:* A table with 1000 rows and only 1 column representing the solar +/// plasma frequency for each solar ring from the center to the corona, measured in eV. The +/// table is provided as a binary table using `.N1f` extension. /// /// Pre-generated solar axion flux tables will be available at the /// [axionlib-data](https://github.com/rest-for-physics/axionlib-data/tree/master) @@ -105,7 +89,7 @@ /// /// \warning When the flux is loaded manually inside the `restRoot` interactive /// shell, or inside a macro or script, after metadata initialization, it is necessary -/// to call the method TRestAxionSolarQCDFlux::LoadTables to trigger the tables +/// to call the method TRestAxionSolarHiddenPhotonFlux::LoadTables to trigger the tables /// initialization. /// /// ### Performing MonteCarlo tests using pre-loaded tables @@ -113,10 +97,10 @@ /// In order to test the response of different solar flux definitions we may use the script /// `solarPlot.py` found at `pipeline/metadata/solarFlux/`. This script will generate a /// number of particles and it will assign to each particle an energy and solar disk -/// location with the help of the method TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius. +/// location with the help of the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. /// /// \code -/// python3 solarPlotQCD.py --fluxname LennertHoofABC --N 1000000 +/// python3 solarPlotHiddenPhoton.py --fluxname HiddenPhoton --N 1000000 /// \endcode /// /// By default, it will load the flux definition found at `fluxes.rml` from the @@ -127,67 +111,21 @@ /// /// ![Solar flux distributions MC-generated with TRestAxionSolarQCDFlux.](ABC_flux_MC.png) /// -/// ### Reading solar flux tables from `.flux` files -/// -/// In a similar way we may initialize the class using a `.flux` file. The `.flux` described -/// previously will contain a high definition flux table measured in `cm-2 s-1 keV-1` as a -/// function of the energy (from 0 to 20keV) and the inner solar radius (from 0 to 1). The -/// binning of this table will be typically between 1eV and 10eV. -/// -/// The class TRestAxionSolarQCDFlux will be initialized directly using the `.flux` file -/// provided under the `fluxDataFile` parameter. During the initialization, the flux will be -/// splitted into two independent flux components. One smooth continuum component integrated -/// in 100 eV steps, and a monochromatic peak components. -/// -/// In order to help with the identification of peaks we need to define the `binSize` used in -/// the `.flux` table and the `peakSigma` defining the number of sigmas over the average for -/// a bin to be considered a peak. -/// -/// \code -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// \endcode -/// -/// We will be able to load this file as usual, using the following recipe inside -/// `restRoot`, -/// -/// \code -/// TRestAxionSolarQCDFlux *sFlux = new TRestAxionSolarQCDFlux("fluxes.rml", "LennertHoofABC") -/// sFlux->Initialize() -/// TCanvas *c = sFlux->DrawSolarFluxes() -/// c->Print("ABC_FluxTable.png" ) -/// \endcode -/// -/// will generate the following figure. -/// -/// \htmlonly \endhtmlonly -/// -/// ![Solar flux distributions generated with TRestAxionSolarQCDFlux::DrawSolarFlux.](ABC_FluxTable.png) -/// /// ### Exporting the solar flux tables /// -/// On top of that, we will be able to export those tables to the TRestAxionSolarQCDFlux standard -/// format to be used in later occasions. +/// On top of that, we will be able to export those tables to the TRestAxionSolarHiddenPhotonFlux +/// standard format to be used in later occasions. /// /// \code -/// TRestAxionSolarQCDFlux *sFlux = new TRestAxionSolarQCDFlux("fluxes.rml", "LennertHoofABC") +/// TRestAxionSolarHiddenPhotonFlux *sFlux = new TRestAxionSolarHiddenPhotonFlux("fluxes.rml", "HiddenPhoton") /// sFlux->Initialize() /// sFlux->ExportTables() /// \endcode /// -/// which will produce two files, a binary table `.N200f` with the continuum flux, and an ASCII -/// table containning the `.spt` monochromatic lines. The filename root will be extracted from -/// the original `.flux` file. Optionally we may export the continuum flux to an ASCII file by -/// indicating it at the TRestAxionSolarQCDFlux::ExportTables method call. The files will be placed -/// at the REST user space, at `$HOME/.rest/export/` directory. +/// which will produce a binary table `.N200f` with the continuum flux. The filename root will be +/// extracted from the original `.flux` file. Optionally we may export the continuum flux to an +/// ASCII file by indicating it at the TRestAxionSolarHiddenPhotonFlux::ExportTables method call. +/// The files will be placed at the REST user space, at `$HOME/.rest/export/` directory. /// /// TODO Implement the method TRestAxionSolarQCDFlux::InitializeSolarTable using /// a solar model description by TRestAxionSolarModel. @@ -202,6 +140,8 @@ /// /// 2023-May: Specific methods extracted from TRestAxionSolarFlux /// Javier Galan +/// 2023-June: TRestAxionSolarHiddenPhotonFlux created by editing TRestAxionSolarQCDFlux +/// Tomas O'Shea /// /// \class TRestAxionSolarQCDFlux /// \author Javier Galan @@ -250,14 +190,12 @@ TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} /// inside the metadata members. /// Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - if (fFluxDataFile == "" && fFluxSptFile == "") return false; + if (fFluxDataFile == "" || fWidthDataFile == "" || + fPlasmaFreqDataFile == "") return false; - if (TRestTools::GetFileNameExtension(fFluxDataFile) == "flux") { - ReadFluxFile(); - } else { - LoadContinuumFluxTable(); - LoadMonoChromaticFluxTable(); - } + LoadContinuumFluxTable(); + LoadWidthTable(); + LoadPlasmaFreqTable(); IntegrateSolarFluxes(); @@ -266,11 +204,11 @@ Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { /////////////////////////////////////////////// /// \brief A helper method to load the data file containing continuum spectra as a -/// function of the solar radius. It will be called by TRestAxionSolarFlux::Initialize. +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. /// -void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { +void TRestAxionSolarHiddenPhotonFlux::LoadContinuumTable() { if (fFluxDataFile == "") { - RESTDebug << "TRestAxionSolarHiddenPhotonflux::LoadContinuumFluxTable. No solar flux table was defined" + RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" << RESTendl; return; } @@ -280,26 +218,14 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; - std::vector> fluxTable; - if (TRestTools::GetFileNameExtension(fFluxDataFile) == "dat") { - std::vector> doubleTable; - if (!TRestTools::ReadASCIITable(fullPathName, doubleTable)) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. " << RESTendl; - RESTError << "Could not read solar flux table : " << fFluxDataFile << RESTendl; - return; - } - for (const auto& row : doubleTable) { - std::vector floatVec(row.begin(), row.end()); - fluxTable.push_back(floatVec); - } - } else if (TRestTools::IsBinaryFile(fFluxDataFile)) - TRestTools::ReadBinaryTable(fullPathName, fluxTable); - else { + std::vector> fluxTable; + + if (!TRestTools::IsBinaryFile(fFluxDataFile)) { fluxTable.clear(); - RESTError << "Filename extension was not recognized!" << RESTendl; - RESTError << "Solar flux table will not be populated" << RESTendl; - RESTError << "Filename extension: " << TRestTools::GetFileNameExtension(fFluxDataFile) << RESTendl; + RESTError << "File is not in binary format!" << RESTendl; } + + TRestTools::ReadBinaryTable(fullPathName, fluxTable); if (fluxTable.size() != 1000 && fluxTable[0].size() != 200) { fluxTable.clear(); @@ -311,104 +237,125 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1F* h = new TH1F(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); - fFluxTable.push_back(h); + fContinuumTable.push_back(h); } } + /////////////////////////////////////////////// -/// \brief A helper method to load the data file containing the plasma frequency as a -/// function of the solar radius. It will be called by TRestAxionPhotonFlux::Initialize. +/// \brief A helper method to load the data file containing resonance width as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. /// -void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { +void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { if (fFluxDataFile == "") { - RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" + RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadWidthTable. No width table was defined" << RESTendl; return; } - string fullPathName = SearchFile((string)fFluxDataFile); + string fullPathName = SearchFile((string)fWidthDataFile); RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; - std::vector> fluxTable; - if (TRestTools::GetFileNameExtension(fFluxDataFile) == "dat") { - std::vector> doubleTable; - if (!TRestTools::ReadASCIITable(fullPathName, doubleTable)) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. " << RESTendl; - RESTError << "Could not read solar flux table : " << fFluxDataFile << RESTendl; - return; - } - for (const auto& row : doubleTable) { - fluxTable.push_back(row); - } - } else if (TRestTools::IsBinaryFile(fFluxDataFile)) - TRestTools::ReadBinaryTable(fullPathName, fluxTable); - else { + std::vector> fluxTable; + + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { fluxTable.clear(); - RESTError << "Filename extension was not recognized!" << RESTendl; - RESTError << "Solar flux table will not be populated" << RESTendl; - RESTError << "Filename extension: " << TRestTools::GetFileNameExtension(fFluxDataFile) << RESTendl; + RESTError << "File is not in binary format!" << RESTendl; } + + TRestTools::ReadBinaryTable(fullPathName, fluxTable); - if (fluxTable.size() != 1000) { + if (fluxTable.size() != 1000 && fluxTable[0].size() != 200) { fluxTable.clear(); - RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows" + RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; } for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1F* h = new TH1F(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); - h->SetBinContent(1, fluxTable[n][0]); - fWpTable.push_back(h); + TH1F* h = new TH1F(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); + fWidthTable.push_back(h); } } + /////////////////////////////////////////////// -/// \brief A helper method to load the data file containning monochromatic spectral -/// lines as a function of the solar radius. It will be called by TRestAxionSolarQCDFlux::Initialize. +/// \brief A helper method to load the data file containing resonance width as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. /// -void TRestAxionSolarQCDFlux::LoadMonoChromaticFluxTable() { - if (fFluxSptFile == "") { - RESTDebug << "TRestAxionSolarflux::LoadMonoChromaticFluxTable. No solar flux monochromatic table was " - "defined" +void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { + if (fFluxDataFile == "") { + RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" << RESTendl; return; } - string fullPathName = SearchFile((string)fFluxSptFile); + string fullPathName = SearchFile((string)fPlasmaFreqDataFile); - RESTDebug << "Loading monochromatic lines from file : " << RESTendl; + RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; - std::vector> doubleTable; - if (!TRestTools::ReadASCIITable(fullPathName, doubleTable)) { - RESTError << "TRestAxionSolarQCDFlux::LoadMonoChromaticFluxTable." << RESTendl; - RESTError << "Could not read solar flux table : " << fFluxSptFile << RESTendl; - return; - } + std::vector> fluxTable; - std::vector> asciiTable; - for (const auto& row : doubleTable) { - std::vector floatVec(row.begin(), row.end()); - asciiTable.push_back(floatVec); + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { + fluxTable.clear(); + RESTError << "File is not in binary format!" << RESTendl; } + + TRestTools::ReadBinaryTable(fullPathName, fluxTable); - fFluxLines.clear(); - - if (asciiTable.size() != 101) { - RESTError << "LoadMonoChromaticFluxTable. The table does not contain the right number of rows" + if (fluxTable.size() != 1000 && fluxTable[0].size() != 1) { + fluxTable.clear(); + RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1F* h = new TH1F(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); + fPlasmaFreqTable.push_back(h); + } +} + + +/////////////////////////////////////////////// +/// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the +/// kinetic mixing parameter and the hidden photon mass. +/// +void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { + if (!LoadTables()) { + RESTError << "CalculateSolarFlux. The component tables cannot be loaded." << RESTendl; return; } - for (unsigned int en = 0; en < asciiTable[0].size(); en++) { - Float_t energy = asciiTable[0][en]; - TH1F* h = new TH1F(Form("%s_MonochromeFluxAtEnergy%6.4lf", GetName(), energy), "", 100, 0, 1); - for (unsigned int r = 1; r < asciiTable.size(); r++) h->SetBinContent(r, asciiTable[r][en]); - fFluxLines[energy] = h; + for (unsigned int n = 0; n < fluxTable.size(); n++) { + // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (wG)^2 ) + + std::vector mass2Vector(200, pow(HiddenPhotonMass,2)); + float wp = fPlasmaFreqTable[n].GetBinContent(1); + std::vector wp2Vector(200, pow(wp,2)); + + TH1F* hMass = new TH1D("hMass", "hMass", 200, 0, 20) + TH1F* hWp = new TH1D("hWp", "hWp", 200, 0, 20) + TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); + + hMass->FillN(200, massVector); // m^2 hist + hWp->FillN(200, wpVector); // wp^2 hist + TH1F* hWg2 = fWidthTable[n] * fWidthTable[n]; // (omega Gamma)^2 + + hMass->Add(hWp, -1); // (m2 - wp2) + hMass->Multiply(hMass); // (m2 - wp2)^2 + hmass->Add(hWg2); // (m2 - wp2)^2 - (wG)^2 + + TH1F* h = fWidthTable[n] * fContinuumTable[n]; + h->Divide(hMass); + h->Scale(pow(HiddenPhotonMass,4) * pow(HiddenPhotonKineticMixing,2)); + + fFluxTable.push_back(h); } } @@ -501,6 +448,50 @@ TH1F* TRestAxionSolarQCDFlux::GetTotalSpectrum() { return fTotalHist; } +/////////////////////////////////////////////// +/// \brief It draws the contents of a .flux file. This method just receives the +/// +TCanvas* TRestAxionSolarQCDFlux::DrawSolarFlux() { + if (fCanvas != nullptr) { + delete fCanvas; + fCanvas = nullptr; + } + fCanvas = new TCanvas("canv", "This is the canvas title", 1200, 500); + fCanvas->Draw(); + + TPad* pad1 = new TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97); + pad1->Divide(2, 1); + pad1->Draw(); + + pad1->cd(1); + pad1->cd(1)->SetLogy(); + pad1->cd(1)->SetRightMargin(0.09); + pad1->cd(1)->SetLeftMargin(0.15); + pad1->cd(1)->SetBottomMargin(0.15); + + TH1F* ht = GetTotalSpectrum(); + ht->SetLineColor(kBlack); + ht->SetFillStyle(4050); + ht->SetFillColor(kBlue - 10); + + TH1F* hm = GetMonochromaticSpectrum(); + hm->SetLineColor(kBlack); + hm->Scale(100); // renormalizing per 100eV-1 + + ht->Draw("hist"); + hm->Draw("hist same"); + + pad1->cd(2); + pad1->cd(2)->SetRightMargin(0.09); + pad1->cd(2)->SetLeftMargin(0.15); + pad1->cd(2)->SetBottomMargin(0.15); + + ht->Draw("hist"); + hm->Draw("hist same"); + + return fCanvas; +} + /////////////////////////////////////////////// /// \brief A helper method to initialize the internal class data members with the /// integrated flux for each solar ring. It will be called by TRestAxionSolarQCDFlux::Initialize. From b58c1f27d4513dba0e027ffa35813287025d996e Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Thu, 22 Jun 2023 10:11:47 +0200 Subject: [PATCH 03/48] Changed comments to HP versions --- inc/TRestAxionSolarHiddenPhotonFlux.h | 12 +++---- src/TRestAxionSolarHiddenPhotonFlux.cxx | 47 +++++++++++-------------- 2 files changed, 27 insertions(+), 32 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 929859a1..aae9caff 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -20,8 +20,8 @@ * For the list of contributors see $REST_PATH/CREDITS. * *************************************************************************/ -#ifndef _TRestAxionSolarQCDFlux -#define _TRestAxionSolarQCDFlux +#ifndef _TRestAxionSolarHiddenPhotonFlux +#define _TRestAxionSolarHiddenPhotonFlux #include #include @@ -125,10 +125,10 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { void PrintIntegratedRingFlux(); void PrintMonoChromaticFlux(); - TRestAxionSolarQCDFlux(); - TRestAxionSolarQCDFlux(const char* cfgFileName, std::string name = ""); - ~TRestAxionSolarQCDFlux(); + TRestAxionSolarHiddenPhotonFlux(); + TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, std::string name = ""); + ~TRestAxionSolarHiddenPhotonFlux(); - ClassDefOverride(TRestAxionSolarQCDFlux, 1); + ClassDefOverride(TRestAxionSolarHiddenPhotonFlux, 1); }; #endif diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 5f4a00af..fc565499 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -21,19 +21,14 @@ *************************************************************************/ ////////////////////////////////////////////////////////////////////////// -/// TRestAxionSolarQCDFlux will use a file in ASCII or binary format to initialize -/// a solar flux table that will describe the solar flux spectrum as a function +/// TRestAxionSolarHiddenPhotonFlux will use a file in ASCII or binary format to initialize +/// a solar flux table that will describe the solar hidden photon flux spectrum as a function /// of the solar radius. /// -/// This class may serve to load any generic flux definition that is independent -/// from the axion mass. However, since the design of the class was motivated to -/// reproduce the standard QCD axion flux, therefore the name of the class. -/// -/// Another scenario arises when the axion or an axion-like particle production -/// mechanism depends on its mass, and we may need to introduce a flux description -/// as the given in the class TRestAxionSolarHiddenPhotonFlux. Both classes are -/// prototyped by a pure base class TRestAxionSolarFlux that defines common methods -/// used to evaluate the flux, and generate Monte-Carlo events inside +/// This class loads the hidden photon flux that depends on the mass and kinetic mixing parameter. +/// For axion-like particle prodution independent of mass there is the class +/// TRestAxionSolarQCDFlux. Both classes are prototyped by a pure base class TRestAxionSolarFlux +/// that defines common methods used to evaluate the flux, and generate Monte-Carlo events inside /// TRestAxionGeneratorProcess. /// /// ### Basic use @@ -143,7 +138,7 @@ /// 2023-June: TRestAxionSolarHiddenPhotonFlux created by editing TRestAxionSolarQCDFlux /// Tomas O'Shea /// -/// \class TRestAxionSolarQCDFlux +/// \class TRestAxionSolarHiddenPhotonFlux /// \author Javier Galan /// ///
@@ -364,7 +359,7 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { /// \brief It builds a histogram with the continuum spectrum component. /// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. /// -TH1F* TRestAxionSolarQCDFlux::GetContinuumSpectrum() { +TH1F* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { if (fContinuumHist != nullptr) { delete fContinuumHist; fContinuumHist = nullptr; @@ -390,7 +385,7 @@ TH1F* TRestAxionSolarQCDFlux::GetContinuumSpectrum() { /// \brief It builds a histogram with the monochromatic spectrum component. /// The flux will be expressed in cm-2 s-1 eV-1. Binned in 1eV steps. /// -TH1F* TRestAxionSolarQCDFlux::GetMonochromaticSpectrum() { +TH1F* TRestAxionSolarHiddenPhotonFlux::GetMonochromaticSpectrum() { if (fMonoHist != nullptr) { delete fMonoHist; fMonoHist = nullptr; @@ -417,7 +412,7 @@ TH1F* TRestAxionSolarQCDFlux::GetMonochromaticSpectrum() { /// spectrum component. The flux will be expressed in cm-2 s-1 keV-1. /// Binned in 1eV steps. /// -TH1F* TRestAxionSolarQCDFlux::GetTotalSpectrum() { +TH1F* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { TH1F* hm = GetMonochromaticSpectrum(); TH1F* hc = GetContinuumSpectrum(); @@ -451,7 +446,7 @@ TH1F* TRestAxionSolarQCDFlux::GetTotalSpectrum() { /////////////////////////////////////////////// /// \brief It draws the contents of a .flux file. This method just receives the /// -TCanvas* TRestAxionSolarQCDFlux::DrawSolarFlux() { +TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { if (fCanvas != nullptr) { delete fCanvas; fCanvas = nullptr; @@ -494,9 +489,9 @@ TCanvas* TRestAxionSolarQCDFlux::DrawSolarFlux() { /////////////////////////////////////////////// /// \brief A helper method to initialize the internal class data members with the -/// integrated flux for each solar ring. It will be called by TRestAxionSolarQCDFlux::Initialize. +/// integrated flux for each solar ring. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. /// -void TRestAxionSolarQCDFlux::IntegrateSolarFluxes() { +void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { fFluxLineIntegrals.clear(); fTotalMonochromaticFlux = 0; @@ -523,7 +518,7 @@ void TRestAxionSolarQCDFlux::IntegrateSolarFluxes() { /////////////////////////////////////////////// /// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range /// -Double_t TRestAxionSolarQCDFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { +Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { if (eRange.X() == -1 && eRange.Y() == -1) { if (GetTotalFlux() == 0) IntegrateSolarFluxes(); return GetTotalFlux(); @@ -547,7 +542,7 @@ Double_t TRestAxionSolarQCDFlux::IntegrateFluxInRange(TVector2 eRange, Double_t /// \brief It returns a random solar radius position and energy according to the /// flux distributions defined inside the solar tables loaded in the class /// -std::pair TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius(TVector2 eRange, +std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, Double_t mass) { std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; @@ -582,7 +577,7 @@ std::pair TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius(T /////////////////////////////////////////////// /// \brief It prints on screen the table that has been loaded in memory /// -void TRestAxionSolarQCDFlux::PrintContinuumSolarTable() { +void TRestAxionSolarHiddenPhotonFlux::PrintContinuumSolarTable() { cout << "Continuum solar flux table: " << endl; cout << "--------------------------- " << endl; for (unsigned int n = 0; n < fFluxTable.size(); n++) { @@ -597,7 +592,7 @@ void TRestAxionSolarQCDFlux::PrintContinuumSolarTable() { /////////////////////////////////////////////// /// \brief It prints on screen the integrated solar flux per solar ring /// -void TRestAxionSolarQCDFlux::PrintIntegratedRingFlux() { +void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { cout << "Integrated solar flux per solar ring: " << endl; cout << "--------------------------- " << endl; /* @@ -610,7 +605,7 @@ void TRestAxionSolarQCDFlux::PrintIntegratedRingFlux() { /////////////////////////////////////////////// /// \brief It prints on screen the spectral lines loaded in memory /// -void TRestAxionSolarQCDFlux::PrintMonoChromaticFlux() { +void TRestAxionSolarHiddenPhotonFlux::PrintMonoChromaticFlux() { // cout << "Number of monochromatic lines: " << fFluxPerRadius.size() << endl; cout << "+++++++++++++++++++++++++++++++++++" << endl; for (auto const& line : fFluxLines) { @@ -623,9 +618,9 @@ void TRestAxionSolarQCDFlux::PrintMonoChromaticFlux() { } /////////////////////////////////////////////// -/// \brief Prints on screen the information about the metadata members of TRestAxionSolarQCDFlux +/// \brief Prints on screen the information about the metadata members of TRestAxionSolarHiddenPhotonFlux /// -void TRestAxionSolarQCDFlux::PrintMetadata() { +void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { TRestAxionSolarFlux::PrintMetadata(); if (fFluxDataFile != "") @@ -648,7 +643,7 @@ void TRestAxionSolarQCDFlux::PrintMetadata() { /// \brief It will create files with the continuum and spectral flux components to be used /// in a later ocasion. /// -void TRestAxionSolarQCDFlux::ExportTables(Bool_t ascii) { +void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { string rootFilename = TRestTools::GetFileNameRoot(fFluxDataFile); string path = REST_USER_PATH + "/export/"; From 17ac38fe97d11eb6d849b999c4f7afc64aae03a5 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Thu, 22 Jun 2023 08:15:14 +0000 Subject: [PATCH 04/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- .gitignore | 2 +- inc/TRestAxionSolarHiddenPhotonFlux.h | 1 - src/TRestAxionSolarHiddenPhotonFlux.cxx | 61 ++++++++++++------------- 3 files changed, 29 insertions(+), 35 deletions(-) diff --git a/.gitignore b/.gitignore index 58ad2261..9632e928 100644 --- a/.gitignore +++ b/.gitignore @@ -1,4 +1,4 @@ build *.root **/.DS_Store -*.json \ No newline at end of file +*.json diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index aae9caff..7551f2cf 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -26,7 +26,6 @@ #include #include - //! A metadata class to load tabulated solar hidden photon fluxes. Mass and coupling set to 1. class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { private: diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index fc565499..97c9ccab 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -112,9 +112,8 @@ /// standard format to be used in later occasions. /// /// \code -/// TRestAxionSolarHiddenPhotonFlux *sFlux = new TRestAxionSolarHiddenPhotonFlux("fluxes.rml", "HiddenPhoton") -/// sFlux->Initialize() -/// sFlux->ExportTables() +/// TRestAxionSolarHiddenPhotonFlux *sFlux = new TRestAxionSolarHiddenPhotonFlux("fluxes.rml", +/// "HiddenPhoton") sFlux->Initialize() sFlux->ExportTables() /// \endcode /// /// which will produce a binary table `.N200f` with the continuum flux. The filename root will be @@ -185,8 +184,7 @@ TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} /// inside the metadata members. /// Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - if (fFluxDataFile == "" || fWidthDataFile == "" || - fPlasmaFreqDataFile == "") return false; + if (fFluxDataFile == "" || fWidthDataFile == "" || fPlasmaFreqDataFile == "") return false; LoadContinuumFluxTable(); LoadWidthTable(); @@ -203,8 +201,9 @@ Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { /// void TRestAxionSolarHiddenPhotonFlux::LoadContinuumTable() { if (fFluxDataFile == "") { - RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" - << RESTendl; + RESTDebug + << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" + << RESTendl; return; } @@ -217,9 +216,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumTable() { if (!TRestTools::IsBinaryFile(fFluxDataFile)) { fluxTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; + RESTError << "File is not in binary format!" << RESTendl; } - + TRestTools::ReadBinaryTable(fullPathName, fluxTable); if (fluxTable.size() != 1000 && fluxTable[0].size() != 200) { @@ -236,7 +235,6 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumTable() { } } - /////////////////////////////////////////////// /// \brief A helper method to load the data file containing resonance width as a /// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. @@ -257,9 +255,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { if (!TRestTools::IsBinaryFile(fWidthDataFile)) { fluxTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; + RESTError << "File is not in binary format!" << RESTendl; } - + TRestTools::ReadBinaryTable(fullPathName, fluxTable); if (fluxTable.size() != 1000 && fluxTable[0].size() != 200) { @@ -276,15 +274,15 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { } } - /////////////////////////////////////////////// /// \brief A helper method to load the data file containing resonance width as a /// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. /// void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { if (fFluxDataFile == "") { - RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" - << RESTendl; + RESTDebug + << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" + << RESTendl; return; } @@ -297,9 +295,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { if (!TRestTools::IsBinaryFile(fWidthDataFile)) { fluxTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; + RESTError << "File is not in binary format!" << RESTendl; } - + TRestTools::ReadBinaryTable(fullPathName, fluxTable); if (fluxTable.size() != 1000 && fluxTable[0].size() != 1) { @@ -316,9 +314,8 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { } } - /////////////////////////////////////////////// -/// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the +/// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the /// kinetic mixing parameter and the hidden photon mass. /// void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { @@ -330,31 +327,29 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { for (unsigned int n = 0; n < fluxTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (wG)^2 ) - std::vector mass2Vector(200, pow(HiddenPhotonMass,2)); + std::vector mass2Vector(200, pow(HiddenPhotonMass, 2)); float wp = fPlasmaFreqTable[n].GetBinContent(1); - std::vector wp2Vector(200, pow(wp,2)); + std::vector wp2Vector(200, pow(wp, 2)); - TH1F* hMass = new TH1D("hMass", "hMass", 200, 0, 20) - TH1F* hWp = new TH1D("hWp", "hWp", 200, 0, 20) - TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); + TH1F* hMass = new TH1D("hMass", "hMass", 200, 0, 20) TH1F* hWp = + new TH1D("hWp", "hWp", 200, 0, 20) TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); - hMass->FillN(200, massVector); // m^2 hist - hWp->FillN(200, wpVector); // wp^2 hist - TH1F* hWg2 = fWidthTable[n] * fWidthTable[n]; // (omega Gamma)^2 + hMass->FillN(200, massVector); // m^2 hist + hWp->FillN(200, wpVector); // wp^2 hist + TH1F* hWg2 = fWidthTable[n] * fWidthTable[n]; // (omega Gamma)^2 - hMass->Add(hWp, -1); // (m2 - wp2) - hMass->Multiply(hMass); // (m2 - wp2)^2 - hmass->Add(hWg2); // (m2 - wp2)^2 - (wG)^2 + hMass->Add(hWp, -1); // (m2 - wp2) + hMass->Multiply(hMass); // (m2 - wp2)^2 + hmass->Add(hWg2); // (m2 - wp2)^2 - (wG)^2 TH1F* h = fWidthTable[n] * fContinuumTable[n]; h->Divide(hMass); - h->Scale(pow(HiddenPhotonMass,4) * pow(HiddenPhotonKineticMixing,2)); + h->Scale(pow(HiddenPhotonMass, 4) * pow(HiddenPhotonKineticMixing, 2)); fFluxTable.push_back(h); } } - /////////////////////////////////////////////// /// \brief It builds a histogram with the continuum spectrum component. /// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. @@ -543,7 +538,7 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, /// flux distributions defined inside the solar tables loaded in the class /// std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, - Double_t mass) { + Double_t mass) { std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); From 76b0c6d29ac58d56139b36b57f9ecce348e5a5eb Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Thu, 22 Jun 2023 10:37:29 +0200 Subject: [PATCH 05/48] Removed all monochromatic and .flux code --- inc/TRestAxionSolarHiddenPhotonFlux.h | 9 +- src/TRestAxionSolarHiddenPhotonFlux.cxx | 139 +----------------------- 2 files changed, 7 insertions(+), 141 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index aae9caff..3e1d4ee3 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -42,15 +42,12 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// The filename containing the resonance width (wGamma) std::string fWidthDataFile = ""; //< - /// The filename containing the plasma freqency (wp) table + /// The filename containing the plasma frequency (wp) table std::string fPlasmaFreqDataFile = ""; //< /// It will be used when loading `.flux` files to define the input file energy binsize in eV. Double_t fBinSize = 0; //< - /// It will be used when loading `.flux` files to define the threshold for peak identification - Double_t fPeakSigma = 0; //< - /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFluxTable; //! @@ -99,14 +96,13 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// It returns the total integrated flux at earth in cm-2 s-1 Double_t GetTotalFlux(Double_t mass = 0) override { - return fTotalContinuumFlux + fTotalMonochromaticFlux; + return fTotalContinuumFlux; } /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 TH1F* GetEnergySpectrum(Double_t m = 0) override { return GetTotalSpectrum(); } TH1F* GetContinuumSpectrum(); - TH1F* GetMonochromaticSpectrum(); TH1F* GetTotalSpectrum(); virtual TCanvas* DrawSolarFlux() override; @@ -123,7 +119,6 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { void PrintContinuumSolarTable(); void PrintIntegratedRingFlux(); - void PrintMonoChromaticFlux(); TRestAxionSolarHiddenPhotonFlux(); TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, std::string name = ""); diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index fc565499..7fc73db6 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -356,7 +356,7 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { /////////////////////////////////////////////// -/// \brief It builds a histogram with the continuum spectrum component. +/// \brief It builds a histogram with the continuum spectrum. /// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. /// TH1F* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { @@ -381,39 +381,12 @@ TH1F* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { return fContinuumHist; } -/////////////////////////////////////////////// -/// \brief It builds a histogram with the monochromatic spectrum component. -/// The flux will be expressed in cm-2 s-1 eV-1. Binned in 1eV steps. -/// -TH1F* TRestAxionSolarHiddenPhotonFlux::GetMonochromaticSpectrum() { - if (fMonoHist != nullptr) { - delete fMonoHist; - fMonoHist = nullptr; - } - - fMonoHist = new TH1F("MonochromaticHist", "", 20000, 0, 20); - for (const auto& x : fFluxLines) { - fMonoHist->Fill(x.first, x.second->Integral()); // cm-2 s-1 eV-1 - } - - fMonoHist->SetStats(0); - fMonoHist->GetXaxis()->SetTitle("Energy [keV]"); - fMonoHist->GetXaxis()->SetTitleSize(0.05); - fMonoHist->GetXaxis()->SetLabelSize(0.05); - fMonoHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 eV-1]"); - fMonoHist->GetYaxis()->SetTitleSize(0.05); - fMonoHist->GetYaxis()->SetLabelSize(0.05); - - return fMonoHist; -} /////////////////////////////////////////////// -/// \brief It builds a histogram adding the continuum and the monochromatic -/// spectrum component. The flux will be expressed in cm-2 s-1 keV-1. -/// Binned in 1eV steps. +/// \brief Same as GetContinuumSpectrum, the flux will be +/// expressed in cm-2 s-1 keV-1. Binned in 1eV steps. /// TH1F* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { - TH1F* hm = GetMonochromaticSpectrum(); TH1F* hc = GetContinuumSpectrum(); if (fTotalHist != nullptr) { @@ -428,10 +401,6 @@ TH1F* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { } } - for (int n = 0; n < hm->GetNbinsX(); n++) - // 1e-2 is the renormalization from 20000 bins to 200 bins - fTotalHist->SetBinContent(n + 1, fTotalHist->GetBinContent(n + 1) + 100 * hm->GetBinContent(n + 1)); - fTotalHist->SetStats(0); fTotalHist->GetXaxis()->SetTitle("Energy [keV]"); fTotalHist->GetXaxis()->SetTitleSize(0.05); @@ -443,66 +412,12 @@ TH1F* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { return fTotalHist; } -/////////////////////////////////////////////// -/// \brief It draws the contents of a .flux file. This method just receives the -/// -TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { - if (fCanvas != nullptr) { - delete fCanvas; - fCanvas = nullptr; - } - fCanvas = new TCanvas("canv", "This is the canvas title", 1200, 500); - fCanvas->Draw(); - - TPad* pad1 = new TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97); - pad1->Divide(2, 1); - pad1->Draw(); - - pad1->cd(1); - pad1->cd(1)->SetLogy(); - pad1->cd(1)->SetRightMargin(0.09); - pad1->cd(1)->SetLeftMargin(0.15); - pad1->cd(1)->SetBottomMargin(0.15); - - TH1F* ht = GetTotalSpectrum(); - ht->SetLineColor(kBlack); - ht->SetFillStyle(4050); - ht->SetFillColor(kBlue - 10); - - TH1F* hm = GetMonochromaticSpectrum(); - hm->SetLineColor(kBlack); - hm->Scale(100); // renormalizing per 100eV-1 - - ht->Draw("hist"); - hm->Draw("hist same"); - - pad1->cd(2); - pad1->cd(2)->SetRightMargin(0.09); - pad1->cd(2)->SetLeftMargin(0.15); - pad1->cd(2)->SetBottomMargin(0.15); - - ht->Draw("hist"); - hm->Draw("hist same"); - - return fCanvas; -} /////////////////////////////////////////////// /// \brief A helper method to initialize the internal class data members with the /// integrated flux for each solar ring. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. /// void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { - fFluxLineIntegrals.clear(); - fTotalMonochromaticFlux = 0; - - for (const auto& line : fFluxLines) { - fTotalMonochromaticFlux += line.second->Integral(); - fFluxLineIntegrals.push_back(fTotalMonochromaticFlux); - } - - for (unsigned int n = 0; n < fFluxLineIntegrals.size(); n++) - fFluxLineIntegrals[n] /= fTotalMonochromaticFlux; - fTotalContinuumFlux = 0.0; for (unsigned int n = 0; n < fFluxTable.size(); n++) { fTotalContinuumFlux += fFluxTable[n]->Integral() * 0.1; // We integrate in 100eV steps @@ -512,7 +427,6 @@ void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { for (unsigned int n = 0; n < fFluxTableIntegrals.size(); n++) fFluxTableIntegrals[n] /= fTotalContinuumFlux; - fFluxRatio = fTotalMonochromaticFlux / (fTotalContinuumFlux + fTotalMonochromaticFlux); } /////////////////////////////////////////////// @@ -525,9 +439,6 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, } Double_t flux = 0; - for (const auto& line : fFluxLines) - if (line.first > eRange.X() && line.first < eRange.Y()) flux += line.second->Integral(); - fTotalContinuumFlux = 0.0; for (unsigned int n = 0; n < fFluxTable.size(); n++) { flux += fFluxTable[n]->Integral(fFluxTable[n]->FindFixBin(eRange.X()), @@ -547,7 +458,7 @@ std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAn std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); - if (fTotalMonochromaticFlux == 0 || fRandom->Rndm() > fFluxRatio) { + if (fRandom->Rndm() > fFluxRatio) { // Continuum for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { if (rnd < fFluxTableIntegrals[r]) { @@ -560,16 +471,6 @@ std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAn return p; } } - } else { - // Monochromatic - int n = 0; - for (const auto& line : fFluxLines) { - if (rnd < fFluxLineIntegrals[n]) { - std::pair p = {line.first, line.second->GetRandom()}; - return p; - } - n++; - } } return result; } @@ -602,20 +503,6 @@ void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { */ } -/////////////////////////////////////////////// -/// \brief It prints on screen the spectral lines loaded in memory -/// -void TRestAxionSolarHiddenPhotonFlux::PrintMonoChromaticFlux() { - // cout << "Number of monochromatic lines: " << fFluxPerRadius.size() << endl; - cout << "+++++++++++++++++++++++++++++++++++" << endl; - for (auto const& line : fFluxLines) { - cout << "Energy : " << line.first << " keV" << endl; - cout << "-----------------" << endl; - for (int n = 0; n < line.second->GetNbinsX(); n++) - cout << "R : " << line.second->GetBinCenter(n + 1) - << " flux : " << line.second->GetBinContent(n + 1) << " cm-2 s-1" << endl; - } -} /////////////////////////////////////////////// /// \brief Prints on screen the information about the metadata members of TRestAxionSolarHiddenPhotonFlux @@ -634,13 +521,12 @@ void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Debug) { PrintContinuumSolarTable(); - PrintMonoChromaticFlux(); PrintIntegratedRingFlux(); } } /////////////////////////////////////////////// -/// \brief It will create files with the continuum and spectral flux components to be used +/// \brief It will create files with spectra to be used /// in a later ocasion. /// void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { @@ -668,19 +554,4 @@ void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { else TRestTools::ExportASCIITable(path + "/" + rootFilename + ".dat", table); } - - if (fFluxLines.size() > 0) { - std::vector> table; - for (const auto& x : fFluxLines) { - std::vector row; - row.push_back(x.first); - for (int n = 0; n < x.second->GetNbinsX(); n++) row.push_back(x.second->GetBinContent(n + 1)); - - table.push_back(row); - } - - TRestTools::TransposeTable(table); - - TRestTools::ExportASCIITable(path + "/" + rootFilename + ".spt", table); - } } From cd4b0e66994980310423b360f3f7dd3b0225f16b Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Thu, 22 Jun 2023 08:37:49 +0000 Subject: [PATCH 06/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarHiddenPhotonFlux.h | 4 +--- src/TRestAxionSolarHiddenPhotonFlux.cxx | 4 ---- 2 files changed, 1 insertion(+), 7 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 80059ddb..f41cb867 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -94,9 +94,7 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Bool_t LoadTables() override; /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux(Double_t mass = 0) override { - return fTotalContinuumFlux; - } + Double_t GetTotalFlux(Double_t mass = 0) override { return fTotalContinuumFlux; } /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 TH1F* GetEnergySpectrum(Double_t m = 0) override { return GetTotalSpectrum(); } diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index db100ef4..52caf875 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -376,7 +376,6 @@ TH1F* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { return fContinuumHist; } - /////////////////////////////////////////////// /// \brief Same as GetContinuumSpectrum, the flux will be /// expressed in cm-2 s-1 keV-1. Binned in 1eV steps. @@ -407,7 +406,6 @@ TH1F* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { return fTotalHist; } - /////////////////////////////////////////////// /// \brief A helper method to initialize the internal class data members with the /// integrated flux for each solar ring. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. @@ -421,7 +419,6 @@ void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { for (unsigned int n = 0; n < fFluxTableIntegrals.size(); n++) fFluxTableIntegrals[n] /= fTotalContinuumFlux; - } /////////////////////////////////////////////// @@ -498,7 +495,6 @@ void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { */ } - /////////////////////////////////////////////// /// \brief Prints on screen the information about the metadata members of TRestAxionSolarHiddenPhotonFlux /// From 4d7b5481d78495991a718e8c37f0ccc3e9e4f1d9 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Tue, 27 Jun 2023 10:52:45 +0200 Subject: [PATCH 07/48] Inlcuded mass dependence and set chi=1 --- inc/TRestAxionSolarFlux.h | 6 +++++ src/TRestAxionSolarHiddenPhotonFlux.cxx | 30 ++++++++++++++++--------- 2 files changed, 25 insertions(+), 11 deletions(-) diff --git a/inc/TRestAxionSolarFlux.h b/inc/TRestAxionSolarFlux.h index 73bcc00d..f417d713 100644 --- a/inc/TRestAxionSolarFlux.h +++ b/inc/TRestAxionSolarFlux.h @@ -38,6 +38,9 @@ class TRestAxionSolarFlux : public TRestMetadata { /// Axion coupling strength Double_t fCouplingStrength = 0; //< + /// Mass parameter + Double_t fMass = 0; //! + /// Seed used in random generator Int_t fSeed = 0; //< @@ -83,6 +86,9 @@ class TRestAxionSolarFlux : public TRestMetadata { Bool_t AreTablesLoaded() { return fTablesLoaded; } + Double_t GetMass() { return fMass; } + void SetMass(const Double_t &m ){ fMass = m; } + TH1F* GetFluxHistogram(std::string fname, Double_t binSize = 0.01); TCanvas* DrawFluxFile(std::string fname, Double_t binSize = 0.01); diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 52caf875..5b50bffd 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -84,7 +84,7 @@ /// /// \warning When the flux is loaded manually inside the `restRoot` interactive /// shell, or inside a macro or script, after metadata initialization, it is necessary -/// to call the method TRestAxionSolarHiddenPhotonFlux::LoadTables to trigger the tables +/// to call the method TRestAxionSolarHiddenPhotonFlux::LoadTables(mass) to trigger the tables /// initialization. /// /// ### Performing MonteCarlo tests using pre-loaded tables @@ -181,15 +181,19 @@ TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} /////////////////////////////////////////////// /// \brief It will load the tables in memory by using the filename information provided -/// inside the metadata members. +/// inside the metadata members, and calculate the solar flux for a given m. /// -Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { +Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables(Double_t mass) { if (fFluxDataFile == "" || fWidthDataFile == "" || fPlasmaFreqDataFile == "") return false; + SetMass(mass); + LoadContinuumFluxTable(); LoadWidthTable(); LoadPlasmaFreqTable(); + CalculateSolarFlux(); + IntegrateSolarFluxes(); return true; @@ -316,18 +320,18 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { /////////////////////////////////////////////// /// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the -/// kinetic mixing parameter and the hidden photon mass. +/// and the hidden photon mass for chi=1. /// void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { - if (!LoadTables()) { - RESTError << "CalculateSolarFlux. The component tables cannot be loaded." << RESTendl; + if (fMass == 0) { + RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; } for (unsigned int n = 0; n < fluxTable.size(); n++) { - // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (wG)^2 ) + // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - std::vector mass2Vector(200, pow(HiddenPhotonMass, 2)); + std::vector mass2Vector(200, pow(fMass, 2)); float wp = fPlasmaFreqTable[n].GetBinContent(1); std::vector wp2Vector(200, pow(wp, 2)); @@ -336,15 +340,15 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { hMass->FillN(200, massVector); // m^2 hist hWp->FillN(200, wpVector); // wp^2 hist - TH1F* hWg2 = fWidthTable[n] * fWidthTable[n]; // (omega Gamma)^2 + TH1F* hWg2 = fWidthTable[n] * fWidthTable[n]; // (w G)^2 hMass->Add(hWp, -1); // (m2 - wp2) hMass->Multiply(hMass); // (m2 - wp2)^2 - hmass->Add(hWg2); // (m2 - wp2)^2 - (wG)^2 + hmass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 TH1F* h = fWidthTable[n] * fContinuumTable[n]; h->Divide(hMass); - h->Scale(pow(HiddenPhotonMass, 4) * pow(HiddenPhotonKineticMixing, 2)); + h->Scale(pow(fMass, 4)); fFluxTable.push_back(h); } @@ -425,6 +429,8 @@ void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { /// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range /// Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { + SetMass(mass); + if (eRange.X() == -1 && eRange.Y() == -1) { if (GetTotalFlux() == 0) IntegrateSolarFluxes(); return GetTotalFlux(); @@ -447,6 +453,8 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, /// std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, Double_t mass) { + SetMass(mass); + std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); From 712ca971f15294c4e4a98fb2a3252b3c80660be9 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Tue, 27 Jun 2023 08:53:24 +0000 Subject: [PATCH 08/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarFlux.h | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/inc/TRestAxionSolarFlux.h b/inc/TRestAxionSolarFlux.h index f417d713..e52656a1 100644 --- a/inc/TRestAxionSolarFlux.h +++ b/inc/TRestAxionSolarFlux.h @@ -39,7 +39,7 @@ class TRestAxionSolarFlux : public TRestMetadata { Double_t fCouplingStrength = 0; //< /// Mass parameter - Double_t fMass = 0; //! + Double_t fMass = 0; //! /// Seed used in random generator Int_t fSeed = 0; //< @@ -87,7 +87,7 @@ class TRestAxionSolarFlux : public TRestMetadata { Bool_t AreTablesLoaded() { return fTablesLoaded; } Double_t GetMass() { return fMass; } - void SetMass(const Double_t &m ){ fMass = m; } + void SetMass(const Double_t& m) { fMass = m; } TH1F* GetFluxHistogram(std::string fname, Double_t binSize = 0.01); TCanvas* DrawFluxFile(std::string fname, Double_t binSize = 0.01); From 43aee1683469108c186179b514b7f4e60f081a9f Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Tue, 27 Jun 2023 11:50:58 +0200 Subject: [PATCH 09/48] Mass set only in loadtables --- inc/TRestAxionSolarHiddenPhotonFlux.h | 20 +++++++------------- src/TRestAxionSolarHiddenPhotonFlux.cxx | 17 ++++++----------- 2 files changed, 13 insertions(+), 24 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index f41cb867..87f8d540 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -26,14 +26,9 @@ #include #include -//! A metadata class to load tabulated solar hidden photon fluxes. Mass and coupling set to 1. +//! A metadata class to load tabulated solar hidden photon fluxes. Kinetic mixing set to 1. class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { private: - /// The hidden photon mass used for calculation - double HiddenPhotonMass; - - /// The value of the kinetic mixing parameter used for calculation - double HiddenPhotonKineticMixing; /// The filename containing the solar flux table with continuum spectrum std::string fFluxDataFile = ""; //< @@ -84,20 +79,19 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Bool_t isPlasmaFreqLoaded() { return fWpTable.size() > 0; } /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range - Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; + Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), - Double_t mass = 0) override; + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; - /// It defines how to read the solar tables at the inhereted class - Bool_t LoadTables() override; + /// It defines how to read the solar tables at the inhereted class for a given mass in eV + Bool_t LoadTables(Double_t mass) override; /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux(Double_t mass = 0) override { return fTotalContinuumFlux; } + Double_t GetTotalFlux() override { return fTotalContinuumFlux; } /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 - TH1F* GetEnergySpectrum(Double_t m = 0) override { return GetTotalSpectrum(); } + TH1F* GetEnergySpectrum() override { return GetTotalSpectrum(); } TH1F* GetContinuumSpectrum(); TH1F* GetTotalSpectrum(); diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 5b50bffd..0ff58605 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -21,7 +21,7 @@ *************************************************************************/ ////////////////////////////////////////////////////////////////////////// -/// TRestAxionSolarHiddenPhotonFlux will use a file in ASCII or binary format to initialize +/// TRestAxionSolarHiddenPhotonFlux will use a file in binary format to initialize /// a solar flux table that will describe the solar hidden photon flux spectrum as a function /// of the solar radius. /// @@ -44,11 +44,11 @@ /// for the range (0,20)keV in steps of 100eV. The table is provided as a binary table using /// `.N200f` extension. /// - *widthDataFile:* A table with 1000 rows representing the width of the hidden photon -/// resonant production for each solar ring from the center to the corona, and 200 columns +/// resonant production (wG) for each solar ring from the center to the corona, and 200 columns /// representing the width, measured in eV2, for the range (0,20)keV in steps of 100eV. The /// table is provided as a binary table using `.N200f` extension. /// - *plasmaFreqDataFile:* A table with 1000 rows and only 1 column representing the solar -/// plasma frequency for each solar ring from the center to the corona, measured in eV. The +/// plasma frequency (wp) for each solar ring from the center to the corona, measured in eV. The /// table is provided as a binary table using `.N1f` extension. /// /// Pre-generated solar axion flux tables will be available at the @@ -428,9 +428,7 @@ void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { /////////////////////////////////////////////// /// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range /// -Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { - SetMass(mass); - +Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) { if (eRange.X() == -1 && eRange.Y() == -1) { if (GetTotalFlux() == 0) IntegrateSolarFluxes(); return GetTotalFlux(); @@ -451,11 +449,8 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, /// \brief It returns a random solar radius position and energy according to the /// flux distributions defined inside the solar tables loaded in the class /// -std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, - Double_t mass) { - SetMass(mass); - - std::pair result = {0, 0}; +std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { + std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); if (fRandom->Rndm() > fFluxRatio) { From d577a5d399b2bf1a17405740040ba4ffb4279c2f Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Tue, 27 Jun 2023 09:51:16 +0000 Subject: [PATCH 10/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarHiddenPhotonFlux.h | 1 - src/TRestAxionSolarHiddenPhotonFlux.cxx | 2 +- 2 files changed, 1 insertion(+), 2 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 87f8d540..2b6e51fb 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -29,7 +29,6 @@ //! A metadata class to load tabulated solar hidden photon fluxes. Kinetic mixing set to 1. class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { private: - /// The filename containing the solar flux table with continuum spectrum std::string fFluxDataFile = ""; //< diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 0ff58605..1f3ebf57 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -450,7 +450,7 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) /// flux distributions defined inside the solar tables loaded in the class /// std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { - std::pair result = {0, 0}; + std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); if (fRandom->Rndm() > fFluxRatio) { From ac0aa28aaf490f63ae9133da157f0f7a249ba8b8 Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Thu, 31 Aug 2023 12:52:21 +0100 Subject: [PATCH 11/48] created hidden photon plot code --- data | 2 +- .../solarFlux/solarPlotHiddenPhoton.py | 187 ++++++++++++++++++ src/TRestAxionSolarHiddenPhotonFlux.cxx | 3 +- 3 files changed, 190 insertions(+), 2 deletions(-) mode change 160000 => 120000 data create mode 100755 pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py diff --git a/data b/data deleted file mode 160000 index 957d9fc5..00000000 --- a/data +++ /dev/null @@ -1 +0,0 @@ -Subproject commit 957d9fc5e24d2e5aef97cfd1f99982f2c3a07a98 diff --git a/data b/data new file mode 120000 index 00000000..95fc0d20 --- /dev/null +++ b/data @@ -0,0 +1 @@ +../axionlib-data \ No newline at end of file diff --git a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py new file mode 100755 index 00000000..bd68972e --- /dev/null +++ b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py @@ -0,0 +1,187 @@ +#!/usr/bin/python3 + +import math +import ROOT +from ROOT import ( + TChain, + TFile, + TTree, + TCanvas, + TPad, + TRandom3, + TH1D, + TH2D, + TH3D, + TProfile, + TProfile2D, + TProfile3D, + TGraph, + TGraph2D, + TF1, + TF2, + TF3, + TFormula, + TLorentzVector, + TVector3, +) + +import argparse + +parser = argparse.ArgumentParser() +parser.add_argument("--rml", dest="rmlfile", type=str, help="The input RML file .rml") +parser.add_argument( + "--out", + dest="outfname", + type=str, + help="The output filename in png,pdf,C or any other ROOT accepted format", +) +parser.add_argument( + "--fluxname", + dest="fluxname", + type=str, + help="The name of the flux definition to be chosen from the RML", +) +parser.add_argument( + "--N", dest="samples", type=int, help="The number of generated particles" +) +parser.add_argument( + "--m", dest="mass", type=float, help="Hidden photon mass" +) +args = parser.parse_args() + +if mass == 0: + print("Hidden photon mass not specified!!") + print("Specify with argument --m") + quit() + +rmlfile = "fluxes.rml" +if args.rmlfile != None: + rmlfile = args.rmlfile + +outfname = "flux.png" +if args.outfname != None: + outfname = args.outfname + +fluxname = "combined" +if args.fluxname != None: + fluxname = args.fluxname + + +samples = 20000 +if args.samples != None: + samples = args.samples + +validation = True +if ( + rmlfile == "fluxes.rml" + and fluxname == "combined" + and outfname == "flux.png" + and samples == 20000 +): + validation = True + +ROOT.gSystem.Load("libRestFramework.so") +ROOT.gSystem.Load("libRestAxion.so") + +c1 = TCanvas("c1", "My canvas", 800, 700) +c1.GetFrame().SetBorderSize(6) +c1.GetFrame().SetBorderMode(-1) + +pad1 = TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97) +pad1.Divide(2, 2) +pad1.Draw() + +combinedFlux = ROOT.TRestAxionSolarHiddenPhotonFlux(rmlfile, fluxname) +combinedFlux.Initialize() +combinedFlux.PrintMetadata() + +if combinedFlux.GetError(): + print(combinedFlux.GetErrorMessage()) + print("\nSolar flux initialization failed! Exit code : 101") + exit(101) + +comb_spt = TH2D("comb_spt", "Energy versus solar radius", 20000, 0, 20, 100, 0, 1) +for x in range(samples): + x = combinedFlux.GetRandomEnergyAndRadius(mass) + comb_spt.Fill(x[0], x[1]) + +rnd = TRandom3(0) +solarDisk = TH2D("solar_disk", "SolarDisk", 120, -1.2, 1.2, 120, -1.2, 1.2) +for x in range(samples): + angle = rnd.Rndm() * 2 * math.pi + x = combinedFlux.GetRandomEnergyAndRadius(mass) + + solarDisk.Fill(x[1] * math.cos(angle), x[1] * math.sin(angle)) + +pad1.cd(1) +pad1.cd(1).SetRightMargin(0.09) +pad1.cd(1).SetLeftMargin(0.15) +pad1.cd(1).SetBottomMargin(0.15) + +comb_spt.SetStats(0) +comb_spt.GetXaxis().SetTitle("Energy [keV]") +comb_spt.GetXaxis().SetTitleSize(0.05) +comb_spt.GetXaxis().SetLabelSize(0.05) +comb_spt.GetYaxis().SetTitle("Solar radius") +comb_spt.GetYaxis().SetTitleSize(0.05) +comb_spt.GetYaxis().SetLabelSize(0.05) +comb_spt.Draw("colz") + +pad1.cd(2) +pad1.cd(2).SetLogy() +pad1.cd(2).SetRightMargin(0.09) +pad1.cd(2).SetLeftMargin(0.15) +pad1.cd(2).SetBottomMargin(0.15) +enSpt = comb_spt.ProjectionX() +enSpt.SetTitle("Energy spectrum") +enSpt.GetYaxis().SetTitleSize(0.05) +enSpt.SetStats(0) +enSpt.SetFillStyle(4050) +enSpt.SetFillColor(ROOT.kBlue - 9) +enSpt.SetLineColor(ROOT.kBlack) +enSpt.Draw() + +pad1.cd(3) +pad1.cd(3).SetRightMargin(0.09) +pad1.cd(3).SetLeftMargin(0.15) +pad1.cd(3).SetBottomMargin(0.15) +rSpt = comb_spt.ProjectionY() +rSpt.SetTitle("Radial distribution") +rSpt.GetYaxis().SetTitleSize(0.05) +rSpt.SetStats(0) +rSpt.SetFillStyle(4050) +rSpt.SetFillColor(ROOT.kBlue - 9) +rSpt.SetLineColor(ROOT.kBlack) +rSpt.Draw() + +pad1.cd(4) +pad1.cd(4).SetRightMargin(0.09) +pad1.cd(4).SetLeftMargin(0.15) +pad1.cd(4).SetBottomMargin(0.15) +solarDisk.SetStats(0) +solarDisk.GetXaxis().SetTitle("X") +solarDisk.GetXaxis().SetTitleSize(0.05) +solarDisk.GetXaxis().SetLabelSize(0.05) +solarDisk.GetYaxis().SetTitle("Y") +solarDisk.GetYaxis().SetTitleOffset(1) +solarDisk.GetYaxis().SetTitleSize(0.05) +solarDisk.GetYaxis().SetLabelSize(0.05) +solarDisk.Draw("colz") + +c1.Print(outfname) +print("Generated file : " + outfname) + +print("\nMaximum energy bin is " + str(enSpt.GetMaximumBin())) +if validation: + if enSpt.GetMaximumBin() != 8001: + print("\nMaximum Bin is not the expected one (8001)! Exit code : 1") + exit(1) + +print("\nMaximum radius bin is " + str(rSpt.GetMaximumBin())) + +if validation: + if rSpt.GetMaximumBin() != 25: + print("\nMaximum Bin is not the expected one (25)! Exit code : 2") + exit(2) + +exit(0) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 1f3ebf57..15cd0b65 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -449,7 +449,8 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) /// \brief It returns a random solar radius position and energy according to the /// flux distributions defined inside the solar tables loaded in the class /// -std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { +std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, Double_t HPmass) { + LoadTables(HPmass); // load tables with specified hidden photon mass std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); From 8a7990f237f1238aff61e530f4e9ff530251da4f Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Thu, 31 Aug 2023 11:55:50 +0000 Subject: [PATCH 12/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py | 10 ++++------ src/TRestAxionSolarHiddenPhotonFlux.cxx | 5 +++-- 2 files changed, 7 insertions(+), 8 deletions(-) diff --git a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py index bd68972e..e80f742d 100755 --- a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py +++ b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py @@ -44,15 +44,13 @@ parser.add_argument( "--N", dest="samples", type=int, help="The number of generated particles" ) -parser.add_argument( - "--m", dest="mass", type=float, help="Hidden photon mass" -) +parser.add_argument("--m", dest="mass", type=float, help="Hidden photon mass") args = parser.parse_args() if mass == 0: - print("Hidden photon mass not specified!!") - print("Specify with argument --m") - quit() + print("Hidden photon mass not specified!!") + print("Specify with argument --m") + quit() rmlfile = "fluxes.rml" if args.rmlfile != None: diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 15cd0b65..6acf83c7 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -449,8 +449,9 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) /// \brief It returns a random solar radius position and energy according to the /// flux distributions defined inside the solar tables loaded in the class /// -std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, Double_t HPmass) { - LoadTables(HPmass); // load tables with specified hidden photon mass +std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, + Double_t HPmass) { + LoadTables(HPmass); // load tables with specified hidden photon mass std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); From f81afa57a67d04757d7021d6e7f9c94affe8629d Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Tue, 5 Sep 2023 07:35:35 +0100 Subject: [PATCH 13/48] fixed args error --- pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py | 4 +++- 1 file changed, 3 insertions(+), 1 deletion(-) diff --git a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py index e80f742d..ecf4bcb6 100755 --- a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py +++ b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py @@ -47,7 +47,9 @@ parser.add_argument("--m", dest="mass", type=float, help="Hidden photon mass") args = parser.parse_args() -if mass == 0: +if args.mass != None: + mass = args.mass +else: print("Hidden photon mass not specified!!") print("Specify with argument --m") quit() From a81dcb44699525a760283b2e547bfd44efd071d9 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Tue, 5 Sep 2023 06:59:21 +0000 Subject: [PATCH 14/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py index ecf4bcb6..88ceca53 100755 --- a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py +++ b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py @@ -48,7 +48,7 @@ args = parser.parse_args() if args.mass != None: - mass = args.mass + mass = args.mass else: print("Hidden photon mass not specified!!") print("Specify with argument --m") From fdedb14c7c101defac90e33c3912f6675c475126 Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Wed, 6 Sep 2023 12:02:04 +0100 Subject: [PATCH 15/48] fixing bugs --- inc/TRestAxionSolarFlux.h | 2 +- inc/TRestAxionSolarHiddenPhotonFlux.h | 14 ++++++++------ inc/TRestAxionSolarQCDFlux.h | 2 +- 3 files changed, 10 insertions(+), 8 deletions(-) diff --git a/inc/TRestAxionSolarFlux.h b/inc/TRestAxionSolarFlux.h index e52656a1..1d068863 100644 --- a/inc/TRestAxionSolarFlux.h +++ b/inc/TRestAxionSolarFlux.h @@ -58,7 +58,7 @@ class TRestAxionSolarFlux : public TRestMetadata { TRestAxionSolarFlux(const char* cfgFileName, std::string name = ""); /// It defines how to read the solar tables at the inhereted class - virtual Bool_t LoadTables() = 0; + virtual Bool_t LoadTables(Double_t mass = 0) = 0; public: /// It is required in order to load solar flux tables into memory diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 2b6e51fb..2cc4821b 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -45,16 +45,18 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { std::vector fFluxTable; //! /// The tabulated resonance width TH1F(200,0,20)keV in eV2 versus solar radius - std::vector fWidthTable; //! + std::vector fWGammaTable; //! /// The solar plasma frequency vector in eV versus solar radius - std::vector fPlasmaFreqTable; //! + std::vector fWpTable; //! /// The total solar flux TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFullFluxTable; //! /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) std::vector fFluxTableIntegrals; //! + + std::vector fTotalContinuumFlux; //! /// A pointer to the continuum spectrum histogram TH1F* fContinuumHist = nullptr; //! @@ -78,19 +80,19 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Bool_t isPlasmaFreqLoaded() { return fWpTable.size() > 0; } /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range - Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; + Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; /// It defines how to read the solar tables at the inhereted class for a given mass in eV Bool_t LoadTables(Double_t mass) override; /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux() override { return fTotalContinuumFlux; } + Double_t GetTotalFlux(Double_t mass = 0) override { return fTotalContinuumFlux; } /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 - TH1F* GetEnergySpectrum() override { return GetTotalSpectrum(); } + TH1F* GetEnergySpectrum(Double_t m = 0) override { return GetTotalSpectrum(); } TH1F* GetContinuumSpectrum(); TH1F* GetTotalSpectrum(); diff --git a/inc/TRestAxionSolarQCDFlux.h b/inc/TRestAxionSolarQCDFlux.h index 373eab33..240fd395 100644 --- a/inc/TRestAxionSolarQCDFlux.h +++ b/inc/TRestAxionSolarQCDFlux.h @@ -91,7 +91,7 @@ class TRestAxionSolarQCDFlux : public TRestAxionSolarFlux { Double_t mass = 0) override; /// It defines how to read the solar tables at the inhereted class - Bool_t LoadTables() override; + Bool_t LoadTables(Double_t mass = 0) override; /// It returns the total integrated flux at earth in cm-2 s-1 Double_t GetTotalFlux(Double_t mass = 0) override { From 98136de1cba4aa97c220f246a6058ba5b8543039 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Wed, 6 Sep 2023 11:03:19 +0000 Subject: [PATCH 16/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarHiddenPhotonFlux.h | 5 +++-- 1 file changed, 3 insertions(+), 2 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 2cc4821b..eb1c18ea 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -55,7 +55,7 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) std::vector fFluxTableIntegrals; //! - + std::vector fTotalContinuumFlux; //! /// A pointer to the continuum spectrum histogram @@ -83,7 +83,8 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), + Double_t mass = 0) override; /// It defines how to read the solar tables at the inhereted class for a given mass in eV Bool_t LoadTables(Double_t mass) override; From c0758b2cdd14c51582b7021905600613bc7fb947 Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Wed, 6 Sep 2023 12:12:50 +0100 Subject: [PATCH 17/48] fixing bugs again --- inc/TRestAxionSolarHiddenPhotonFlux.h | 3 ++- 1 file changed, 2 insertions(+), 1 deletion(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index eb1c18ea..5eaf7a9e 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -56,7 +56,8 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) std::vector fFluxTableIntegrals; //! - std::vector fTotalContinuumFlux; //! + /// Total solar flux for monochromatic contributions + Double_t fTotalContinuumFlux = 0; //! /// A pointer to the continuum spectrum histogram TH1F* fContinuumHist = nullptr; //! From 0a1f729aca99ce9ad4499d6d8a93465ff7e034ee Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Wed, 6 Sep 2023 12:44:04 +0100 Subject: [PATCH 18/48] fixing bugs again --- inc/TRestAxionSolarHiddenPhotonFlux.h | 8 +++++++- src/TRestAxionSolarHiddenPhotonFlux.cxx | 10 +--------- src/TRestAxionSolarQCDFlux.cxx | 2 +- 3 files changed, 9 insertions(+), 11 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 5eaf7a9e..8d8cec56 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -89,7 +89,13 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// It defines how to read the solar tables at the inhereted class for a given mass in eV Bool_t LoadTables(Double_t mass) override; - + + void LoadContinuumTable(); + void LoadWidthTable(); + void LoadPlasmaFreqTable(); + + // calculate solar HP flux from the 3 tables and mass + void CalculateSolarFlux(); /// It returns the total integrated flux at earth in cm-2 s-1 Double_t GetTotalFlux(Double_t mass = 0) override { return fTotalContinuumFlux; } diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 6acf83c7..2b3881f1 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -428,7 +428,7 @@ void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { /////////////////////////////////////////////// /// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range /// -Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) { +Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { if (eRange.X() == -1 && eRange.Y() == -1) { if (GetTotalFlux() == 0) IntegrateSolarFluxes(); return GetTotalFlux(); @@ -455,8 +455,6 @@ std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAn std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); - if (fRandom->Rndm() > fFluxRatio) { - // Continuum for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { if (rnd < fFluxTableIntegrals[r]) { Double_t energy = fFluxTable[r]->GetRandom(); @@ -466,7 +464,6 @@ std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAn Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.01; std::pair p = {energy, radius}; return p; - } } } return result; @@ -506,12 +503,7 @@ void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { TRestAxionSolarFlux::PrintMetadata(); - if (fFluxDataFile != "") - RESTMetadata << " - Solar axion flux datafile (continuum) : " << fFluxDataFile << RESTendl; - if (fFluxSptFile != "") - RESTMetadata << " - Solar axion flux datafile (monochromatic) : " << fFluxSptFile << RESTendl; RESTMetadata << "-------" << RESTendl; - RESTMetadata << " - Total monochromatic flux : " << fTotalMonochromaticFlux << " cm-2 s-1" << RESTendl; RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; RESTMetadata << "++++++++++++++++++" << RESTendl; diff --git a/src/TRestAxionSolarQCDFlux.cxx b/src/TRestAxionSolarQCDFlux.cxx index 5cdd2d46..c64969df 100644 --- a/src/TRestAxionSolarQCDFlux.cxx +++ b/src/TRestAxionSolarQCDFlux.cxx @@ -249,7 +249,7 @@ TRestAxionSolarQCDFlux::~TRestAxionSolarQCDFlux() {} /// \brief It will load the tables in memory by using the filename information provided /// inside the metadata members. /// -Bool_t TRestAxionSolarQCDFlux::LoadTables() { +Bool_t TRestAxionSolarQCDFlux::LoadTables(Double_t mass) { if (fFluxDataFile == "" && fFluxSptFile == "") return false; if (TRestTools::GetFileNameExtension(fFluxDataFile) == "flux") { From 1b71f052b821f8d1eccf112f1e073943b71b11ed Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Wed, 6 Sep 2023 11:44:55 +0000 Subject: [PATCH 19/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarHiddenPhotonFlux.h | 4 ++-- src/TRestAxionSolarHiddenPhotonFlux.cxx | 18 +++++++++--------- 2 files changed, 11 insertions(+), 11 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 8d8cec56..548f914a 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -89,11 +89,11 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// It defines how to read the solar tables at the inhereted class for a given mass in eV Bool_t LoadTables(Double_t mass) override; - + void LoadContinuumTable(); void LoadWidthTable(); void LoadPlasmaFreqTable(); - + // calculate solar HP flux from the 3 tables and mass void CalculateSolarFlux(); /// It returns the total integrated flux at earth in cm-2 s-1 diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 2b3881f1..3520095e 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -455,15 +455,15 @@ std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAn std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); - for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { - if (rnd < fFluxTableIntegrals[r]) { - Double_t energy = fFluxTable[r]->GetRandom(); - if (eRange.X() != -1 && eRange.Y() != -1) { - if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); - } - Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.01; - std::pair p = {energy, radius}; - return p; + for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { + if (rnd < fFluxTableIntegrals[r]) { + Double_t energy = fFluxTable[r]->GetRandom(); + if (eRange.X() != -1 && eRange.Y() != -1) { + if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); + } + Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.01; + std::pair p = {energy, radius}; + return p; } } return result; From 3712ce27fd09c74770d4fbf276aaed4c3625f836 Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Wed, 6 Sep 2023 12:58:14 +0100 Subject: [PATCH 20/48] fixing bugs pt.4 --- inc/TRestAxionSolarHiddenPhotonFlux.h | 11 +++++++---- src/TRestAxionSolarHiddenPhotonFlux.cxx | 13 +++++++------ 2 files changed, 14 insertions(+), 10 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 548f914a..be3216ad 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -43,12 +43,15 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFluxTable; //! + + /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fContinuumTable; //! /// The tabulated resonance width TH1F(200,0,20)keV in eV2 versus solar radius - std::vector fWGammaTable; //! + std::vector fWidthTable; //! /// The solar plasma frequency vector in eV versus solar radius - std::vector fWpTable; //! + std::vector fPlasmaFreqTable; //! /// The total solar flux TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFullFluxTable; //! @@ -75,10 +78,10 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } /// It returns true if width table was loaded - Bool_t isWidthTableLoaded() { return fWGammaTable.size() > 0; } + Bool_t isWidthTableLoaded() { return fWidthTable.size() > 0; } /// It returns true if plasma frequency table was loaded - Bool_t isPlasmaFreqLoaded() { return fWpTable.size() > 0; } + Bool_t isPlasmaFreqLoaded() { return fPlasmaFreqTable.size() > 0; } /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 3520095e..0a5ffdfc 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -323,20 +323,21 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { /// and the hidden photon mass for chi=1. /// void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { - if (fMass == 0) { + if (GetMass() == 0) { RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; } - + Double_t mass = GetMass() for (unsigned int n = 0; n < fluxTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - std::vector mass2Vector(200, pow(fMass, 2)); + std::vector mass2Vector(200, pow(mass, 2)); float wp = fPlasmaFreqTable[n].GetBinContent(1); std::vector wp2Vector(200, pow(wp, 2)); - TH1F* hMass = new TH1D("hMass", "hMass", 200, 0, 20) TH1F* hWp = - new TH1D("hWp", "hWp", 200, 0, 20) TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); + TH1F* hMass = new TH1D("hMass", "hMass", 200, 0, 20); + TH1F* hWp = new TH1D("hWp", "hWp", 200, 0, 20); + TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); hMass->FillN(200, massVector); // m^2 hist hWp->FillN(200, wpVector); // wp^2 hist @@ -348,7 +349,7 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { TH1F* h = fWidthTable[n] * fContinuumTable[n]; h->Divide(hMass); - h->Scale(pow(fMass, 4)); + h->Scale(pow(mass, 4)); fFluxTable.push_back(h); } From b261cc0cfc6d8e98daf94cea7fec5ab824d7845e Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Wed, 6 Sep 2023 13:08:43 +0100 Subject: [PATCH 21/48] fixing bugs pt.5 --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 0a5ffdfc..ed379a51 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -327,7 +327,7 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; } - Double_t mass = GetMass() + Double_t mass = GetMass(); for (unsigned int n = 0; n < fluxTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) From 74e04fbc6c8b356a1cb035ca76c150e724eb2c20 Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Wed, 6 Sep 2023 13:16:11 +0100 Subject: [PATCH 22/48] fixing bugs pt.6 --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index ed379a51..7b04589c 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -328,7 +328,7 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { return; } Double_t mass = GetMass(); - for (unsigned int n = 0; n < fluxTable.size(); n++) { + for (unsigned int n = 0; n < fContinuumTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) std::vector mass2Vector(200, pow(mass, 2)); From 3871b57b210903373f70e9381cf4664732854890 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Wed, 6 Sep 2023 12:16:40 +0000 Subject: [PATCH 23/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarHiddenPhotonFlux.h | 2 +- src/TRestAxionSolarHiddenPhotonFlux.cxx | 2 +- 2 files changed, 2 insertions(+), 2 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index be3216ad..502983af 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -43,7 +43,7 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFluxTable; //! - + /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fContinuumTable; //! diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 7b04589c..5fee2462 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -327,7 +327,7 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; } - Double_t mass = GetMass(); + Double_t mass = GetMass(); for (unsigned int n = 0; n < fContinuumTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) From 1abf76653ab8e16a5089d2e7def12257b05178c1 Mon Sep 17 00:00:00 2001 From: Tomas OShea Date: Thu, 7 Sep 2023 11:25:58 +0200 Subject: [PATCH 24/48] fixed bugs, now compiles --- inc/TRestAxionSolarHiddenPhotonFlux.h | 6 +-- src/TRestAxionSolarHiddenPhotonFlux.cxx | 63 +++++++++++++++++++++---- 2 files changed, 56 insertions(+), 13 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 502983af..05dbc4eb 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -43,7 +43,7 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFluxTable; //! - + /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fContinuumTable; //! @@ -92,11 +92,11 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// It defines how to read the solar tables at the inhereted class for a given mass in eV Bool_t LoadTables(Double_t mass) override; - + void LoadContinuumTable(); void LoadWidthTable(); void LoadPlasmaFreqTable(); - + // calculate solar HP flux from the 3 tables and mass void CalculateSolarFlux(); /// It returns the total integrated flux at earth in cm-2 s-1 diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 5fee2462..7984838f 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -331,23 +331,27 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { for (unsigned int n = 0; n < fContinuumTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - std::vector mass2Vector(200, pow(mass, 2)); - float wp = fPlasmaFreqTable[n].GetBinContent(1); - std::vector wp2Vector(200, pow(wp, 2)); + vector mass2Vector(200, pow(mass, 2)); + double wp = fPlasmaFreqTable[n]->GetBinContent(1); + vector wp2Vector(200, pow(wp, 2)); + vector weights(200, 1); - TH1F* hMass = new TH1D("hMass", "hMass", 200, 0, 20); - TH1F* hWp = new TH1D("hWp", "hWp", 200, 0, 20); + TH1F* hMass = new TH1F("hMass", "hMass", 200, 0, 20); + TH1F* hWp = new TH1F("hWp", "hWp", 200, 0, 20); TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); + hWg2->Multiply(hWg2); // (w G)^2 - hMass->FillN(200, massVector); // m^2 hist - hWp->FillN(200, wpVector); // wp^2 hist - TH1F* hWg2 = fWidthTable[n] * fWidthTable[n]; // (w G)^2 + //hMass->FillN(200, mass2Vector); // m^2 hist + hMass->FillN(200, mass2Vector.data(), weights.data()); // m^2 hist + //hWp->FillN(200, wp2Vector); // wp^2 hist + hWp->FillN(200, wp2Vector.data(), weights.data()); // wp^2 hist hMass->Add(hWp, -1); // (m2 - wp2) hMass->Multiply(hMass); // (m2 - wp2)^2 - hmass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 + hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 - TH1F* h = fWidthTable[n] * fContinuumTable[n]; + TH1F* h = (TH1F*)fWidthTable[n]->Clone(); + h->Multiply(fContinuumTable[n]); h->Divide(hMass); h->Scale(pow(mass, 4)); @@ -544,3 +548,42 @@ void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { TRestTools::ExportASCIITable(path + "/" + rootFilename + ".dat", table); } } + +/////////////////////////////////////////////// +/// \brief It draws the contents of a .flux file. This method just receives the +/// +TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { + if (fCanvas != nullptr) { + delete fCanvas; + fCanvas = nullptr; + } + fCanvas = new TCanvas("canv", "This is the canvas title", 1200, 500); + fCanvas->Draw(); + + TPad* pad1 = new TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97); + pad1->Divide(2, 1); + pad1->Draw(); + + pad1->cd(1); + pad1->cd(1)->SetLogy(); + pad1->cd(1)->SetRightMargin(0.09); + pad1->cd(1)->SetLeftMargin(0.15); + pad1->cd(1)->SetBottomMargin(0.15); + + TH1F* ht = GetTotalSpectrum(); + ht->SetLineColor(kBlack); + ht->SetFillStyle(4050); + ht->SetFillColor(kBlue - 10); + + ht->Draw("hist"); + + pad1->cd(2); + pad1->cd(2)->SetRightMargin(0.09); + pad1->cd(2)->SetLeftMargin(0.15); + pad1->cd(2)->SetBottomMargin(0.15); + + ht->Draw("hist"); + + return fCanvas; +} + From 18850772174817ff83c7f1e55bf4fe52937b33b4 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Thu, 7 Sep 2023 09:26:51 +0000 Subject: [PATCH 25/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarHiddenPhotonFlux.h | 6 +++--- src/TRestAxionSolarHiddenPhotonFlux.cxx | 11 +++++------ 2 files changed, 8 insertions(+), 9 deletions(-) diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 05dbc4eb..502983af 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -43,7 +43,7 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFluxTable; //! - + /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fContinuumTable; //! @@ -92,11 +92,11 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// It defines how to read the solar tables at the inhereted class for a given mass in eV Bool_t LoadTables(Double_t mass) override; - + void LoadContinuumTable(); void LoadWidthTable(); void LoadPlasmaFreqTable(); - + // calculate solar HP flux from the 3 tables and mass void CalculateSolarFlux(); /// It returns the total integrated flux at earth in cm-2 s-1 diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 7984838f..fe285b04 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -339,12 +339,12 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { TH1F* hMass = new TH1F("hMass", "hMass", 200, 0, 20); TH1F* hWp = new TH1F("hWp", "hWp", 200, 0, 20); TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); - hWg2->Multiply(hWg2); // (w G)^2 + hWg2->Multiply(hWg2); // (w G)^2 - //hMass->FillN(200, mass2Vector); // m^2 hist - hMass->FillN(200, mass2Vector.data(), weights.data()); // m^2 hist - //hWp->FillN(200, wp2Vector); // wp^2 hist - hWp->FillN(200, wp2Vector.data(), weights.data()); // wp^2 hist + // hMass->FillN(200, mass2Vector); // m^2 hist + hMass->FillN(200, mass2Vector.data(), weights.data()); // m^2 hist + // hWp->FillN(200, wp2Vector); // wp^2 hist + hWp->FillN(200, wp2Vector.data(), weights.data()); // wp^2 hist hMass->Add(hWp, -1); // (m2 - wp2) hMass->Multiply(hMass); // (m2 - wp2)^2 @@ -586,4 +586,3 @@ TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { return fCanvas; } - From b4984f9648cc0442c94efae675fb893358af9436 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Fri, 8 Sep 2023 15:54:37 +0200 Subject: [PATCH 26/48] changed how mass is set for hidden photon --- flux.png | Bin 0 -> 19725 bytes .../solarFlux/solarPlotHiddenPhoton.py | 27 ++++++------------ 2 files changed, 9 insertions(+), 18 deletions(-) create mode 100644 flux.png diff --git a/flux.png b/flux.png new file mode 100644 index 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type=int, help="The number of generated particles" ) -parser.add_argument("--m", dest="mass", type=float, help="Hidden photon mass") +parser.add_argument( + "--mass", dest="mass", type=float, help="Hidden photon mass [eV]" +) + args = parser.parse_args() +mass = 10 # eV if args.mass != None: mass = args.mass -else: - print("Hidden photon mass not specified!!") - print("Specify with argument --m") - quit() rmlfile = "fluxes.rml" if args.rmlfile != None: @@ -62,23 +62,15 @@ if args.outfname != None: outfname = args.outfname -fluxname = "combined" +fluxname = "HiddenPhoton" if args.fluxname != None: fluxname = args.fluxname - samples = 20000 if args.samples != None: samples = args.samples validation = True -if ( - rmlfile == "fluxes.rml" - and fluxname == "combined" - and outfname == "flux.png" - and samples == 20000 -): - validation = True ROOT.gSystem.Load("libRestFramework.so") ROOT.gSystem.Load("libRestAxion.so") @@ -92,7 +84,7 @@ pad1.Draw() combinedFlux = ROOT.TRestAxionSolarHiddenPhotonFlux(rmlfile, fluxname) -combinedFlux.Initialize() +combinedFlux.Initialize(mass) combinedFlux.PrintMetadata() if combinedFlux.GetError(): @@ -102,15 +94,14 @@ comb_spt = TH2D("comb_spt", "Energy versus solar radius", 20000, 0, 20, 100, 0, 1) for x in range(samples): - x = combinedFlux.GetRandomEnergyAndRadius(mass) + x = combinedFlux.GetRandomEnergyAndRadius((-1,-1)) comb_spt.Fill(x[0], x[1]) rnd = TRandom3(0) solarDisk = TH2D("solar_disk", "SolarDisk", 120, -1.2, 1.2, 120, -1.2, 1.2) for x in range(samples): angle = rnd.Rndm() * 2 * math.pi - x = combinedFlux.GetRandomEnergyAndRadius(mass) - + x = combinedFlux.GetRandomEnergyAndRadius((-1,-1)) solarDisk.Fill(x[1] * math.cos(angle), x[1] * math.sin(angle)) pad1.cd(1) From 55492be454907f32b8b2179f799ac27d0fda4729 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Fri, 8 Sep 2023 13:55:58 +0000 Subject: [PATCH 27/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py | 10 ++++------ 1 file changed, 4 insertions(+), 6 deletions(-) diff --git a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py index 7743f843..d24dfcc1 100755 --- a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py +++ b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py @@ -44,13 +44,11 @@ parser.add_argument( "--N", dest="samples", type=int, help="The number of generated particles" ) -parser.add_argument( - "--mass", dest="mass", type=float, help="Hidden photon mass [eV]" -) +parser.add_argument("--mass", dest="mass", type=float, help="Hidden photon mass [eV]") args = parser.parse_args() -mass = 10 # eV +mass = 10 # eV if args.mass != None: mass = args.mass @@ -94,14 +92,14 @@ comb_spt = TH2D("comb_spt", "Energy versus solar radius", 20000, 0, 20, 100, 0, 1) for x in range(samples): - x = combinedFlux.GetRandomEnergyAndRadius((-1,-1)) + x = combinedFlux.GetRandomEnergyAndRadius((-1, -1)) comb_spt.Fill(x[0], x[1]) rnd = TRandom3(0) solarDisk = TH2D("solar_disk", "SolarDisk", 120, -1.2, 1.2, 120, -1.2, 1.2) for x in range(samples): angle = rnd.Rndm() * 2 * math.pi - x = combinedFlux.GetRandomEnergyAndRadius((-1,-1)) + x = combinedFlux.GetRandomEnergyAndRadius((-1, -1)) solarDisk.Fill(x[1] * math.cos(angle), x[1] * math.sin(angle)) pad1.cd(1) From 3950fa13fedf6cf16e816186292e4e6d26e44ff9 Mon Sep 17 00:00:00 2001 From: Javier Galan Date: Mon, 11 Sep 2023 12:51:52 +0200 Subject: [PATCH 28/48] Revert "created hidden photon plot code" This reverts commit ac0aa28aaf490f63ae9133da157f0f7a249ba8b8. --- data | 1 - src/TRestAxionSolarHiddenPhotonFlux.cxx | 4 +--- 2 files changed, 1 insertion(+), 4 deletions(-) delete mode 120000 data diff --git a/data b/data deleted file mode 120000 index 95fc0d20..00000000 --- a/data +++ /dev/null @@ -1 +0,0 @@ -../axionlib-data \ No newline at end of file diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index fe285b04..77abd9b8 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -454,9 +454,7 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, /// \brief It returns a random solar radius position and energy according to the /// flux distributions defined inside the solar tables loaded in the class /// -std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange, - Double_t HPmass) { - LoadTables(HPmass); // load tables with specified hidden photon mass +std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); From ee57b39a1064684847bfe43688d2ae1b5072d491 Mon Sep 17 00:00:00 2001 From: Javier Galan Date: Mon, 11 Sep 2023 12:58:39 +0200 Subject: [PATCH 29/48] Readding data submodule? --- .gitmodules | 2 +- data | 1 + 2 files changed, 2 insertions(+), 1 deletion(-) create mode 160000 data diff --git a/.gitmodules b/.gitmodules index 29be5f3e..7fe95128 100644 --- a/.gitmodules +++ b/.gitmodules @@ -1,6 +1,6 @@ [submodule "data"] path = data - url = https://github.com/rest-for-physics/axionlib-data.git + url = https://github.com/rest-for-physics/axionlib-data [submodule "external/solarAxionFlux"] path = external/solarAxionFlux url = https://github.com/sebhoof/SolarAxionFlux.git diff --git a/data b/data new file mode 160000 index 00000000..957d9fc5 --- /dev/null +++ b/data @@ -0,0 +1 @@ +Subproject commit 957d9fc5e24d2e5aef97cfd1f99982f2c3a07a98 From d2e3d9b929dd076dd0cb27f0197acbf1e0902d2b Mon Sep 17 00:00:00 2001 From: Javier Galan Date: Mon, 11 Sep 2023 13:08:24 +0200 Subject: [PATCH 30/48] TRestAxionSolarXYZFlux. Fixing compilation issues --- inc/TRestAxionSolarFlux.h | 3 +-- inc/TRestAxionSolarHiddenPhotonFlux.h | 3 +-- inc/TRestAxionSolarQCDFlux.h | 3 +-- src/TRestAxionSolarQCDFlux.cxx | 3 +-- 4 files changed, 4 insertions(+), 8 deletions(-) diff --git a/inc/TRestAxionSolarFlux.h b/inc/TRestAxionSolarFlux.h index 1d068863..30c49340 100644 --- a/inc/TRestAxionSolarFlux.h +++ b/inc/TRestAxionSolarFlux.h @@ -71,8 +71,7 @@ class TRestAxionSolarFlux : public TRestMetadata { virtual Double_t GetTotalFlux(Double_t mass = 0) = 0; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - virtual std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), - Double_t mass = 0) = 0; + virtual std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) = 0; /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 virtual TH1F* GetEnergySpectrum(Double_t m = 0) = 0; diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 502983af..876a29ef 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -87,8 +87,7 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), - Double_t mass = 0) override; + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; /// It defines how to read the solar tables at the inhereted class for a given mass in eV Bool_t LoadTables(Double_t mass) override; diff --git a/inc/TRestAxionSolarQCDFlux.h b/inc/TRestAxionSolarQCDFlux.h index 240fd395..13246023 100644 --- a/inc/TRestAxionSolarQCDFlux.h +++ b/inc/TRestAxionSolarQCDFlux.h @@ -87,8 +87,7 @@ class TRestAxionSolarQCDFlux : public TRestAxionSolarFlux { Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1), - Double_t mass = 0) override; + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; /// It defines how to read the solar tables at the inhereted class Bool_t LoadTables(Double_t mass = 0) override; diff --git a/src/TRestAxionSolarQCDFlux.cxx b/src/TRestAxionSolarQCDFlux.cxx index c64969df..457bd31f 100644 --- a/src/TRestAxionSolarQCDFlux.cxx +++ b/src/TRestAxionSolarQCDFlux.cxx @@ -658,8 +658,7 @@ Double_t TRestAxionSolarQCDFlux::IntegrateFluxInRange(TVector2 eRange, Double_t /// \brief It returns a random solar radius position and energy according to the /// flux distributions defined inside the solar tables loaded in the class /// -std::pair TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius(TVector2 eRange, - Double_t mass) { +std::pair TRestAxionSolarQCDFlux::GetRandomEnergyAndRadius(TVector2 eRange) { std::pair result = {0, 0}; if (!AreTablesLoaded()) return result; Double_t rnd = fRandom->Rndm(); From 56f58d2669f586816e6224b64427308bb06b9da0 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Tue, 12 Sep 2023 10:28:40 +0200 Subject: [PATCH 31/48] fixing hidden photon solar plot --- inc/TRestAxionSolarFlux.h | 21 +- inc/TRestAxionSolarHiddenPhotonFlux.h | 36 +- inc/TRestAxionSolarHiddenPhotonFlux.h.new | 131 ++++ inc/TRestAxionSolarHiddenPhotonFlux.h.old | 131 ++++ inc/TRestAxionSolarQCDFlux.h | 26 +- .../solarFlux/solarPlotHiddenPhoton.py | 31 +- src/TRestAxionSolarFlux.cxx | 22 +- src/TRestAxionSolarHiddenPhotonFlux.cxx | 163 +++-- src/TRestAxionSolarHiddenPhotonFlux.cxx.new | 583 +++++++++++++++++ src/TRestAxionSolarHiddenPhotonFlux.cxx.old | 613 ++++++++++++++++++ src/TRestAxionSolarQCDFlux.cxx | 82 +-- 11 files changed, 1646 insertions(+), 193 deletions(-) create mode 100644 inc/TRestAxionSolarHiddenPhotonFlux.h.new create mode 100644 inc/TRestAxionSolarHiddenPhotonFlux.h.old create mode 100644 src/TRestAxionSolarHiddenPhotonFlux.cxx.new create mode 100644 src/TRestAxionSolarHiddenPhotonFlux.cxx.old diff --git a/inc/TRestAxionSolarFlux.h b/inc/TRestAxionSolarFlux.h index 30c49340..9a917211 100644 --- a/inc/TRestAxionSolarFlux.h +++ b/inc/TRestAxionSolarFlux.h @@ -24,8 +24,8 @@ #define _TRestAxionSolarFlux #include -#include -#include +#include +#include #include #include @@ -58,23 +58,29 @@ class TRestAxionSolarFlux : public TRestMetadata { TRestAxionSolarFlux(const char* cfgFileName, std::string name = ""); /// It defines how to read the solar tables at the inhereted class - virtual Bool_t LoadTables(Double_t mass = 0) = 0; + virtual Bool_t LoadTables() = 0; public: /// It is required in order to load solar flux tables into memory void Initialize(); + /// It is required in order to load solar flux tables into memory for specific mass + void InitializeMass( Double_t mass ) { SetMass(mass); Initialize(); } + + /// Set mass and reinitialise + void SetMass( Double_t m ) { fMass = m; } //Initialize(); } + /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range - virtual Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) = 0; + virtual Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) = 0; /// It returns the total integrated flux at earth in cm-2 s-1 - virtual Double_t GetTotalFlux(Double_t mass = 0) = 0; + virtual Double_t GetTotalFlux() = 0; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux virtual std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) = 0; /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 - virtual TH1F* GetEnergySpectrum(Double_t m = 0) = 0; + virtual TH1D* GetEnergySpectrum() = 0; virtual TCanvas* DrawSolarFlux(); @@ -86,9 +92,8 @@ class TRestAxionSolarFlux : public TRestMetadata { Bool_t AreTablesLoaded() { return fTablesLoaded; } Double_t GetMass() { return fMass; } - void SetMass(const Double_t& m) { fMass = m; } - TH1F* GetFluxHistogram(std::string fname, Double_t binSize = 0.01); + TH1D* GetFluxHistogram(std::string fname, Double_t binSize = 0.01); TCanvas* DrawFluxFile(std::string fname, Double_t binSize = 0.01); void PrintMetadata(); diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 876a29ef..2df02f96 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -41,20 +41,20 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { /// It will be used when loading `.flux` files to define the input file energy binsize in eV. Double_t fBinSize = 0; //< - /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fFluxTable; //! + /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFluxTable; //! - /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fContinuumTable; //! + /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector> fContinuumTable; //! - /// The tabulated resonance width TH1F(200,0,20)keV in eV2 versus solar radius - std::vector fWidthTable; //! + /// The tabulated resonance width TH1D(200,0,20)keV in eV2 versus solar radius + std::vector> fWidthTable; //! /// The solar plasma frequency vector in eV versus solar radius - std::vector fPlasmaFreqTable; //! + std::vector> fPlasmaFreqTable; //! - /// The total solar flux TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fFullFluxTable; //! + /// The total solar flux TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFullFluxTable; //! /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) std::vector fFluxTableIntegrals; //! @@ -63,17 +63,17 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Double_t fTotalContinuumFlux = 0; //! /// A pointer to the continuum spectrum histogram - TH1F* fContinuumHist = nullptr; //! + TH1D* fContinuumHist = nullptr; //! /// A pointer to the superposed monochromatic and continuum spectrum histogram - TH1F* fTotalHist = nullptr; //! + TH1D* fTotalHist = nullptr; //! void ReadFluxFile(); void LoadContinuumFluxTable(); void LoadMonoChromaticFluxTable(); void IntegrateSolarFluxes(); - public: + public: /// It returns true if continuum flux spectra was loaded Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } @@ -84,13 +84,13 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { Bool_t isPlasmaFreqLoaded() { return fPlasmaFreqTable.size() > 0; } /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range - Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; + Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; /// It defines how to read the solar tables at the inhereted class for a given mass in eV - Bool_t LoadTables(Double_t mass) override; + Bool_t LoadTables() override; void LoadContinuumTable(); void LoadWidthTable(); @@ -99,13 +99,13 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { // calculate solar HP flux from the 3 tables and mass void CalculateSolarFlux(); /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux(Double_t mass = 0) override { return fTotalContinuumFlux; } + Double_t GetTotalFlux() override { return fTotalContinuumFlux; } /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 - TH1F* GetEnergySpectrum(Double_t m = 0) override { return GetTotalSpectrum(); } + TH1D* GetEnergySpectrum() override { return GetTotalSpectrum(); } - TH1F* GetContinuumSpectrum(); - TH1F* GetTotalSpectrum(); + TH1D* GetContinuumSpectrum(); + TH1D* GetTotalSpectrum(); virtual TCanvas* DrawSolarFlux() override; diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h.new b/inc/TRestAxionSolarHiddenPhotonFlux.h.new new file mode 100644 index 00000000..2df02f96 --- /dev/null +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h.new @@ -0,0 +1,131 @@ +/************************************************************************* + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +#ifndef _TRestAxionSolarHiddenPhotonFlux +#define _TRestAxionSolarHiddenPhotonFlux + +#include +#include + +//! A metadata class to load tabulated solar hidden photon fluxes. Kinetic mixing set to 1. +class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { + private: + /// The filename containing the solar flux table with continuum spectrum + std::string fFluxDataFile = ""; //< + + /// The filename containing the resonance width (wGamma) + std::string fWidthDataFile = ""; //< + + /// The filename containing the plasma frequency (wp) table + std::string fPlasmaFreqDataFile = ""; //< + + /// It will be used when loading `.flux` files to define the input file energy binsize in eV. + Double_t fBinSize = 0; //< + + /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFluxTable; //! + + /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector> fContinuumTable; //! + + /// The tabulated resonance width TH1D(200,0,20)keV in eV2 versus solar radius + std::vector> fWidthTable; //! + + /// The solar plasma frequency vector in eV versus solar radius + std::vector> fPlasmaFreqTable; //! + + /// The total solar flux TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFullFluxTable; //! + + /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) + std::vector fFluxTableIntegrals; //! + + /// Total solar flux for monochromatic contributions + Double_t fTotalContinuumFlux = 0; //! + + /// A pointer to the continuum spectrum histogram + TH1D* fContinuumHist = nullptr; //! + + /// A pointer to the superposed monochromatic and continuum spectrum histogram + TH1D* fTotalHist = nullptr; //! + + void ReadFluxFile(); + void LoadContinuumFluxTable(); + void LoadMonoChromaticFluxTable(); + void IntegrateSolarFluxes(); + + public: + /// It returns true if continuum flux spectra was loaded + Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } + + /// It returns true if width table was loaded + Bool_t isWidthTableLoaded() { return fWidthTable.size() > 0; } + + /// It returns true if plasma frequency table was loaded + Bool_t isPlasmaFreqLoaded() { return fPlasmaFreqTable.size() > 0; } + + /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range + Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; + + /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; + + /// It defines how to read the solar tables at the inhereted class for a given mass in eV + Bool_t LoadTables() override; + + void LoadContinuumTable(); + void LoadWidthTable(); + void LoadPlasmaFreqTable(); + + // calculate solar HP flux from the 3 tables and mass + void CalculateSolarFlux(); + /// It returns the total integrated flux at earth in cm-2 s-1 + Double_t GetTotalFlux() override { return fTotalContinuumFlux; } + + /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 + TH1D* GetEnergySpectrum() override { return GetTotalSpectrum(); } + + TH1D* GetContinuumSpectrum(); + TH1D* GetTotalSpectrum(); + + virtual TCanvas* DrawSolarFlux() override; + + /// Tables might be loaded using a solar model description by TRestAxionSolarModel + void InitializeSolarTable(TRestAxionSolarModel* model) { + // TOBE implemented + // This method should initialize the tables fFluxTable and fFluxLines + } + + void ExportTables(Bool_t ascii = false) override; + + void PrintMetadata() override; + + void PrintContinuumSolarTable(); + void PrintIntegratedRingFlux(); + + TRestAxionSolarHiddenPhotonFlux(); + TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, std::string name = ""); + ~TRestAxionSolarHiddenPhotonFlux(); + + ClassDefOverride(TRestAxionSolarHiddenPhotonFlux, 1); +}; +#endif diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h.old b/inc/TRestAxionSolarHiddenPhotonFlux.h.old new file mode 100644 index 00000000..bdc44040 --- /dev/null +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h.old @@ -0,0 +1,131 @@ +/************************************************************************* + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +#ifndef _TRestAxionSolarHiddenPhotonFlux +#define _TRestAxionSolarHiddenPhotonFlux + +#include +#include + +//! A metadata class to load tabulated solar hidden photon fluxes. Kinetic mixing set to 1. +class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { + private: + /// The filename containing the solar flux table with continuum spectrum + std::string fFluxDataFile = ""; //< + + /// The filename containing the resonance width (wGamma) + std::string fWidthDataFile = ""; //< + + /// The filename containing the plasma frequency (wp) table + std::string fPlasmaFreqDataFile = ""; //< + + /// It will be used when loading `.flux` files to define the input file energy binsize in eV. + Double_t fBinSize = 0; //< + + /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFluxTable; //! + + /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fContinuumTable; //! + + /// The tabulated resonance width TH1D(200,0,20)keV in eV2 versus solar radius + std::vector fWidthTable; //! + + /// The solar plasma frequency vector in eV versus solar radius + std::vector fPlasmaFreqTable; //! + + /// The total solar flux TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFullFluxTable; //! + + /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) + std::vector fFluxTableIntegrals; //! + + /// Total solar flux for monochromatic contributions + Double_t fTotalContinuumFlux = 0; //! + + /// A pointer to the continuum spectrum histogram + TH1D* fContinuumHist = nullptr; //! + + /// A pointer to the superposed monochromatic and continuum spectrum histogram + TH1D* fTotalHist = nullptr; //! + + void ReadFluxFile(); + void LoadContinuumFluxTable(); + void LoadMonoChromaticFluxTable(); + void IntegrateSolarFluxes(); + + public: + /// It returns true if continuum flux spectra was loaded + Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } + + /// It returns true if width table was loaded + Bool_t isWidthTableLoaded() { return fWidthTable.size() > 0; } + + /// It returns true if plasma frequency table was loaded + Bool_t isPlasmaFreqLoaded() { return fPlasmaFreqTable.size() > 0; } + + /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range + Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; + + /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux + std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; + + /// It defines how to read the solar tables at the inhereted class for a given mass in eV + Bool_t LoadTables() override; + + void LoadContinuumTable(); + void LoadWidthTable(); + void LoadPlasmaFreqTable(); + + // calculate solar HP flux from the 3 tables and mass + void CalculateSolarFlux(); + /// It returns the total integrated flux at earth in cm-2 s-1 + Double_t GetTotalFlux() override { return fTotalContinuumFlux; } + + /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 + TH1D* GetEnergySpectrum() override { return GetTotalSpectrum(); } + + TH1D* GetContinuumSpectrum(); + TH1D* GetTotalSpectrum(); + + virtual TCanvas* DrawSolarFlux() override; + + /// Tables might be loaded using a solar model description by TRestAxionSolarModel + void InitializeSolarTable(TRestAxionSolarModel* model) { + // TOBE implemented + // This method should initialize the tables fFluxTable and fFluxLines + } + + void ExportTables(Bool_t ascii = false) override; + + void PrintMetadata() override; + + void PrintContinuumSolarTable(); + void PrintIntegratedRingFlux(); + + TRestAxionSolarHiddenPhotonFlux(); + TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, std::string name = ""); + ~TRestAxionSolarHiddenPhotonFlux(); + + ClassDefOverride(TRestAxionSolarHiddenPhotonFlux, 1); +}; +#endif diff --git a/inc/TRestAxionSolarQCDFlux.h b/inc/TRestAxionSolarQCDFlux.h index 13246023..10db402e 100644 --- a/inc/TRestAxionSolarQCDFlux.h +++ b/inc/TRestAxionSolarQCDFlux.h @@ -41,11 +41,11 @@ class TRestAxionSolarQCDFlux : public TRestAxionSolarFlux { /// It will be used when loading `.flux` files to define the threshold for peak identification Double_t fPeakSigma = 0; //< - /// The tabulated solar flux continuum spectra TH1F(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fFluxTable; //! + /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius + std::vector fFluxTable; //! /// The tabulated solar flux in cm-2 s-1 for a number of monochromatic energies versus solar radius - std::map fFluxLines; //! + std::map fFluxLines; //! /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) std::vector fFluxTableIntegrals; //! @@ -63,13 +63,13 @@ class TRestAxionSolarQCDFlux : public TRestAxionSolarFlux { Double_t fFluxRatio = 0; //! /// A pointer to the continuum spectrum histogram - TH1F* fContinuumHist = nullptr; //! + TH1D* fContinuumHist = nullptr; //! /// A pointer to the monochromatic spectrum histogram - TH1F* fMonoHist = nullptr; //! + TH1D* fMonoHist = nullptr; //! /// A pointer to the superposed monochromatic and continuum spectrum histogram - TH1F* fTotalHist = nullptr; //! + TH1D* fTotalHist = nullptr; //! void ReadFluxFile(); void LoadContinuumFluxTable(); @@ -84,25 +84,25 @@ class TRestAxionSolarQCDFlux : public TRestAxionSolarFlux { Bool_t isSolarSpectrumLoaded() { return fFluxLines.size() > 0; } /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range - Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1), Double_t mass = 0) override; + Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; /// It defines how to read the solar tables at the inhereted class - Bool_t LoadTables(Double_t mass = 0) override; + Bool_t LoadTables() override; /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux(Double_t mass = 0) override { + Double_t GetTotalFlux() override { return fTotalContinuumFlux + fTotalMonochromaticFlux; } /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 - TH1F* GetEnergySpectrum(Double_t m = 0) override { return GetTotalSpectrum(); } + TH1D* GetEnergySpectrum() override { return GetTotalSpectrum(); } - TH1F* GetContinuumSpectrum(); - TH1F* GetMonochromaticSpectrum(); - TH1F* GetTotalSpectrum(); + TH1D* GetContinuumSpectrum(); + TH1D* GetMonochromaticSpectrum(); + TH1D* GetTotalSpectrum(); virtual TCanvas* DrawSolarFlux() override; diff --git a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py index d24dfcc1..c07ac580 100755 --- a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py +++ b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py @@ -44,11 +44,12 @@ parser.add_argument( "--N", dest="samples", type=int, help="The number of generated particles" ) -parser.add_argument("--mass", dest="mass", type=float, help="Hidden photon mass [eV]") - +parser.add_argument( + "--m", dest="mass", type=float, help="Hidden photon mass [eV]" +) args = parser.parse_args() -mass = 10 # eV +mass = 10. # eV if args.mass != None: mass = args.mass @@ -68,7 +69,7 @@ if args.samples != None: samples = args.samples -validation = True +validation = False ROOT.gSystem.Load("libRestFramework.so") ROOT.gSystem.Load("libRestAxion.so") @@ -82,7 +83,9 @@ pad1.Draw() combinedFlux = ROOT.TRestAxionSolarHiddenPhotonFlux(rmlfile, fluxname) -combinedFlux.Initialize(mass) +combinedFlux.SetMass(mass) +print(combinedFlux.GetMass()) +combinedFlux.Initialize() combinedFlux.PrintMetadata() if combinedFlux.GetError(): @@ -91,8 +94,9 @@ exit(101) comb_spt = TH2D("comb_spt", "Energy versus solar radius", 20000, 0, 20, 100, 0, 1) -for x in range(samples): +for i in range(samples): x = combinedFlux.GetRandomEnergyAndRadius((-1, -1)) + #print(x) comb_spt.Fill(x[0], x[1]) rnd = TRandom3(0) @@ -160,17 +164,4 @@ c1.Print(outfname) print("Generated file : " + outfname) -print("\nMaximum energy bin is " + str(enSpt.GetMaximumBin())) -if validation: - if enSpt.GetMaximumBin() != 8001: - print("\nMaximum Bin is not the expected one (8001)! Exit code : 1") - exit(1) - -print("\nMaximum radius bin is " + str(rSpt.GetMaximumBin())) - -if validation: - if rSpt.GetMaximumBin() != 25: - print("\nMaximum Bin is not the expected one (25)! Exit code : 2") - exit(2) - -exit(0) +#exit(0) diff --git a/src/TRestAxionSolarFlux.cxx b/src/TRestAxionSolarFlux.cxx index a2e0ccd6..f82d9e34 100644 --- a/src/TRestAxionSolarFlux.cxx +++ b/src/TRestAxionSolarFlux.cxx @@ -64,7 +64,7 @@ /// on the flux distribution initialized. /// - **LoadTables**: It is called by TRestAxionSolarFlux::Initialize to allow the inherited /// class to load all the necessary tables in memory. -/// - **GetEnergySpectrum**: It should return a TH1F pointer with a energy spectrum histogram. +/// - **GetEnergySpectrum**: It should return a TH1D pointer with a energy spectrum histogram. /// ///-------------------------------------------------------------------------- /// @@ -125,12 +125,7 @@ void TRestAxionSolarFlux::Initialize() { fTablesLoaded = false; if (LoadTables()) fTablesLoaded = true; - if (!fRandom) { - delete fRandom; - fRandom = nullptr; - } - - if (fRandom != nullptr) { + if (fRandom) { delete fRandom; fRandom = nullptr; } @@ -139,11 +134,18 @@ void TRestAxionSolarFlux::Initialize() { fSeed = fRandom->TRandom::GetSeed(); } + +/////////////////////////////////////////////// +/// \brief Initialization of TRestAxionSolarFlux members with specific mass +/// +//void TRestAxionSolarFlux::InitializeMass( Double_t mass ) { SetMass(mass); RESTMetadata << GetMass() << RESTendl; } // SetMass calls Initialize + + /////////////////////////////////////////////// /// \brief It builds a histogram using the contents of the .flux file given /// in the argument. /// -TH1F* TRestAxionSolarFlux::GetFluxHistogram(string fname, Double_t binSize) { +TH1D* TRestAxionSolarFlux::GetFluxHistogram(string fname, Double_t binSize) { string fullPathName = SearchFile(fname); std::vector> fluxData; @@ -160,7 +162,7 @@ TH1F* TRestAxionSolarFlux::GetFluxHistogram(string fname, Double_t binSize) { originalHist->Fill(r, en, flux); } - return (TH1F*)originalHist->ProjectionY(); + return (TH1D*)originalHist->ProjectionY(); } /////////////////////////////////////////////// @@ -206,7 +208,7 @@ TCanvas* TRestAxionSolarFlux::DrawSolarFlux() { pad1->SetLeftMargin(0.15); pad1->SetBottomMargin(0.15); - TH1F* ht = GetEnergySpectrum(); + TH1D* ht = GetEnergySpectrum(); ht->SetLineColor(kBlack); ht->SetFillStyle(4050); ht->SetFillColor(kBlue - 10); diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 77abd9b8..01f443fa 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -183,10 +183,25 @@ TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} /// \brief It will load the tables in memory by using the filename information provided /// inside the metadata members, and calculate the solar flux for a given m. /// -Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables(Double_t mass) { - if (fFluxDataFile == "" || fWidthDataFile == "" || fPlasmaFreqDataFile == "") return false; +Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - SetMass(mass); + if (GetMass() <= 0 ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; + return false; + } + if ( fFluxDataFile == "" ){ + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; + return false; + } + if ( fWidthDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; + return false; + } + if ( fPlasmaFreqDataFile == "" ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; + return false; + } LoadContinuumFluxTable(); LoadWidthTable(); @@ -195,7 +210,6 @@ Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables(Double_t mass) { CalculateSolarFlux(); IntegrateSolarFluxes(); - return true; } @@ -203,9 +217,9 @@ Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables(Double_t mass) { /// \brief A helper method to load the data file containing continuum spectra as a /// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. /// -void TRestAxionSolarHiddenPhotonFlux::LoadContinuumTable() { +void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { if (fFluxDataFile == "") { - RESTDebug + RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" << RESTendl; return; @@ -216,26 +230,18 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; - std::vector> fluxTable; - if (!TRestTools::IsBinaryFile(fFluxDataFile)) { - fluxTable.clear(); + fContinuumTable.clear(); RESTError << "File is not in binary format!" << RESTendl; } - TRestTools::ReadBinaryTable(fullPathName, fluxTable); + TRestTools::ReadBinaryTable(fullPathName, fContinuumTable); - if (fluxTable.size() != 1000 && fluxTable[0].size() != 200) { - fluxTable.clear(); + if (fContinuumTable.size() != 1000 || fContinuumTable[0].size() != 200) { RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; - } - - for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1F* h = new TH1F(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); - fContinuumTable.push_back(h); + fContinuumTable.clear(); } } @@ -245,7 +251,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumTable() { /// void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { if (fFluxDataFile == "") { - RESTDebug << "TRestAxionSolarHiddenPhotonFlux::LoadWidthTable. No width table was defined" + RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadWidthTable. No width table was defined" << RESTendl; return; } @@ -255,26 +261,18 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; - std::vector> fluxTable; - if (!TRestTools::IsBinaryFile(fWidthDataFile)) { - fluxTable.clear(); + fWidthTable.clear(); RESTError << "File is not in binary format!" << RESTendl; } - TRestTools::ReadBinaryTable(fullPathName, fluxTable); - - if (fluxTable.size() != 1000 && fluxTable[0].size() != 200) { - fluxTable.clear(); + TRestTools::ReadBinaryTable(fullPathName, fWidthTable); + + if (fWidthTable.size() != 1000 || fWidthTable[0].size() != 200) { RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; - } - - for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1F* h = new TH1F(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); - fWidthTable.push_back(h); + fWidthTable.clear(); } } @@ -284,7 +282,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { /// void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { if (fFluxDataFile == "") { - RESTDebug + RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" << RESTendl; return; @@ -295,26 +293,18 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; - std::vector> fluxTable; - if (!TRestTools::IsBinaryFile(fWidthDataFile)) { - fluxTable.clear(); RESTError << "File is not in binary format!" << RESTendl; + fPlasmaFreqTable.clear(); } - TRestTools::ReadBinaryTable(fullPathName, fluxTable); - - if (fluxTable.size() != 1000 && fluxTable[0].size() != 1) { - fluxTable.clear(); - RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" + TRestTools::ReadBinaryTable(fullPathName, fPlasmaFreqTable); + + if (fPlasmaFreqTable.size() != 1000 || fPlasmaFreqTable[0].size() != 1) { + RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; - } - - for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1F* h = new TH1F(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); - fPlasmaFreqTable.push_back(h); + fPlasmaFreqTable.clear(); } } @@ -326,35 +316,37 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { if (GetMass() == 0) { RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; + } + if (fContinuumTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; + return; } + if (fPlasmaFreqTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; + return; + } + if (fWidthTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; + return; + } + Double_t mass = GetMass(); for (unsigned int n = 0; n < fContinuumTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - vector mass2Vector(200, pow(mass, 2)); - double wp = fPlasmaFreqTable[n]->GetBinContent(1); - vector wp2Vector(200, pow(wp, 2)); - vector weights(200, 1); - - TH1F* hMass = new TH1F("hMass", "hMass", 200, 0, 20); - TH1F* hWp = new TH1F("hWp", "hWp", 200, 0, 20); - TH1F* hWg2 = (TH1F*)fWidthTable[n]->Clone(); - hWg2->Multiply(hWg2); // (w G)^2 - - // hMass->FillN(200, mass2Vector); // m^2 hist - hMass->FillN(200, mass2Vector.data(), weights.data()); // m^2 hist - // hWp->FillN(200, wp2Vector); // wp^2 hist - hWp->FillN(200, wp2Vector.data(), weights.data()); // wp^2 hist - - hMass->Add(hWp, -1); // (m2 - wp2) - hMass->Multiply(hMass); // (m2 - wp2)^2 - hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 - - TH1F* h = (TH1F*)fWidthTable[n]->Clone(); - h->Multiply(fContinuumTable[n]); - h->Divide(hMass); - h->Scale(pow(mass, 4)); - + Double_t wp = fPlasmaFreqTable[n][0]; + vector wG = fWidthTable[n]; + vector flux = fContinuumTable[n]; + vector v; + for( unsigned int c; c < wG.size(); c++ ) { + Double_t d1 = ( wG[c] * flux[c] * pow(mass,4) ); // m4 * wG * flux + Double_t d2 = ( pow( pow(mass,2) - pow(wp,2) , 2 ) + pow(wG[c],2) ); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + v.push_back(d1/d2); + } + + TH1D* h = new TH1D(Form("%s_TotalFluxTable%d", GetName(), n), "", 200, 0, 20); + for (unsigned int c = 0; c < v.size(); c++) { h->SetBinContent(c + 1, v[c]); } + //for (unsigned int c = 0; c < v.size(); c++) { h->Fill(v[c]); } fFluxTable.push_back(h); } } @@ -363,13 +355,13 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { /// \brief It builds a histogram with the continuum spectrum. /// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. /// -TH1F* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { +TH1D* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { if (fContinuumHist != nullptr) { delete fContinuumHist; fContinuumHist = nullptr; } - fContinuumHist = new TH1F("ContinuumHist", "", 200, 0, 20); + fContinuumHist = new TH1D("ContinuumHist", "", 200, 0, 20); for (const auto& x : fFluxTable) { fContinuumHist->Add(x); } @@ -389,15 +381,15 @@ TH1F* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { /// \brief Same as GetContinuumSpectrum, the flux will be /// expressed in cm-2 s-1 keV-1. Binned in 1eV steps. /// -TH1F* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { - TH1F* hc = GetContinuumSpectrum(); +TH1D* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { + TH1D* hc = GetContinuumSpectrum(); if (fTotalHist != nullptr) { delete fTotalHist; fTotalHist = nullptr; } - fTotalHist = new TH1F("fTotalHist", "", 20000, 0, 20); + fTotalHist = new TH1D("fTotalHist", "", 20000, 0, 20); for (int n = 0; n < hc->GetNbinsX(); n++) { for (int m = 0; m < 100; m++) { fTotalHist->SetBinContent(n * 100 + 1 + m, hc->GetBinContent(n + 1)); @@ -433,7 +425,7 @@ void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { /////////////////////////////////////////////// /// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range /// -Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { +Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) { if (eRange.X() == -1 && eRange.Y() == -1) { if (GetTotalFlux() == 0) IntegrateSolarFluxes(); return GetTotalFlux(); @@ -455,8 +447,9 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange, /// flux distributions defined inside the solar tables loaded in the class /// std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { + std::pair result = {0, 0}; - if (!AreTablesLoaded()) return result; + if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } Double_t rnd = fRandom->Rndm(); for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { if (rnd < fFluxTableIntegrals[r]) { @@ -464,7 +457,7 @@ std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAn if (eRange.X() != -1 && eRange.Y() != -1) { if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); } - Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.01; + Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.001; std::pair p = {energy, radius}; return p; } @@ -473,7 +466,7 @@ std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAn } /////////////////////////////////////////////// -/// \brief It prints on screen the table that has been loaded in memory +/// \brief It prints on screen the flux table that has been read from file /// void TRestAxionSolarHiddenPhotonFlux::PrintContinuumSolarTable() { cout << "Continuum solar flux table: " << endl; @@ -506,6 +499,9 @@ void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { TRestAxionSolarFlux::PrintMetadata(); + RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; RESTMetadata << "-------" << RESTendl; RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; RESTMetadata << "++++++++++++++++++" << RESTendl; @@ -532,9 +528,9 @@ void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { } if (fFluxTable.size() > 0) { - std::vector> table; + std::vector> table; for (const auto& x : fFluxTable) { - std::vector row; + std::vector row; for (int n = 0; n < x->GetNbinsX(); n++) row.push_back(x->GetBinContent(n + 1)); table.push_back(row); @@ -568,7 +564,7 @@ TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { pad1->cd(1)->SetLeftMargin(0.15); pad1->cd(1)->SetBottomMargin(0.15); - TH1F* ht = GetTotalSpectrum(); + TH1D* ht = GetTotalSpectrum(); ht->SetLineColor(kBlack); ht->SetFillStyle(4050); ht->SetFillColor(kBlue - 10); @@ -584,3 +580,4 @@ TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { return fCanvas; } + diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx.new b/src/TRestAxionSolarHiddenPhotonFlux.cxx.new new file mode 100644 index 00000000..26c782c1 --- /dev/null +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx.new @@ -0,0 +1,583 @@ +/******************** REST disclaimer *********************************** + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +////////////////////////////////////////////////////////////////////////// +/// TRestAxionSolarHiddenPhotonFlux will use a file in binary format to initialize +/// a solar flux table that will describe the solar hidden photon flux spectrum as a function +/// of the solar radius. +/// +/// This class loads the hidden photon flux that depends on the mass and kinetic mixing parameter. +/// For axion-like particle prodution independent of mass there is the class +/// TRestAxionSolarQCDFlux. Both classes are prototyped by a pure base class TRestAxionSolarFlux +/// that defines common methods used to evaluate the flux, and generate Monte-Carlo events inside +/// TRestAxionGeneratorProcess. +/// +/// ### Basic use +/// +/// Once the class has been initialized, the main use of this class will be provided +/// by the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. This method will +/// return a random axion energy and position inside the solar radius following the +/// distributions given by the solar flux tables. +/// +/// Description of the specific parameters accepted by this metadata class. +/// - *fluxDataFile:* A table with 1000 rows representing the solar ring flux from the +/// center to the corona, and 200 columns representing the flux, measured in cm-2 s-1 keV-1, +/// for the range (0,20)keV in steps of 100eV. The table is provided as a binary table using +/// `.N200f` extension. +/// - *widthDataFile:* A table with 1000 rows representing the width of the hidden photon +/// resonant production (wG) for each solar ring from the center to the corona, and 200 columns +/// representing the width, measured in eV2, for the range (0,20)keV in steps of 100eV. The +/// table is provided as a binary table using `.N200f` extension. +/// - *plasmaFreqDataFile:* A table with 1000 rows and only 1 column representing the solar +/// plasma frequency (wp) for each solar ring from the center to the corona, measured in eV. The +/// table is provided as a binary table using `.N1f` extension. +/// +/// Pre-generated solar axion flux tables will be available at the +/// [axionlib-data](https://github.com/rest-for-physics/axionlib-data/tree/master) +/// repository. The different RML flux definitions used to load those tables +/// will be found at the +/// [fluxes.rml](https://github.com/rest-for-physics/axionlib-data/blob/master/solarFlux/fluxes.rml) +/// file found at the axionlib-data repository. +/// +/// Inside a local REST installation, the `fluxes.rml` file will be found at the REST +/// installation directory, and it will be located automatically by the +/// TRestMetadata::SearchFile method. +/// +/// ### A basic RML definition +/// +/// The following definition integrates an axion-photon component with a continuum +/// spectrum using a Primakoff production model, and a dummy spectrum file that +/// includes two monocrhomatic lines at different solar disk radius positions. +/// +/// \code +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// \endcode +/// +/// \warning When the flux is loaded manually inside the `restRoot` interactive +/// shell, or inside a macro or script, after metadata initialization, it is necessary +/// to call the method TRestAxionSolarHiddenPhotonFlux::LoadTables(mass) to trigger the tables +/// initialization. +/// +/// ### Performing MonteCarlo tests using pre-loaded tables +/// +/// In order to test the response of different solar flux definitions we may use the script +/// `solarPlot.py` found at `pipeline/metadata/solarFlux/`. This script will generate a +/// number of particles and it will assign to each particle an energy and solar disk +/// location with the help of the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. +/// +/// \code +/// python3 solarPlotHiddenPhoton.py --fluxname HiddenPhoton --N 1000000 +/// \endcode +/// +/// By default, it will load the flux definition found at `fluxes.rml` from the +/// `axionlib-data` repository, and generate a `png` image with the resuts from the +/// Monte Carlo execution. +/// +/// \htmlonly \endhtmlonly +/// +/// ![Solar flux distributions MC-generated with TRestAxionSolarQCDFlux.](ABC_flux_MC.png) +/// +/// ### Exporting the solar flux tables +/// +/// On top of that, we will be able to export those tables to the TRestAxionSolarHiddenPhotonFlux +/// standard format to be used in later occasions. +/// +/// \code +/// TRestAxionSolarHiddenPhotonFlux *sFlux = new TRestAxionSolarHiddenPhotonFlux("fluxes.rml", +/// "HiddenPhoton") sFlux->Initialize() sFlux->ExportTables() +/// \endcode +/// +/// which will produce a binary table `.N200f` with the continuum flux. The filename root will be +/// extracted from the original `.flux` file. Optionally we may export the continuum flux to an +/// ASCII file by indicating it at the TRestAxionSolarHiddenPhotonFlux::ExportTables method call. +/// The files will be placed at the REST user space, at `$HOME/.rest/export/` directory. +/// +/// TODO Implement the method TRestAxionSolarQCDFlux::InitializeSolarTable using +/// a solar model description by TRestAxionSolarModel. +/// +/// TODO Perhaps it would be interesting to replace fFluxTable for a TH2D +/// +///-------------------------------------------------------------------------- +/// +/// RESTsoft - Software for Rare Event Searches with TPCs +/// +/// History of developments: +/// +/// 2023-May: Specific methods extracted from TRestAxionSolarFlux +/// Javier Galan +/// 2023-June: TRestAxionSolarHiddenPhotonFlux created by editing TRestAxionSolarQCDFlux +/// Tomas O'Shea +/// +/// \class TRestAxionSolarHiddenPhotonFlux +/// \author Javier Galan +/// +///
+/// + +#include "TRestAxionSolarHiddenPhotonFlux.h" +using namespace std; + +ClassImp(TRestAxionSolarHiddenPhotonFlux); + +/////////////////////////////////////////////// +/// \brief Default constructor +/// +TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux() : TRestAxionSolarFlux() {} + +/////////////////////////////////////////////// +/// \brief Constructor loading data from a config file +/// +/// If no configuration path is defined using TRestMetadata::SetConfigFilePath +/// the path to the config file must be specified using full path, absolute or +/// relative. +/// +/// The default behaviour is that the config file must be specified with +/// full path, absolute or relative. +/// +/// \param cfgFileName A const char* giving the path to an RML file. +/// \param name The name of the specific metadata. It will be used to find the +/// corresponding TRestAxionMagneticField section inside the RML. +/// +TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, string name) + : TRestAxionSolarFlux(cfgFileName) { + LoadConfigFromFile(fConfigFileName, name); + + if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Info) PrintMetadata(); +} + +/////////////////////////////////////////////// +/// \brief Default destructor +/// +TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} + +/////////////////////////////////////////////// +/// \brief It will load the tables in memory by using the filename information provided +/// inside the metadata members, and calculate the solar flux for a given m. +/// +Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { + + if (GetMass() <= 0 ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; + return false; + } + if ( fFluxDataFile == "" ){ + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; + return false; + } + if ( fWidthDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; + return false; + } + if ( fPlasmaFreqDataFile == "" ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; + return false; + } + + LoadContinuumFluxTable(); + LoadWidthTable(); + LoadPlasmaFreqTable(); + + CalculateSolarFlux(); + + IntegrateSolarFluxes(); + return true; +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing continuum spectra as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { + if (fFluxDataFile == "") { + RESTError + << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fFluxDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + if (!TRestTools::IsBinaryFile(fFluxDataFile)) { + fContinuumTable.clear(); + RESTError << "File is not in binary format!" << RESTendl; + } + + TRestTools::ReadBinaryTable(fullPathName, fContinuumTable); + + if (fContinuumTable.size() != 1000 || fContinuumTable[0].size() != 200) { + RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows or columns" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + fContinuumTable.clear(); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing resonance width as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { + if (fFluxDataFile == "") { + RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadWidthTable. No width table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fWidthDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { + fWidthTable.clear(); + RESTError << "File is not in binary format!" << RESTendl; + } + + TRestTools::ReadBinaryTable(fullPathName, fWidthTable); + + if (fWidthTable.size() != 1000 || fWidthTable[0].size() != 200) { + RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + fWidthTable.clear(); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing resonance width as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { + if (fFluxDataFile == "") { + RESTError + << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fPlasmaFreqDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { + RESTError << "File is not in binary format!" << RESTendl; + fPlasmaFreqTable.clear(); + } + + TRestTools::ReadBinaryTable(fullPathName, fPlasmaFreqTable); + + if (fPlasmaFreqTable.size() != 1000 || fPlasmaFreqTable[0].size() != 1) { + RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + fPlasmaFreqTable.clear(); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the +/// and the hidden photon mass for chi=1. +/// +void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { + if (GetMass() == 0) { + RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; + return; + } + if (fContinuumTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; + return; + } + if (fPlasmaFreqTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; + return; + } + if (fWidthTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; + return; + } + fFluxTable.clear(); + Double_t mass = GetMass(); + for (unsigned int n = 0; n < fContinuumTable.size(); n++) { + // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + + Double_t wp = fPlasmaFreqTable[n][0]; + vector wG = fWidthTable[n]; + vector flux = fContinuumTable[n]; + vector v; + for( unsigned int c; c < wG.size(); c++ ) { + Double_t d1 = ( wG[c] * flux[c] * pow(mass,4) ); // m4 * wG * flux + Double_t d2 = ( pow( pow(mass,2) - pow(wp,2) , 2 ) + pow(wG[c],2) ); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + v.push_back(d1/d2); + } + + TH1D* h = new TH1D(Form("%s_TotalFluxTable%d", GetName(), n), "", 200, 0, 20); + for (unsigned int c = 0; c < v.size(); c++) { h->SetBinContent(c + 1, v[c]); } + //for (unsigned int c = 0; c < v.size(); c++) { h->Fill(v[c]); } + fFluxTable.push_back(h); + } +} + +/////////////////////////////////////////////// +/// \brief It builds a histogram with the continuum spectrum. +/// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. +/// +TH1D* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { + if (fContinuumHist != nullptr) { + delete fContinuumHist; + fContinuumHist = nullptr; + } + + fContinuumHist = new TH1D("ContinuumHist", "", 200, 0, 20); + for (const auto& x : fFluxTable) { + fContinuumHist->Add(x); + } + + fContinuumHist->SetStats(0); + fContinuumHist->GetXaxis()->SetTitle("Energy [keV]"); + fContinuumHist->GetXaxis()->SetTitleSize(0.05); + fContinuumHist->GetXaxis()->SetLabelSize(0.05); + fContinuumHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); + fContinuumHist->GetYaxis()->SetTitleSize(0.05); + fContinuumHist->GetYaxis()->SetLabelSize(0.05); + + return fContinuumHist; +} + +/////////////////////////////////////////////// +/// \brief Same as GetContinuumSpectrum, the flux will be +/// expressed in cm-2 s-1 keV-1. Binned in 1eV steps. +/// +TH1D* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { + TH1D* hc = GetContinuumSpectrum(); + + if (fTotalHist != nullptr) { + delete fTotalHist; + fTotalHist = nullptr; + } + + fTotalHist = new TH1D("fTotalHist", "", 20000, 0, 20); + for (int n = 0; n < hc->GetNbinsX(); n++) { + for (int m = 0; m < 100; m++) { + fTotalHist->SetBinContent(n * 100 + 1 + m, hc->GetBinContent(n + 1)); + } + } + + fTotalHist->SetStats(0); + fTotalHist->GetXaxis()->SetTitle("Energy [keV]"); + fTotalHist->GetXaxis()->SetTitleSize(0.05); + fTotalHist->GetXaxis()->SetLabelSize(0.05); + fTotalHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); + fTotalHist->GetYaxis()->SetTitleSize(0.05); + fTotalHist->GetYaxis()->SetLabelSize(0.05); + + return fTotalHist; +} + +/////////////////////////////////////////////// +/// \brief A helper method to initialize the internal class data members with the +/// integrated flux for each solar ring. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { + fTotalContinuumFlux = 0.0; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + fTotalContinuumFlux += fFluxTable[n]->Integral() * 0.1; // We integrate in 100eV steps + fFluxTableIntegrals.push_back(fTotalContinuumFlux); + } + + for (unsigned int n = 0; n < fFluxTableIntegrals.size(); n++) + fFluxTableIntegrals[n] /= fTotalContinuumFlux; +} + +/////////////////////////////////////////////// +/// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range +/// +Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) { + if (eRange.X() == -1 && eRange.Y() == -1) { + if (GetTotalFlux() == 0) IntegrateSolarFluxes(); + return GetTotalFlux(); + } + + Double_t flux = 0; + fTotalContinuumFlux = 0.0; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + flux += fFluxTable[n]->Integral(fFluxTable[n]->FindFixBin(eRange.X()), + fFluxTable[n]->FindFixBin(eRange.Y())) * + 0.1; // We integrate in 100eV steps + } + + return flux; +} + +/////////////////////////////////////////////// +/// \brief It returns a random solar radius position and energy according to the +/// flux distributions defined inside the solar tables loaded in the class +/// +std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { + + std::pair result = {0, 0}; + if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } + Double_t rnd = fRandom->Rndm(); + for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { + if (rnd < fFluxTableIntegrals[r]) { + Double_t energy = fFluxTable[r]->GetRandom(); + if (eRange.X() != -1 && eRange.Y() != -1) { + if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); + } + Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.001; + std::pair p = {energy, radius}; + return p; + } + } + return result; +} + +/////////////////////////////////////////////// +/// \brief It prints on screen the flux table that has been read from file +/// +void TRestAxionSolarHiddenPhotonFlux::PrintContinuumSolarTable() { + cout << "Continuum solar flux table: " << endl; + cout << "--------------------------- " << endl; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + for (int m = 0; m < fFluxTable[n]->GetNbinsX(); m++) + cout << fFluxTable[n]->GetBinContent(m + 1) << "\t"; + cout << endl; + cout << endl; + } + cout << endl; +} + +/////////////////////////////////////////////// +/// \brief It prints on screen the integrated solar flux per solar ring +/// +void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { + cout << "Integrated solar flux per solar ring: " << endl; + cout << "--------------------------- " << endl; + /* + for (int n = 0; n < fFluxPerRadius.size(); n++) + cout << "n : " << n << " flux : " << fFluxPerRadius[n] << endl; + cout << endl; + */ +} + +/////////////////////////////////////////////// +/// \brief Prints on screen the information about the metadata members of TRestAxionSolarHiddenPhotonFlux +/// +void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { + TRestAxionSolarFlux::PrintMetadata(); + + RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; + RESTMetadata << "-------" << RESTendl; + RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; + RESTMetadata << "++++++++++++++++++" << RESTendl; + + if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Debug) { + PrintContinuumSolarTable(); + PrintIntegratedRingFlux(); + } +} + +/////////////////////////////////////////////// +/// \brief It will create files with spectra to be used +/// in a later ocasion. +/// +void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { + string rootFilename = TRestTools::GetFileNameRoot(fFluxDataFile); + + string path = REST_USER_PATH + "/export/"; + + if (!TRestTools::fileExists(path)) { + std::cout << "Creating path: " << path << std::endl; + int z = system(("mkdir -p " + path).c_str()); + if (z != 0) RESTError << "Could not create directory " << path << RESTendl; + } + + if (fFluxTable.size() > 0) { + std::vector> table; + for (const auto& x : fFluxTable) { + std::vector row; + for (int n = 0; n < x->GetNbinsX(); n++) row.push_back(x->GetBinContent(n + 1)); + + table.push_back(row); + } + + if (!ascii) + TRestTools::ExportBinaryTable(path + "/" + rootFilename + ".N200f", table); + else + TRestTools::ExportASCIITable(path + "/" + rootFilename + ".dat", table); + } +} + +/////////////////////////////////////////////// +/// \brief It draws the contents of a .flux file. This method just receives the +/// +TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { + if (fCanvas != nullptr) { + delete fCanvas; + fCanvas = nullptr; + } + fCanvas = new TCanvas("canv", "This is the canvas title", 1200, 500); + fCanvas->Draw(); + + TPad* pad1 = new TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97); + pad1->Divide(2, 1); + pad1->Draw(); + + pad1->cd(1); + pad1->cd(1)->SetLogy(); + pad1->cd(1)->SetRightMargin(0.09); + pad1->cd(1)->SetLeftMargin(0.15); + pad1->cd(1)->SetBottomMargin(0.15); + + TH1D* ht = GetTotalSpectrum(); + ht->SetLineColor(kBlack); + ht->SetFillStyle(4050); + ht->SetFillColor(kBlue - 10); + + ht->Draw("hist"); + + pad1->cd(2); + pad1->cd(2)->SetRightMargin(0.09); + pad1->cd(2)->SetLeftMargin(0.15); + pad1->cd(2)->SetBottomMargin(0.15); + + ht->Draw("hist"); + + return fCanvas; +} + diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx.old b/src/TRestAxionSolarHiddenPhotonFlux.cxx.old new file mode 100644 index 00000000..e61f0630 --- /dev/null +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx.old @@ -0,0 +1,613 @@ +/******************** REST disclaimer *********************************** + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +////////////////////////////////////////////////////////////////////////// +/// TRestAxionSolarHiddenPhotonFlux will use a file in binary format to initialize +/// a solar flux table that will describe the solar hidden photon flux spectrum as a function +/// of the solar radius. +/// +/// This class loads the hidden photon flux that depends on the mass and kinetic mixing parameter. +/// For axion-like particle prodution independent of mass there is the class +/// TRestAxionSolarQCDFlux. Both classes are prototyped by a pure base class TRestAxionSolarFlux +/// that defines common methods used to evaluate the flux, and generate Monte-Carlo events inside +/// TRestAxionGeneratorProcess. +/// +/// ### Basic use +/// +/// Once the class has been initialized, the main use of this class will be provided +/// by the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. This method will +/// return a random axion energy and position inside the solar radius following the +/// distributions given by the solar flux tables. +/// +/// Description of the specific parameters accepted by this metadata class. +/// - *fluxDataFile:* A table with 1000 rows representing the solar ring flux from the +/// center to the corona, and 200 columns representing the flux, measured in cm-2 s-1 keV-1, +/// for the range (0,20)keV in steps of 100eV. The table is provided as a binary table using +/// `.N200f` extension. +/// - *widthDataFile:* A table with 1000 rows representing the width of the hidden photon +/// resonant production (wG) for each solar ring from the center to the corona, and 200 columns +/// representing the width, measured in eV2, for the range (0,20)keV in steps of 100eV. The +/// table is provided as a binary table using `.N200f` extension. +/// - *plasmaFreqDataFile:* A table with 1000 rows and only 1 column representing the solar +/// plasma frequency (wp) for each solar ring from the center to the corona, measured in eV. The +/// table is provided as a binary table using `.N1f` extension. +/// +/// Pre-generated solar axion flux tables will be available at the +/// [axionlib-data](https://github.com/rest-for-physics/axionlib-data/tree/master) +/// repository. The different RML flux definitions used to load those tables +/// will be found at the +/// [fluxes.rml](https://github.com/rest-for-physics/axionlib-data/blob/master/solarFlux/fluxes.rml) +/// file found at the axionlib-data repository. +/// +/// Inside a local REST installation, the `fluxes.rml` file will be found at the REST +/// installation directory, and it will be located automatically by the +/// TRestMetadata::SearchFile method. +/// +/// ### A basic RML definition +/// +/// The following definition integrates an axion-photon component with a continuum +/// spectrum using a Primakoff production model, and a dummy spectrum file that +/// includes two monocrhomatic lines at different solar disk radius positions. +/// +/// \code +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// +/// \endcode +/// +/// \warning When the flux is loaded manually inside the `restRoot` interactive +/// shell, or inside a macro or script, after metadata initialization, it is necessary +/// to call the method TRestAxionSolarHiddenPhotonFlux::LoadTables(mass) to trigger the tables +/// initialization. +/// +/// ### Performing MonteCarlo tests using pre-loaded tables +/// +/// In order to test the response of different solar flux definitions we may use the script +/// `solarPlot.py` found at `pipeline/metadata/solarFlux/`. This script will generate a +/// number of particles and it will assign to each particle an energy and solar disk +/// location with the help of the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. +/// +/// \code +/// python3 solarPlotHiddenPhoton.py --fluxname HiddenPhoton --N 1000000 +/// \endcode +/// +/// By default, it will load the flux definition found at `fluxes.rml` from the +/// `axionlib-data` repository, and generate a `png` image with the resuts from the +/// Monte Carlo execution. +/// +/// \htmlonly \endhtmlonly +/// +/// ![Solar flux distributions MC-generated with TRestAxionSolarQCDFlux.](ABC_flux_MC.png) +/// +/// ### Exporting the solar flux tables +/// +/// On top of that, we will be able to export those tables to the TRestAxionSolarHiddenPhotonFlux +/// standard format to be used in later occasions. +/// +/// \code +/// TRestAxionSolarHiddenPhotonFlux *sFlux = new TRestAxionSolarHiddenPhotonFlux("fluxes.rml", +/// "HiddenPhoton") sFlux->Initialize() sFlux->ExportTables() +/// \endcode +/// +/// which will produce a binary table `.N200f` with the continuum flux. The filename root will be +/// extracted from the original `.flux` file. Optionally we may export the continuum flux to an +/// ASCII file by indicating it at the TRestAxionSolarHiddenPhotonFlux::ExportTables method call. +/// The files will be placed at the REST user space, at `$HOME/.rest/export/` directory. +/// +/// TODO Implement the method TRestAxionSolarQCDFlux::InitializeSolarTable using +/// a solar model description by TRestAxionSolarModel. +/// +/// TODO Perhaps it would be interesting to replace fFluxTable for a TH2D +/// +///-------------------------------------------------------------------------- +/// +/// RESTsoft - Software for Rare Event Searches with TPCs +/// +/// History of developments: +/// +/// 2023-May: Specific methods extracted from TRestAxionSolarFlux +/// Javier Galan +/// 2023-June: TRestAxionSolarHiddenPhotonFlux created by editing TRestAxionSolarQCDFlux +/// Tomas O'Shea +/// +/// \class TRestAxionSolarHiddenPhotonFlux +/// \author Javier Galan +/// +///
+/// + +#include "TRestAxionSolarHiddenPhotonFlux.h" +using namespace std; + +ClassImp(TRestAxionSolarHiddenPhotonFlux); + +/////////////////////////////////////////////// +/// \brief Default constructor +/// +TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux() : TRestAxionSolarFlux() {} + +/////////////////////////////////////////////// +/// \brief Constructor loading data from a config file +/// +/// If no configuration path is defined using TRestMetadata::SetConfigFilePath +/// the path to the config file must be specified using full path, absolute or +/// relative. +/// +/// The default behaviour is that the config file must be specified with +/// full path, absolute or relative. +/// +/// \param cfgFileName A const char* giving the path to an RML file. +/// \param name The name of the specific metadata. It will be used to find the +/// corresponding TRestAxionMagneticField section inside the RML. +/// +TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, string name) + : TRestAxionSolarFlux(cfgFileName) { + LoadConfigFromFile(fConfigFileName, name); + + if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Info) PrintMetadata(); +} + +/////////////////////////////////////////////// +/// \brief Default destructor +/// +TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} + +/////////////////////////////////////////////// +/// \brief It will load the tables in memory by using the filename information provided +/// inside the metadata members, and calculate the solar flux for a given m. +/// +Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { + + if (GetMass() <= 0 ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; + return false; + } + if ( fFluxDataFile == "" ){ + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; + return false; + } + if ( fWidthDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; + return false; + } + if ( fPlasmaFreqDataFile == "" ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; + return false; + } + + LoadContinuumFluxTable(); + LoadWidthTable(); + LoadPlasmaFreqTable(); + + CalculateSolarFlux(); + + IntegrateSolarFluxes(); + return true; +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing continuum spectra as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { + if (fFluxDataFile == "") { + RESTError + << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fFluxDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + std::vector> fluxTable; + + if (!TRestTools::IsBinaryFile(fFluxDataFile)) { + fluxTable.clear(); + RESTError << "File is not in binary format!" << RESTendl; + } + + TRestTools::ReadBinaryTable(fullPathName, fluxTable); + + if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { + fluxTable.clear(); + RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows or columns" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1D* h = new TH1D(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + fContinuumTable.push_back(h); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing resonance width as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { + if (fFluxDataFile == "") { + RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadWidthTable. No width table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fWidthDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + std::vector> fluxTable; + + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { + fluxTable.clear(); + RESTError << "File is not in binary format!" << RESTendl; + } + + TRestTools::ReadBinaryTable(fullPathName, fluxTable); + //RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << RESTendl; + + if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { + fluxTable.clear(); + RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1D* h = new TH1D(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + fWidthTable.push_back(h); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to load the data file containing resonance width as a +/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { + if (fFluxDataFile == "") { + RESTError + << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" + << RESTendl; + return; + } + + string fullPathName = SearchFile((string)fPlasmaFreqDataFile); + + RESTDebug << "Loading table from file : " << RESTendl; + RESTDebug << "File : " << fullPathName << RESTendl; + + std::vector> fluxTable; + + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { + fluxTable.clear(); + RESTError << "File is not in binary format!" << RESTendl; + } + + TRestTools::ReadBinaryTable(fullPathName, fluxTable); + + if (fluxTable.size() != 1000 || fluxTable[0].size() != 1) { + fluxTable.clear(); + RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" + << RESTendl; + RESTError << "Table will not be populated" << RESTendl; + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1D* h = new TH1D(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + fPlasmaFreqTable.push_back(h); + } +} + +/////////////////////////////////////////////// +/// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the +/// and the hidden photon mass for chi=1. +/// +void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { + if (GetMass() == 0) { + RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; + return; + } + if (fContinuumTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; + return; + } + if (fPlasmaFreqTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; + return; + } + if (fWidthTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; + return; + } + + Double_t mass = GetMass(); + cout << mass << endl; + for (unsigned int n = 0; n < fContinuumTable.size(); n++) { + // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + + Double_t wp = fPlasmaFreqTable[n]->GetBinContent(1); + TH1D* hMass = new TH1D(Form("%s_hMass%d", GetName(), n), "hMass", 200, 0, 20); + TH1D* hWg2 = (TH1D*)fWidthTable[n]->Clone(); + hWg2->Multiply(hWg2); // (w G)^2 + + for ( unsigned int c; c < 200; c++ ) { + Double_t wG = fWidthTable[n]->GetBinContent(c+1); + hMass->SetBinContent( c+1, pow(mass,-4) * ( pow( pow(mass,2) - pow(wp,2) , 2 )));// + pow(wG,2) ) ); // m2 + } + + hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 + + TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG + h->Multiply(fContinuumTable[n]); // wG * flux + h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + //h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + + fFluxTable.push_back(h); + } +} + +/////////////////////////////////////////////// +/// \brief It builds a histogram with the continuum spectrum. +/// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. +/// +TH1D* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { + if (fContinuumHist != nullptr) { + delete fContinuumHist; + fContinuumHist = nullptr; + } + + fContinuumHist = new TH1D("ContinuumHist", "", 200, 0, 20); + for (const auto& x : fFluxTable) { + fContinuumHist->Add(x); + } + + fContinuumHist->SetStats(0); + fContinuumHist->GetXaxis()->SetTitle("Energy [keV]"); + fContinuumHist->GetXaxis()->SetTitleSize(0.05); + fContinuumHist->GetXaxis()->SetLabelSize(0.05); + fContinuumHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); + fContinuumHist->GetYaxis()->SetTitleSize(0.05); + fContinuumHist->GetYaxis()->SetLabelSize(0.05); + + return fContinuumHist; +} + +/////////////////////////////////////////////// +/// \brief Same as GetContinuumSpectrum, the flux will be +/// expressed in cm-2 s-1 keV-1. Binned in 1eV steps. +/// +TH1D* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { + TH1D* hc = GetContinuumSpectrum(); + + if (fTotalHist != nullptr) { + delete fTotalHist; + fTotalHist = nullptr; + } + + fTotalHist = new TH1D("fTotalHist", "", 20000, 0, 20); + for (int n = 0; n < hc->GetNbinsX(); n++) { + for (int m = 0; m < 100; m++) { + fTotalHist->SetBinContent(n * 100 + 1 + m, hc->GetBinContent(n + 1)); + } + } + + fTotalHist->SetStats(0); + fTotalHist->GetXaxis()->SetTitle("Energy [keV]"); + fTotalHist->GetXaxis()->SetTitleSize(0.05); + fTotalHist->GetXaxis()->SetLabelSize(0.05); + fTotalHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); + fTotalHist->GetYaxis()->SetTitleSize(0.05); + fTotalHist->GetYaxis()->SetLabelSize(0.05); + + return fTotalHist; +} + +/////////////////////////////////////////////// +/// \brief A helper method to initialize the internal class data members with the +/// integrated flux for each solar ring. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. +/// +void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { + fTotalContinuumFlux = 0.0; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + fTotalContinuumFlux += fFluxTable[n]->Integral() * 0.1; // We integrate in 100eV steps + fFluxTableIntegrals.push_back(fTotalContinuumFlux); + } + + for (unsigned int n = 0; n < fFluxTableIntegrals.size(); n++) + fFluxTableIntegrals[n] /= fTotalContinuumFlux; +} + +/////////////////////////////////////////////// +/// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range +/// +Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) { + if (eRange.X() == -1 && eRange.Y() == -1) { + if (GetTotalFlux() == 0) IntegrateSolarFluxes(); + return GetTotalFlux(); + } + + Double_t flux = 0; + fTotalContinuumFlux = 0.0; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + flux += fFluxTable[n]->Integral(fFluxTable[n]->FindFixBin(eRange.X()), + fFluxTable[n]->FindFixBin(eRange.Y())) * + 0.1; // We integrate in 100eV steps + } + + return flux; +} + +/////////////////////////////////////////////// +/// \brief It returns a random solar radius position and energy according to the +/// flux distributions defined inside the solar tables loaded in the class +/// +std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { + + std::pair result = {0, 0}; + if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } + Double_t rnd = fRandom->Rndm(); + for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { + if (rnd < fFluxTableIntegrals[r]) { + Double_t energy = fFluxTable[r]->GetRandom(); + if (eRange.X() != -1 && eRange.Y() != -1) { + if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); + } + Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.001; + std::pair p = {energy, radius}; + return p; + } + } + return result; +} + +/////////////////////////////////////////////// +/// \brief It prints on screen the flux table that has been read from file +/// +void TRestAxionSolarHiddenPhotonFlux::PrintContinuumSolarTable() { + cout << "Continuum solar flux table: " << endl; + cout << "--------------------------- " << endl; + for (unsigned int n = 0; n < fFluxTable.size(); n++) { + for (int m = 0; m < fFluxTable[n]->GetNbinsX(); m++) + cout << fFluxTable[n]->GetBinContent(m + 1) << "\t"; + cout << endl; + cout << endl; + } + cout << endl; +} + +/////////////////////////////////////////////// +/// \brief It prints on screen the integrated solar flux per solar ring +/// +void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { + cout << "Integrated solar flux per solar ring: " << endl; + cout << "--------------------------- " << endl; + /* + for (int n = 0; n < fFluxPerRadius.size(); n++) + cout << "n : " << n << " flux : " << fFluxPerRadius[n] << endl; + cout << endl; + */ +} + +/////////////////////////////////////////////// +/// \brief Prints on screen the information about the metadata members of TRestAxionSolarHiddenPhotonFlux +/// +void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { + TRestAxionSolarFlux::PrintMetadata(); + + RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; + RESTMetadata << "-------" << RESTendl; + RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; + RESTMetadata << "++++++++++++++++++" << RESTendl; + + if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Debug) { + PrintContinuumSolarTable(); + PrintIntegratedRingFlux(); + } +} + +/////////////////////////////////////////////// +/// \brief It will create files with spectra to be used +/// in a later ocasion. +/// +void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { + string rootFilename = TRestTools::GetFileNameRoot(fFluxDataFile); + + string path = REST_USER_PATH + "/export/"; + + if (!TRestTools::fileExists(path)) { + std::cout << "Creating path: " << path << std::endl; + int z = system(("mkdir -p " + path).c_str()); + if (z != 0) RESTError << "Could not create directory " << path << RESTendl; + } + + if (fFluxTable.size() > 0) { + std::vector> table; + for (const auto& x : fFluxTable) { + std::vector row; + for (int n = 0; n < x->GetNbinsX(); n++) row.push_back(x->GetBinContent(n + 1)); + + table.push_back(row); + } + + if (!ascii) + TRestTools::ExportBinaryTable(path + "/" + rootFilename + ".N200f", table); + else + TRestTools::ExportASCIITable(path + "/" + rootFilename + ".dat", table); + } +} + +/////////////////////////////////////////////// +/// \brief It draws the contents of a .flux file. This method just receives the +/// +TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { + if (fCanvas != nullptr) { + delete fCanvas; + fCanvas = nullptr; + } + fCanvas = new TCanvas("canv", "This is the canvas title", 1200, 500); + fCanvas->Draw(); + + TPad* pad1 = new TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97); + pad1->Divide(2, 1); + pad1->Draw(); + + pad1->cd(1); + pad1->cd(1)->SetLogy(); + pad1->cd(1)->SetRightMargin(0.09); + pad1->cd(1)->SetLeftMargin(0.15); + pad1->cd(1)->SetBottomMargin(0.15); + + TH1D* ht = GetTotalSpectrum(); + ht->SetLineColor(kBlack); + ht->SetFillStyle(4050); + ht->SetFillColor(kBlue - 10); + + ht->Draw("hist"); + + pad1->cd(2); + pad1->cd(2)->SetRightMargin(0.09); + pad1->cd(2)->SetLeftMargin(0.15); + pad1->cd(2)->SetBottomMargin(0.15); + + ht->Draw("hist"); + + return fCanvas; +} + diff --git a/src/TRestAxionSolarQCDFlux.cxx b/src/TRestAxionSolarQCDFlux.cxx index 457bd31f..79b5452e 100644 --- a/src/TRestAxionSolarQCDFlux.cxx +++ b/src/TRestAxionSolarQCDFlux.cxx @@ -249,7 +249,7 @@ TRestAxionSolarQCDFlux::~TRestAxionSolarQCDFlux() {} /// \brief It will load the tables in memory by using the filename information provided /// inside the metadata members. /// -Bool_t TRestAxionSolarQCDFlux::LoadTables(Double_t mass) { +Bool_t TRestAxionSolarQCDFlux::LoadTables() { if (fFluxDataFile == "" && fFluxSptFile == "") return false; if (TRestTools::GetFileNameExtension(fFluxDataFile) == "flux") { @@ -265,7 +265,7 @@ Bool_t TRestAxionSolarQCDFlux::LoadTables(Double_t mass) { } /////////////////////////////////////////////// -/// \brief A helper method to load the data file containning continuum spectra as a +/// \brief A helper method to load the data file containing continuum spectra as a /// function of the solar radius. It will be called by TRestAxionSolarQCDFlux::Initialize. /// void TRestAxionSolarQCDFlux::LoadContinuumFluxTable() { @@ -280,7 +280,7 @@ void TRestAxionSolarQCDFlux::LoadContinuumFluxTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; - std::vector> fluxTable; + std::vector> fluxTable; if (TRestTools::GetFileNameExtension(fFluxDataFile) == "dat") { std::vector> doubleTable; if (!TRestTools::ReadASCIITable(fullPathName, doubleTable)) { @@ -289,8 +289,8 @@ void TRestAxionSolarQCDFlux::LoadContinuumFluxTable() { return; } for (const auto& row : doubleTable) { - std::vector floatVec(row.begin(), row.end()); - fluxTable.push_back(floatVec); + std::vector doubleVec(row.begin(), row.end()); + fluxTable.push_back(doubleVec); } } else if (TRestTools::IsBinaryFile(fFluxDataFile)) TRestTools::ReadBinaryTable(fullPathName, fluxTable); @@ -309,14 +309,14 @@ void TRestAxionSolarQCDFlux::LoadContinuumFluxTable() { } for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1F* h = new TH1F(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); + TH1D* h = new TH1D(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); for (unsigned int m = 0; m < fluxTable[n].size(); m++) h->SetBinContent(m + 1, fluxTable[n][m]); fFluxTable.push_back(h); } } /////////////////////////////////////////////// -/// \brief A helper method to load the data file containning monochromatic spectral +/// \brief A helper method to load the data file containing monochromatic spectral /// lines as a function of the solar radius. It will be called by TRestAxionSolarQCDFlux::Initialize. /// void TRestAxionSolarQCDFlux::LoadMonoChromaticFluxTable() { @@ -339,10 +339,10 @@ void TRestAxionSolarQCDFlux::LoadMonoChromaticFluxTable() { return; } - std::vector> asciiTable; + std::vector> asciiTable; for (const auto& row : doubleTable) { - std::vector floatVec(row.begin(), row.end()); - asciiTable.push_back(floatVec); + std::vector doubleVec(row.begin(), row.end()); + asciiTable.push_back(doubleVec); } fFluxLines.clear(); @@ -355,8 +355,8 @@ void TRestAxionSolarQCDFlux::LoadMonoChromaticFluxTable() { } for (unsigned int en = 0; en < asciiTable[0].size(); en++) { - Float_t energy = asciiTable[0][en]; - TH1F* h = new TH1F(Form("%s_MonochromeFluxAtEnergy%6.4lf", GetName(), energy), "", 100, 0, 1); + Double_t energy = asciiTable[0][en]; + TH1D* h = new TH1D(Form("%s_MonochromeFluxAtEnergy%6.4lf", GetName(), energy), "", 100, 0, 1); for (unsigned int r = 1; r < asciiTable.size(); r++) h->SetBinContent(r, asciiTable[r][en]); fFluxLines[energy] = h; } @@ -399,12 +399,12 @@ void TRestAxionSolarQCDFlux::ReadFluxFile() { Double_t fluxBinSize = TRestTools::GetLowestIncreaseFromTable(fluxData, 1); for (const auto& data : fluxData) { - Float_t r = 0.005 + data[0]; - Float_t en = data[1] - 0.005; - Float_t flux = data[2] * fluxBinSize; // flux in cm-2 s-1 bin-1 + Double_t r = 0.005 + data[0]; + Double_t en = data[1] - 0.005; + Double_t flux = data[2] * fluxBinSize; // flux in cm-2 s-1 bin-1 - originalHist->Fill(r, en, (Float_t)flux); - continuumHist->Fill(r, en, (Float_t)flux); + originalHist->Fill(r, en, (Double_t)flux); + continuumHist->Fill(r, en, (Double_t)flux); } RESTDebug << "Histograms filled" << RESTendl; @@ -415,8 +415,8 @@ void TRestAxionSolarQCDFlux::ReadFluxFile() { const int smearPoints = (Int_t)(5 / (fBinSize * 100)); const int excludePoints = smearPoints / 5; for (const auto& data : fluxData) { - Float_t r = 0.005 + data[0]; - Float_t en = data[1] - 0.005; + Double_t r = 0.005 + data[0]; + Double_t en = data[1] - 0.005; Int_t binR = continuumHist->GetXaxis()->FindBin(r); Int_t binE = continuumHist->GetYaxis()->FindBin(en); @@ -430,8 +430,8 @@ void TRestAxionSolarQCDFlux::ReadFluxFile() { } avgFlux /= n; - Float_t targetBinFlux = continuumHist->GetBinContent(binR, binE); - Float_t thrFlux = avgFlux + fPeakSigma * TMath::Sqrt(avgFlux); + Double_t targetBinFlux = continuumHist->GetBinContent(binR, binE); + Double_t thrFlux = avgFlux + fPeakSigma * TMath::Sqrt(avgFlux); if (targetBinFlux > 0 && targetBinFlux > thrFlux) { continuumHist->SetBinContent(binR, binE, avgFlux); peaks++; @@ -441,8 +441,8 @@ void TRestAxionSolarQCDFlux::ReadFluxFile() { for (int n = 0; n < originalHist->GetNbinsX(); n++) for (int m = 0; m < originalHist->GetNbinsY(); m++) { - Float_t orig = originalHist->GetBinContent(n + 1, m + 1); - Float_t cont = continuumHist->GetBinContent(n + 1, m + 1); + Double_t orig = originalHist->GetBinContent(n + 1, m + 1); + Double_t cont = continuumHist->GetBinContent(n + 1, m + 1); spectrumHist->SetBinContent(n + 1, m + 1, orig - cont); } @@ -453,8 +453,8 @@ void TRestAxionSolarQCDFlux::ReadFluxFile() { fFluxTable.clear(); for (int n = 0; n < continuumHist->GetNbinsX(); n++) { - TH1F* hc = - (TH1F*)continuumHist->ProjectionY(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), n + 1, n + 1); + TH1D* hc = + (TH1D*)continuumHist->ProjectionY(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), n + 1, n + 1); fFluxTable.push_back(hc); } @@ -462,7 +462,7 @@ void TRestAxionSolarQCDFlux::ReadFluxFile() { for (int n = 0; n < spectrumHist->GetNbinsY(); n++) { if (spectrumHist->ProjectionX("", n + 1, n + 1)->Integral() > 0) { Double_t energy = spectrumHist->ProjectionY()->GetBinCenter(n + 1); - TH1F* hm = (TH1F*)spectrumHist->ProjectionX( + TH1D* hm = (TH1D*)spectrumHist->ProjectionX( Form("%s_MonochromeFluxAtEnergy%5.3lf", GetName(), energy), n + 1, n + 1); fFluxLines[energy] = hm; } @@ -475,13 +475,13 @@ void TRestAxionSolarQCDFlux::ReadFluxFile() { /// \brief It builds a histogram with the continuum spectrum component. /// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. /// -TH1F* TRestAxionSolarQCDFlux::GetContinuumSpectrum() { +TH1D* TRestAxionSolarQCDFlux::GetContinuumSpectrum() { if (fContinuumHist != nullptr) { delete fContinuumHist; fContinuumHist = nullptr; } - fContinuumHist = new TH1F("ContinuumHist", "", 200, 0, 20); + fContinuumHist = new TH1D("ContinuumHist", "", 200, 0, 20); for (const auto& x : fFluxTable) { fContinuumHist->Add(x); } @@ -501,13 +501,13 @@ TH1F* TRestAxionSolarQCDFlux::GetContinuumSpectrum() { /// \brief It builds a histogram with the monochromatic spectrum component. /// The flux will be expressed in cm-2 s-1 eV-1. Binned in 1eV steps. /// -TH1F* TRestAxionSolarQCDFlux::GetMonochromaticSpectrum() { +TH1D* TRestAxionSolarQCDFlux::GetMonochromaticSpectrum() { if (fMonoHist != nullptr) { delete fMonoHist; fMonoHist = nullptr; } - fMonoHist = new TH1F("MonochromaticHist", "", 20000, 0, 20); + fMonoHist = new TH1D("MonochromaticHist", "", 20000, 0, 20); for (const auto& x : fFluxLines) { fMonoHist->Fill(x.first, x.second->Integral()); // cm-2 s-1 eV-1 } @@ -528,16 +528,16 @@ TH1F* TRestAxionSolarQCDFlux::GetMonochromaticSpectrum() { /// spectrum component. The flux will be expressed in cm-2 s-1 keV-1. /// Binned in 1eV steps. /// -TH1F* TRestAxionSolarQCDFlux::GetTotalSpectrum() { - TH1F* hm = GetMonochromaticSpectrum(); - TH1F* hc = GetContinuumSpectrum(); +TH1D* TRestAxionSolarQCDFlux::GetTotalSpectrum() { + TH1D* hm = GetMonochromaticSpectrum(); + TH1D* hc = GetContinuumSpectrum(); if (fTotalHist != nullptr) { delete fTotalHist; fTotalHist = nullptr; } - fTotalHist = new TH1F("fTotalHist", "", 20000, 0, 20); + fTotalHist = new TH1D("fTotalHist", "", 20000, 0, 20); for (int n = 0; n < hc->GetNbinsX(); n++) { for (int m = 0; m < 100; m++) { fTotalHist->SetBinContent(n * 100 + 1 + m, hc->GetBinContent(n + 1)); @@ -580,12 +580,12 @@ TCanvas* TRestAxionSolarQCDFlux::DrawSolarFlux() { pad1->cd(1)->SetLeftMargin(0.15); pad1->cd(1)->SetBottomMargin(0.15); - TH1F* ht = GetTotalSpectrum(); + TH1D* ht = GetTotalSpectrum(); ht->SetLineColor(kBlack); ht->SetFillStyle(4050); ht->SetFillColor(kBlue - 10); - TH1F* hm = GetMonochromaticSpectrum(); + TH1D* hm = GetMonochromaticSpectrum(); hm->SetLineColor(kBlack); hm->Scale(100); // renormalizing per 100eV-1 @@ -634,7 +634,7 @@ void TRestAxionSolarQCDFlux::IntegrateSolarFluxes() { /////////////////////////////////////////////// /// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range /// -Double_t TRestAxionSolarQCDFlux::IntegrateFluxInRange(TVector2 eRange, Double_t mass) { +Double_t TRestAxionSolarQCDFlux::IntegrateFluxInRange(TVector2 eRange) { if (eRange.X() == -1 && eRange.Y() == -1) { if (GetTotalFlux() == 0) IntegrateSolarFluxes(); return GetTotalFlux(); @@ -770,9 +770,9 @@ void TRestAxionSolarQCDFlux::ExportTables(Bool_t ascii) { } if (fFluxTable.size() > 0) { - std::vector> table; + std::vector> table; for (const auto& x : fFluxTable) { - std::vector row; + std::vector row; for (int n = 0; n < x->GetNbinsX(); n++) row.push_back(x->GetBinContent(n + 1)); table.push_back(row); @@ -785,9 +785,9 @@ void TRestAxionSolarQCDFlux::ExportTables(Bool_t ascii) { } if (fFluxLines.size() > 0) { - std::vector> table; + std::vector> table; for (const auto& x : fFluxLines) { - std::vector row; + std::vector row; row.push_back(x.first); for (int n = 0; n < x.second->GetNbinsX(); n++) row.push_back(x.second->GetBinContent(n + 1)); From 6e94816681a7854ffb1875b48f8d667bb5716776 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Fri, 15 Sep 2023 12:24:50 +0200 Subject: [PATCH 32/48] fixed unspecified int c = 0 --- inc/TRestAxionSolarHiddenPhotonFlux.h | 6 +- inc/TRestAxionSolarHiddenPhotonFlux.h.new | 131 ----- inc/TRestAxionSolarHiddenPhotonFlux.h.old | 131 ----- src/TRestAxionSolarHiddenPhotonFlux.cxx | 76 ++- src/TRestAxionSolarHiddenPhotonFlux.cxx.new | 583 ------------------- src/TRestAxionSolarHiddenPhotonFlux.cxx.old | 613 -------------------- 6 files changed, 56 insertions(+), 1484 deletions(-) delete mode 100644 inc/TRestAxionSolarHiddenPhotonFlux.h.new delete mode 100644 inc/TRestAxionSolarHiddenPhotonFlux.h.old delete mode 100644 src/TRestAxionSolarHiddenPhotonFlux.cxx.new delete mode 100644 src/TRestAxionSolarHiddenPhotonFlux.cxx.old diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index 2df02f96..bdc44040 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -45,13 +45,13 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { std::vector fFluxTable; //! /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector> fContinuumTable; //! + std::vector fContinuumTable; //! /// The tabulated resonance width TH1D(200,0,20)keV in eV2 versus solar radius - std::vector> fWidthTable; //! + std::vector fWidthTable; //! /// The solar plasma frequency vector in eV versus solar radius - std::vector> fPlasmaFreqTable; //! + std::vector fPlasmaFreqTable; //! /// The total solar flux TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius std::vector fFullFluxTable; //! diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h.new b/inc/TRestAxionSolarHiddenPhotonFlux.h.new deleted file mode 100644 index 2df02f96..00000000 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h.new +++ /dev/null @@ -1,131 +0,0 @@ -/************************************************************************* - * This file is part of the REST software framework. * - * * - * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * - * For more information see http://gifna.unizar.es/trex * - * * - * REST is free software: you can redistribute it and/or modify * - * it under the terms of the GNU General Public License as published by * - * the Free Software Foundation, either version 3 of the License, or * - * (at your option) any later version. * - * * - * REST is distributed in the hope that it will be useful, * - * but WITHOUT ANY WARRANTY; without even the implied warranty of * - * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * - * GNU General Public License for more details. * - * * - * You should have a copy of the GNU General Public License along with * - * REST in $REST_PATH/LICENSE. * - * If not, see http://www.gnu.org/licenses/. * - * For the list of contributors see $REST_PATH/CREDITS. * - *************************************************************************/ - -#ifndef _TRestAxionSolarHiddenPhotonFlux -#define _TRestAxionSolarHiddenPhotonFlux - -#include -#include - -//! A metadata class to load tabulated solar hidden photon fluxes. Kinetic mixing set to 1. -class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { - private: - /// The filename containing the solar flux table with continuum spectrum - std::string fFluxDataFile = ""; //< - - /// The filename containing the resonance width (wGamma) - std::string fWidthDataFile = ""; //< - - /// The filename containing the plasma frequency (wp) table - std::string fPlasmaFreqDataFile = ""; //< - - /// It will be used when loading `.flux` files to define the input file energy binsize in eV. - Double_t fBinSize = 0; //< - - /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fFluxTable; //! - - /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector> fContinuumTable; //! - - /// The tabulated resonance width TH1D(200,0,20)keV in eV2 versus solar radius - std::vector> fWidthTable; //! - - /// The solar plasma frequency vector in eV versus solar radius - std::vector> fPlasmaFreqTable; //! - - /// The total solar flux TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fFullFluxTable; //! - - /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) - std::vector fFluxTableIntegrals; //! - - /// Total solar flux for monochromatic contributions - Double_t fTotalContinuumFlux = 0; //! - - /// A pointer to the continuum spectrum histogram - TH1D* fContinuumHist = nullptr; //! - - /// A pointer to the superposed monochromatic and continuum spectrum histogram - TH1D* fTotalHist = nullptr; //! - - void ReadFluxFile(); - void LoadContinuumFluxTable(); - void LoadMonoChromaticFluxTable(); - void IntegrateSolarFluxes(); - - public: - /// It returns true if continuum flux spectra was loaded - Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } - - /// It returns true if width table was loaded - Bool_t isWidthTableLoaded() { return fWidthTable.size() > 0; } - - /// It returns true if plasma frequency table was loaded - Bool_t isPlasmaFreqLoaded() { return fPlasmaFreqTable.size() > 0; } - - /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range - Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; - - /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; - - /// It defines how to read the solar tables at the inhereted class for a given mass in eV - Bool_t LoadTables() override; - - void LoadContinuumTable(); - void LoadWidthTable(); - void LoadPlasmaFreqTable(); - - // calculate solar HP flux from the 3 tables and mass - void CalculateSolarFlux(); - /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux() override { return fTotalContinuumFlux; } - - /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 - TH1D* GetEnergySpectrum() override { return GetTotalSpectrum(); } - - TH1D* GetContinuumSpectrum(); - TH1D* GetTotalSpectrum(); - - virtual TCanvas* DrawSolarFlux() override; - - /// Tables might be loaded using a solar model description by TRestAxionSolarModel - void InitializeSolarTable(TRestAxionSolarModel* model) { - // TOBE implemented - // This method should initialize the tables fFluxTable and fFluxLines - } - - void ExportTables(Bool_t ascii = false) override; - - void PrintMetadata() override; - - void PrintContinuumSolarTable(); - void PrintIntegratedRingFlux(); - - TRestAxionSolarHiddenPhotonFlux(); - TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, std::string name = ""); - ~TRestAxionSolarHiddenPhotonFlux(); - - ClassDefOverride(TRestAxionSolarHiddenPhotonFlux, 1); -}; -#endif diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h.old b/inc/TRestAxionSolarHiddenPhotonFlux.h.old deleted file mode 100644 index bdc44040..00000000 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h.old +++ /dev/null @@ -1,131 +0,0 @@ -/************************************************************************* - * This file is part of the REST software framework. * - * * - * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * - * For more information see http://gifna.unizar.es/trex * - * * - * REST is free software: you can redistribute it and/or modify * - * it under the terms of the GNU General Public License as published by * - * the Free Software Foundation, either version 3 of the License, or * - * (at your option) any later version. * - * * - * REST is distributed in the hope that it will be useful, * - * but WITHOUT ANY WARRANTY; without even the implied warranty of * - * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * - * GNU General Public License for more details. * - * * - * You should have a copy of the GNU General Public License along with * - * REST in $REST_PATH/LICENSE. * - * If not, see http://www.gnu.org/licenses/. * - * For the list of contributors see $REST_PATH/CREDITS. * - *************************************************************************/ - -#ifndef _TRestAxionSolarHiddenPhotonFlux -#define _TRestAxionSolarHiddenPhotonFlux - -#include -#include - -//! A metadata class to load tabulated solar hidden photon fluxes. Kinetic mixing set to 1. -class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { - private: - /// The filename containing the solar flux table with continuum spectrum - std::string fFluxDataFile = ""; //< - - /// The filename containing the resonance width (wGamma) - std::string fWidthDataFile = ""; //< - - /// The filename containing the plasma frequency (wp) table - std::string fPlasmaFreqDataFile = ""; //< - - /// It will be used when loading `.flux` files to define the input file energy binsize in eV. - Double_t fBinSize = 0; //< - - /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fFluxTable; //! - - /// The tabulated solar flux continuum spectra TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fContinuumTable; //! - - /// The tabulated resonance width TH1D(200,0,20)keV in eV2 versus solar radius - std::vector fWidthTable; //! - - /// The solar plasma frequency vector in eV versus solar radius - std::vector fPlasmaFreqTable; //! - - /// The total solar flux TH1D(200,0,20)keV in cm-2 s-1 keV-1 versus solar radius - std::vector fFullFluxTable; //! - - /// Accumulative integrated solar flux for each solar ring for continuum spectrum (renormalized to unity) - std::vector fFluxTableIntegrals; //! - - /// Total solar flux for monochromatic contributions - Double_t fTotalContinuumFlux = 0; //! - - /// A pointer to the continuum spectrum histogram - TH1D* fContinuumHist = nullptr; //! - - /// A pointer to the superposed monochromatic and continuum spectrum histogram - TH1D* fTotalHist = nullptr; //! - - void ReadFluxFile(); - void LoadContinuumFluxTable(); - void LoadMonoChromaticFluxTable(); - void IntegrateSolarFluxes(); - - public: - /// It returns true if continuum flux spectra was loaded - Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } - - /// It returns true if width table was loaded - Bool_t isWidthTableLoaded() { return fWidthTable.size() > 0; } - - /// It returns true if plasma frequency table was loaded - Bool_t isPlasmaFreqLoaded() { return fPlasmaFreqTable.size() > 0; } - - /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range - Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) override; - - /// It defines how to generate Monte Carlo energy and radius values to reproduce the flux - std::pair GetRandomEnergyAndRadius(TVector2 eRange = TVector2(-1, -1)) override; - - /// It defines how to read the solar tables at the inhereted class for a given mass in eV - Bool_t LoadTables() override; - - void LoadContinuumTable(); - void LoadWidthTable(); - void LoadPlasmaFreqTable(); - - // calculate solar HP flux from the 3 tables and mass - void CalculateSolarFlux(); - /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux() override { return fTotalContinuumFlux; } - - /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 - TH1D* GetEnergySpectrum() override { return GetTotalSpectrum(); } - - TH1D* GetContinuumSpectrum(); - TH1D* GetTotalSpectrum(); - - virtual TCanvas* DrawSolarFlux() override; - - /// Tables might be loaded using a solar model description by TRestAxionSolarModel - void InitializeSolarTable(TRestAxionSolarModel* model) { - // TOBE implemented - // This method should initialize the tables fFluxTable and fFluxLines - } - - void ExportTables(Bool_t ascii = false) override; - - void PrintMetadata() override; - - void PrintContinuumSolarTable(); - void PrintIntegratedRingFlux(); - - TRestAxionSolarHiddenPhotonFlux(); - TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, std::string name = ""); - ~TRestAxionSolarHiddenPhotonFlux(); - - ClassDefOverride(TRestAxionSolarHiddenPhotonFlux, 1); -}; -#endif diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 01f443fa..0c213f20 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -230,18 +230,26 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; + std::vector> fluxTable; + if (!TRestTools::IsBinaryFile(fFluxDataFile)) { - fContinuumTable.clear(); + fluxTable.clear(); RESTError << "File is not in binary format!" << RESTendl; } - TRestTools::ReadBinaryTable(fullPathName, fContinuumTable); + TRestTools::ReadBinaryTable(fullPathName, fluxTable); - if (fContinuumTable.size() != 1000 || fContinuumTable[0].size() != 200) { + if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { + fluxTable.clear(); RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; - fContinuumTable.clear(); + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1D* h = new TH1D(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + fContinuumTable.push_back(h); } } @@ -261,18 +269,27 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; + std::vector> fluxTable; + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { - fWidthTable.clear(); + fluxTable.clear(); RESTError << "File is not in binary format!" << RESTendl; } - TRestTools::ReadBinaryTable(fullPathName, fWidthTable); + TRestTools::ReadBinaryTable(fullPathName, fluxTable); + //RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << RESTendl; - if (fWidthTable.size() != 1000 || fWidthTable[0].size() != 200) { + if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { + fluxTable.clear(); RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; - fWidthTable.clear(); + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1D* h = new TH1D(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + fWidthTable.push_back(h); } } @@ -293,18 +310,26 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { RESTDebug << "Loading table from file : " << RESTendl; RESTDebug << "File : " << fullPathName << RESTendl; + std::vector> fluxTable; + if (!TRestTools::IsBinaryFile(fWidthDataFile)) { + fluxTable.clear(); RESTError << "File is not in binary format!" << RESTendl; - fPlasmaFreqTable.clear(); } - TRestTools::ReadBinaryTable(fullPathName, fPlasmaFreqTable); + TRestTools::ReadBinaryTable(fullPathName, fluxTable); - if (fPlasmaFreqTable.size() != 1000 || fPlasmaFreqTable[0].size() != 1) { + if (fluxTable.size() != 1000 || fluxTable[0].size() != 1) { + fluxTable.clear(); RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" << RESTendl; RESTError << "Table will not be populated" << RESTendl; - fPlasmaFreqTable.clear(); + } + + for (unsigned int n = 0; n < fluxTable.size(); n++) { + TH1D* h = new TH1D(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + fPlasmaFreqTable.push_back(h); } } @@ -331,22 +356,27 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { } Double_t mass = GetMass(); + cout << mass << endl; for (unsigned int n = 0; n < fContinuumTable.size(); n++) { // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - Double_t wp = fPlasmaFreqTable[n][0]; - vector wG = fWidthTable[n]; - vector flux = fContinuumTable[n]; - vector v; - for( unsigned int c; c < wG.size(); c++ ) { - Double_t d1 = ( wG[c] * flux[c] * pow(mass,4) ); // m4 * wG * flux - Double_t d2 = ( pow( pow(mass,2) - pow(wp,2) , 2 ) + pow(wG[c],2) ); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - v.push_back(d1/d2); + Double_t wp = fPlasmaFreqTable[n]->GetBinContent(1); + TH1D* hMass = new TH1D(Form("%s_hMass%d", GetName(), n), "hMass", 200, 0, 20); + TH1D* hWg2 = (TH1D*)fWidthTable[n]->Clone(); + hWg2->Multiply(hWg2); // (w G)^2 + + for ( unsigned int c = 0; c < 200; c++ ) { + Double_t wG = fWidthTable[n]->GetBinContent(c+1); + hMass->SetBinContent( c+1, pow(mass,-4) * ( pow( pow(mass,2) - pow(wp,2) , 2 )));// + pow(wG,2) ) ); // m2 } + + hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 + + TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG + h->Multiply(fContinuumTable[n]); // wG * flux + h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + //h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - TH1D* h = new TH1D(Form("%s_TotalFluxTable%d", GetName(), n), "", 200, 0, 20); - for (unsigned int c = 0; c < v.size(); c++) { h->SetBinContent(c + 1, v[c]); } - //for (unsigned int c = 0; c < v.size(); c++) { h->Fill(v[c]); } fFluxTable.push_back(h); } } diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx.new b/src/TRestAxionSolarHiddenPhotonFlux.cxx.new deleted file mode 100644 index 26c782c1..00000000 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx.new +++ /dev/null @@ -1,583 +0,0 @@ -/******************** REST disclaimer *********************************** - * This file is part of the REST software framework. * - * * - * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * - * For more information see http://gifna.unizar.es/trex * - * * - * REST is free software: you can redistribute it and/or modify * - * it under the terms of the GNU General Public License as published by * - * the Free Software Foundation, either version 3 of the License, or * - * (at your option) any later version. * - * * - * REST is distributed in the hope that it will be useful, * - * but WITHOUT ANY WARRANTY; without even the implied warranty of * - * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * - * GNU General Public License for more details. * - * * - * You should have a copy of the GNU General Public License along with * - * REST in $REST_PATH/LICENSE. * - * If not, see http://www.gnu.org/licenses/. * - * For the list of contributors see $REST_PATH/CREDITS. * - *************************************************************************/ - -////////////////////////////////////////////////////////////////////////// -/// TRestAxionSolarHiddenPhotonFlux will use a file in binary format to initialize -/// a solar flux table that will describe the solar hidden photon flux spectrum as a function -/// of the solar radius. -/// -/// This class loads the hidden photon flux that depends on the mass and kinetic mixing parameter. -/// For axion-like particle prodution independent of mass there is the class -/// TRestAxionSolarQCDFlux. Both classes are prototyped by a pure base class TRestAxionSolarFlux -/// that defines common methods used to evaluate the flux, and generate Monte-Carlo events inside -/// TRestAxionGeneratorProcess. -/// -/// ### Basic use -/// -/// Once the class has been initialized, the main use of this class will be provided -/// by the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. This method will -/// return a random axion energy and position inside the solar radius following the -/// distributions given by the solar flux tables. -/// -/// Description of the specific parameters accepted by this metadata class. -/// - *fluxDataFile:* A table with 1000 rows representing the solar ring flux from the -/// center to the corona, and 200 columns representing the flux, measured in cm-2 s-1 keV-1, -/// for the range (0,20)keV in steps of 100eV. The table is provided as a binary table using -/// `.N200f` extension. -/// - *widthDataFile:* A table with 1000 rows representing the width of the hidden photon -/// resonant production (wG) for each solar ring from the center to the corona, and 200 columns -/// representing the width, measured in eV2, for the range (0,20)keV in steps of 100eV. The -/// table is provided as a binary table using `.N200f` extension. -/// - *plasmaFreqDataFile:* A table with 1000 rows and only 1 column representing the solar -/// plasma frequency (wp) for each solar ring from the center to the corona, measured in eV. The -/// table is provided as a binary table using `.N1f` extension. -/// -/// Pre-generated solar axion flux tables will be available at the -/// [axionlib-data](https://github.com/rest-for-physics/axionlib-data/tree/master) -/// repository. The different RML flux definitions used to load those tables -/// will be found at the -/// [fluxes.rml](https://github.com/rest-for-physics/axionlib-data/blob/master/solarFlux/fluxes.rml) -/// file found at the axionlib-data repository. -/// -/// Inside a local REST installation, the `fluxes.rml` file will be found at the REST -/// installation directory, and it will be located automatically by the -/// TRestMetadata::SearchFile method. -/// -/// ### A basic RML definition -/// -/// The following definition integrates an axion-photon component with a continuum -/// spectrum using a Primakoff production model, and a dummy spectrum file that -/// includes two monocrhomatic lines at different solar disk radius positions. -/// -/// \code -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// \endcode -/// -/// \warning When the flux is loaded manually inside the `restRoot` interactive -/// shell, or inside a macro or script, after metadata initialization, it is necessary -/// to call the method TRestAxionSolarHiddenPhotonFlux::LoadTables(mass) to trigger the tables -/// initialization. -/// -/// ### Performing MonteCarlo tests using pre-loaded tables -/// -/// In order to test the response of different solar flux definitions we may use the script -/// `solarPlot.py` found at `pipeline/metadata/solarFlux/`. This script will generate a -/// number of particles and it will assign to each particle an energy and solar disk -/// location with the help of the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. -/// -/// \code -/// python3 solarPlotHiddenPhoton.py --fluxname HiddenPhoton --N 1000000 -/// \endcode -/// -/// By default, it will load the flux definition found at `fluxes.rml` from the -/// `axionlib-data` repository, and generate a `png` image with the resuts from the -/// Monte Carlo execution. -/// -/// \htmlonly \endhtmlonly -/// -/// ![Solar flux distributions MC-generated with TRestAxionSolarQCDFlux.](ABC_flux_MC.png) -/// -/// ### Exporting the solar flux tables -/// -/// On top of that, we will be able to export those tables to the TRestAxionSolarHiddenPhotonFlux -/// standard format to be used in later occasions. -/// -/// \code -/// TRestAxionSolarHiddenPhotonFlux *sFlux = new TRestAxionSolarHiddenPhotonFlux("fluxes.rml", -/// "HiddenPhoton") sFlux->Initialize() sFlux->ExportTables() -/// \endcode -/// -/// which will produce a binary table `.N200f` with the continuum flux. The filename root will be -/// extracted from the original `.flux` file. Optionally we may export the continuum flux to an -/// ASCII file by indicating it at the TRestAxionSolarHiddenPhotonFlux::ExportTables method call. -/// The files will be placed at the REST user space, at `$HOME/.rest/export/` directory. -/// -/// TODO Implement the method TRestAxionSolarQCDFlux::InitializeSolarTable using -/// a solar model description by TRestAxionSolarModel. -/// -/// TODO Perhaps it would be interesting to replace fFluxTable for a TH2D -/// -///-------------------------------------------------------------------------- -/// -/// RESTsoft - Software for Rare Event Searches with TPCs -/// -/// History of developments: -/// -/// 2023-May: Specific methods extracted from TRestAxionSolarFlux -/// Javier Galan -/// 2023-June: TRestAxionSolarHiddenPhotonFlux created by editing TRestAxionSolarQCDFlux -/// Tomas O'Shea -/// -/// \class TRestAxionSolarHiddenPhotonFlux -/// \author Javier Galan -/// -///
-/// - -#include "TRestAxionSolarHiddenPhotonFlux.h" -using namespace std; - -ClassImp(TRestAxionSolarHiddenPhotonFlux); - -/////////////////////////////////////////////// -/// \brief Default constructor -/// -TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux() : TRestAxionSolarFlux() {} - -/////////////////////////////////////////////// -/// \brief Constructor loading data from a config file -/// -/// If no configuration path is defined using TRestMetadata::SetConfigFilePath -/// the path to the config file must be specified using full path, absolute or -/// relative. -/// -/// The default behaviour is that the config file must be specified with -/// full path, absolute or relative. -/// -/// \param cfgFileName A const char* giving the path to an RML file. -/// \param name The name of the specific metadata. It will be used to find the -/// corresponding TRestAxionMagneticField section inside the RML. -/// -TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, string name) - : TRestAxionSolarFlux(cfgFileName) { - LoadConfigFromFile(fConfigFileName, name); - - if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Info) PrintMetadata(); -} - -/////////////////////////////////////////////// -/// \brief Default destructor -/// -TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} - -/////////////////////////////////////////////// -/// \brief It will load the tables in memory by using the filename information provided -/// inside the metadata members, and calculate the solar flux for a given m. -/// -Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - - if (GetMass() <= 0 ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; - return false; - } - if ( fFluxDataFile == "" ){ - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; - return false; - } - if ( fWidthDataFile == "") { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; - return false; - } - if ( fPlasmaFreqDataFile == "" ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; - return false; - } - - LoadContinuumFluxTable(); - LoadWidthTable(); - LoadPlasmaFreqTable(); - - CalculateSolarFlux(); - - IntegrateSolarFluxes(); - return true; -} - -/////////////////////////////////////////////// -/// \brief A helper method to load the data file containing continuum spectra as a -/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { - if (fFluxDataFile == "") { - RESTError - << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" - << RESTendl; - return; - } - - string fullPathName = SearchFile((string)fFluxDataFile); - - RESTDebug << "Loading table from file : " << RESTendl; - RESTDebug << "File : " << fullPathName << RESTendl; - - if (!TRestTools::IsBinaryFile(fFluxDataFile)) { - fContinuumTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; - } - - TRestTools::ReadBinaryTable(fullPathName, fContinuumTable); - - if (fContinuumTable.size() != 1000 || fContinuumTable[0].size() != 200) { - RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows or columns" - << RESTendl; - RESTError << "Table will not be populated" << RESTendl; - fContinuumTable.clear(); - } -} - -/////////////////////////////////////////////// -/// \brief A helper method to load the data file containing resonance width as a -/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { - if (fFluxDataFile == "") { - RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadWidthTable. No width table was defined" - << RESTendl; - return; - } - - string fullPathName = SearchFile((string)fWidthDataFile); - - RESTDebug << "Loading table from file : " << RESTendl; - RESTDebug << "File : " << fullPathName << RESTendl; - - if (!TRestTools::IsBinaryFile(fWidthDataFile)) { - fWidthTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; - } - - TRestTools::ReadBinaryTable(fullPathName, fWidthTable); - - if (fWidthTable.size() != 1000 || fWidthTable[0].size() != 200) { - RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" - << RESTendl; - RESTError << "Table will not be populated" << RESTendl; - fWidthTable.clear(); - } -} - -/////////////////////////////////////////////// -/// \brief A helper method to load the data file containing resonance width as a -/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { - if (fFluxDataFile == "") { - RESTError - << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" - << RESTendl; - return; - } - - string fullPathName = SearchFile((string)fPlasmaFreqDataFile); - - RESTDebug << "Loading table from file : " << RESTendl; - RESTDebug << "File : " << fullPathName << RESTendl; - - if (!TRestTools::IsBinaryFile(fWidthDataFile)) { - RESTError << "File is not in binary format!" << RESTendl; - fPlasmaFreqTable.clear(); - } - - TRestTools::ReadBinaryTable(fullPathName, fPlasmaFreqTable); - - if (fPlasmaFreqTable.size() != 1000 || fPlasmaFreqTable[0].size() != 1) { - RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" - << RESTendl; - RESTError << "Table will not be populated" << RESTendl; - fPlasmaFreqTable.clear(); - } -} - -/////////////////////////////////////////////// -/// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the -/// and the hidden photon mass for chi=1. -/// -void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { - if (GetMass() == 0) { - RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; - return; - } - if (fContinuumTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; - return; - } - if (fPlasmaFreqTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; - return; - } - if (fWidthTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; - return; - } - fFluxTable.clear(); - Double_t mass = GetMass(); - for (unsigned int n = 0; n < fContinuumTable.size(); n++) { - // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - - Double_t wp = fPlasmaFreqTable[n][0]; - vector wG = fWidthTable[n]; - vector flux = fContinuumTable[n]; - vector v; - for( unsigned int c; c < wG.size(); c++ ) { - Double_t d1 = ( wG[c] * flux[c] * pow(mass,4) ); // m4 * wG * flux - Double_t d2 = ( pow( pow(mass,2) - pow(wp,2) , 2 ) + pow(wG[c],2) ); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - v.push_back(d1/d2); - } - - TH1D* h = new TH1D(Form("%s_TotalFluxTable%d", GetName(), n), "", 200, 0, 20); - for (unsigned int c = 0; c < v.size(); c++) { h->SetBinContent(c + 1, v[c]); } - //for (unsigned int c = 0; c < v.size(); c++) { h->Fill(v[c]); } - fFluxTable.push_back(h); - } -} - -/////////////////////////////////////////////// -/// \brief It builds a histogram with the continuum spectrum. -/// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. -/// -TH1D* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { - if (fContinuumHist != nullptr) { - delete fContinuumHist; - fContinuumHist = nullptr; - } - - fContinuumHist = new TH1D("ContinuumHist", "", 200, 0, 20); - for (const auto& x : fFluxTable) { - fContinuumHist->Add(x); - } - - fContinuumHist->SetStats(0); - fContinuumHist->GetXaxis()->SetTitle("Energy [keV]"); - fContinuumHist->GetXaxis()->SetTitleSize(0.05); - fContinuumHist->GetXaxis()->SetLabelSize(0.05); - fContinuumHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); - fContinuumHist->GetYaxis()->SetTitleSize(0.05); - fContinuumHist->GetYaxis()->SetLabelSize(0.05); - - return fContinuumHist; -} - -/////////////////////////////////////////////// -/// \brief Same as GetContinuumSpectrum, the flux will be -/// expressed in cm-2 s-1 keV-1. Binned in 1eV steps. -/// -TH1D* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { - TH1D* hc = GetContinuumSpectrum(); - - if (fTotalHist != nullptr) { - delete fTotalHist; - fTotalHist = nullptr; - } - - fTotalHist = new TH1D("fTotalHist", "", 20000, 0, 20); - for (int n = 0; n < hc->GetNbinsX(); n++) { - for (int m = 0; m < 100; m++) { - fTotalHist->SetBinContent(n * 100 + 1 + m, hc->GetBinContent(n + 1)); - } - } - - fTotalHist->SetStats(0); - fTotalHist->GetXaxis()->SetTitle("Energy [keV]"); - fTotalHist->GetXaxis()->SetTitleSize(0.05); - fTotalHist->GetXaxis()->SetLabelSize(0.05); - fTotalHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); - fTotalHist->GetYaxis()->SetTitleSize(0.05); - fTotalHist->GetYaxis()->SetLabelSize(0.05); - - return fTotalHist; -} - -/////////////////////////////////////////////// -/// \brief A helper method to initialize the internal class data members with the -/// integrated flux for each solar ring. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { - fTotalContinuumFlux = 0.0; - for (unsigned int n = 0; n < fFluxTable.size(); n++) { - fTotalContinuumFlux += fFluxTable[n]->Integral() * 0.1; // We integrate in 100eV steps - fFluxTableIntegrals.push_back(fTotalContinuumFlux); - } - - for (unsigned int n = 0; n < fFluxTableIntegrals.size(); n++) - fFluxTableIntegrals[n] /= fTotalContinuumFlux; -} - -/////////////////////////////////////////////// -/// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range -/// -Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) { - if (eRange.X() == -1 && eRange.Y() == -1) { - if (GetTotalFlux() == 0) IntegrateSolarFluxes(); - return GetTotalFlux(); - } - - Double_t flux = 0; - fTotalContinuumFlux = 0.0; - for (unsigned int n = 0; n < fFluxTable.size(); n++) { - flux += fFluxTable[n]->Integral(fFluxTable[n]->FindFixBin(eRange.X()), - fFluxTable[n]->FindFixBin(eRange.Y())) * - 0.1; // We integrate in 100eV steps - } - - return flux; -} - -/////////////////////////////////////////////// -/// \brief It returns a random solar radius position and energy according to the -/// flux distributions defined inside the solar tables loaded in the class -/// -std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { - - std::pair result = {0, 0}; - if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } - Double_t rnd = fRandom->Rndm(); - for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { - if (rnd < fFluxTableIntegrals[r]) { - Double_t energy = fFluxTable[r]->GetRandom(); - if (eRange.X() != -1 && eRange.Y() != -1) { - if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); - } - Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.001; - std::pair p = {energy, radius}; - return p; - } - } - return result; -} - -/////////////////////////////////////////////// -/// \brief It prints on screen the flux table that has been read from file -/// -void TRestAxionSolarHiddenPhotonFlux::PrintContinuumSolarTable() { - cout << "Continuum solar flux table: " << endl; - cout << "--------------------------- " << endl; - for (unsigned int n = 0; n < fFluxTable.size(); n++) { - for (int m = 0; m < fFluxTable[n]->GetNbinsX(); m++) - cout << fFluxTable[n]->GetBinContent(m + 1) << "\t"; - cout << endl; - cout << endl; - } - cout << endl; -} - -/////////////////////////////////////////////// -/// \brief It prints on screen the integrated solar flux per solar ring -/// -void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { - cout << "Integrated solar flux per solar ring: " << endl; - cout << "--------------------------- " << endl; - /* - for (int n = 0; n < fFluxPerRadius.size(); n++) - cout << "n : " << n << " flux : " << fFluxPerRadius[n] << endl; - cout << endl; - */ -} - -/////////////////////////////////////////////// -/// \brief Prints on screen the information about the metadata members of TRestAxionSolarHiddenPhotonFlux -/// -void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { - TRestAxionSolarFlux::PrintMetadata(); - - RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; - RESTMetadata << "-------" << RESTendl; - RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; - RESTMetadata << "++++++++++++++++++" << RESTendl; - - if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Debug) { - PrintContinuumSolarTable(); - PrintIntegratedRingFlux(); - } -} - -/////////////////////////////////////////////// -/// \brief It will create files with spectra to be used -/// in a later ocasion. -/// -void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { - string rootFilename = TRestTools::GetFileNameRoot(fFluxDataFile); - - string path = REST_USER_PATH + "/export/"; - - if (!TRestTools::fileExists(path)) { - std::cout << "Creating path: " << path << std::endl; - int z = system(("mkdir -p " + path).c_str()); - if (z != 0) RESTError << "Could not create directory " << path << RESTendl; - } - - if (fFluxTable.size() > 0) { - std::vector> table; - for (const auto& x : fFluxTable) { - std::vector row; - for (int n = 0; n < x->GetNbinsX(); n++) row.push_back(x->GetBinContent(n + 1)); - - table.push_back(row); - } - - if (!ascii) - TRestTools::ExportBinaryTable(path + "/" + rootFilename + ".N200f", table); - else - TRestTools::ExportASCIITable(path + "/" + rootFilename + ".dat", table); - } -} - -/////////////////////////////////////////////// -/// \brief It draws the contents of a .flux file. This method just receives the -/// -TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { - if (fCanvas != nullptr) { - delete fCanvas; - fCanvas = nullptr; - } - fCanvas = new TCanvas("canv", "This is the canvas title", 1200, 500); - fCanvas->Draw(); - - TPad* pad1 = new TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97); - pad1->Divide(2, 1); - pad1->Draw(); - - pad1->cd(1); - pad1->cd(1)->SetLogy(); - pad1->cd(1)->SetRightMargin(0.09); - pad1->cd(1)->SetLeftMargin(0.15); - pad1->cd(1)->SetBottomMargin(0.15); - - TH1D* ht = GetTotalSpectrum(); - ht->SetLineColor(kBlack); - ht->SetFillStyle(4050); - ht->SetFillColor(kBlue - 10); - - ht->Draw("hist"); - - pad1->cd(2); - pad1->cd(2)->SetRightMargin(0.09); - pad1->cd(2)->SetLeftMargin(0.15); - pad1->cd(2)->SetBottomMargin(0.15); - - ht->Draw("hist"); - - return fCanvas; -} - diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx.old b/src/TRestAxionSolarHiddenPhotonFlux.cxx.old deleted file mode 100644 index e61f0630..00000000 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx.old +++ /dev/null @@ -1,613 +0,0 @@ -/******************** REST disclaimer *********************************** - * This file is part of the REST software framework. * - * * - * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * - * For more information see http://gifna.unizar.es/trex * - * * - * REST is free software: you can redistribute it and/or modify * - * it under the terms of the GNU General Public License as published by * - * the Free Software Foundation, either version 3 of the License, or * - * (at your option) any later version. * - * * - * REST is distributed in the hope that it will be useful, * - * but WITHOUT ANY WARRANTY; without even the implied warranty of * - * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * - * GNU General Public License for more details. * - * * - * You should have a copy of the GNU General Public License along with * - * REST in $REST_PATH/LICENSE. * - * If not, see http://www.gnu.org/licenses/. * - * For the list of contributors see $REST_PATH/CREDITS. * - *************************************************************************/ - -////////////////////////////////////////////////////////////////////////// -/// TRestAxionSolarHiddenPhotonFlux will use a file in binary format to initialize -/// a solar flux table that will describe the solar hidden photon flux spectrum as a function -/// of the solar radius. -/// -/// This class loads the hidden photon flux that depends on the mass and kinetic mixing parameter. -/// For axion-like particle prodution independent of mass there is the class -/// TRestAxionSolarQCDFlux. Both classes are prototyped by a pure base class TRestAxionSolarFlux -/// that defines common methods used to evaluate the flux, and generate Monte-Carlo events inside -/// TRestAxionGeneratorProcess. -/// -/// ### Basic use -/// -/// Once the class has been initialized, the main use of this class will be provided -/// by the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. This method will -/// return a random axion energy and position inside the solar radius following the -/// distributions given by the solar flux tables. -/// -/// Description of the specific parameters accepted by this metadata class. -/// - *fluxDataFile:* A table with 1000 rows representing the solar ring flux from the -/// center to the corona, and 200 columns representing the flux, measured in cm-2 s-1 keV-1, -/// for the range (0,20)keV in steps of 100eV. The table is provided as a binary table using -/// `.N200f` extension. -/// - *widthDataFile:* A table with 1000 rows representing the width of the hidden photon -/// resonant production (wG) for each solar ring from the center to the corona, and 200 columns -/// representing the width, measured in eV2, for the range (0,20)keV in steps of 100eV. The -/// table is provided as a binary table using `.N200f` extension. -/// - *plasmaFreqDataFile:* A table with 1000 rows and only 1 column representing the solar -/// plasma frequency (wp) for each solar ring from the center to the corona, measured in eV. The -/// table is provided as a binary table using `.N1f` extension. -/// -/// Pre-generated solar axion flux tables will be available at the -/// [axionlib-data](https://github.com/rest-for-physics/axionlib-data/tree/master) -/// repository. The different RML flux definitions used to load those tables -/// will be found at the -/// [fluxes.rml](https://github.com/rest-for-physics/axionlib-data/blob/master/solarFlux/fluxes.rml) -/// file found at the axionlib-data repository. -/// -/// Inside a local REST installation, the `fluxes.rml` file will be found at the REST -/// installation directory, and it will be located automatically by the -/// TRestMetadata::SearchFile method. -/// -/// ### A basic RML definition -/// -/// The following definition integrates an axion-photon component with a continuum -/// spectrum using a Primakoff production model, and a dummy spectrum file that -/// includes two monocrhomatic lines at different solar disk radius positions. -/// -/// \code -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// -/// \endcode -/// -/// \warning When the flux is loaded manually inside the `restRoot` interactive -/// shell, or inside a macro or script, after metadata initialization, it is necessary -/// to call the method TRestAxionSolarHiddenPhotonFlux::LoadTables(mass) to trigger the tables -/// initialization. -/// -/// ### Performing MonteCarlo tests using pre-loaded tables -/// -/// In order to test the response of different solar flux definitions we may use the script -/// `solarPlot.py` found at `pipeline/metadata/solarFlux/`. This script will generate a -/// number of particles and it will assign to each particle an energy and solar disk -/// location with the help of the method TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius. -/// -/// \code -/// python3 solarPlotHiddenPhoton.py --fluxname HiddenPhoton --N 1000000 -/// \endcode -/// -/// By default, it will load the flux definition found at `fluxes.rml` from the -/// `axionlib-data` repository, and generate a `png` image with the resuts from the -/// Monte Carlo execution. -/// -/// \htmlonly \endhtmlonly -/// -/// ![Solar flux distributions MC-generated with TRestAxionSolarQCDFlux.](ABC_flux_MC.png) -/// -/// ### Exporting the solar flux tables -/// -/// On top of that, we will be able to export those tables to the TRestAxionSolarHiddenPhotonFlux -/// standard format to be used in later occasions. -/// -/// \code -/// TRestAxionSolarHiddenPhotonFlux *sFlux = new TRestAxionSolarHiddenPhotonFlux("fluxes.rml", -/// "HiddenPhoton") sFlux->Initialize() sFlux->ExportTables() -/// \endcode -/// -/// which will produce a binary table `.N200f` with the continuum flux. The filename root will be -/// extracted from the original `.flux` file. Optionally we may export the continuum flux to an -/// ASCII file by indicating it at the TRestAxionSolarHiddenPhotonFlux::ExportTables method call. -/// The files will be placed at the REST user space, at `$HOME/.rest/export/` directory. -/// -/// TODO Implement the method TRestAxionSolarQCDFlux::InitializeSolarTable using -/// a solar model description by TRestAxionSolarModel. -/// -/// TODO Perhaps it would be interesting to replace fFluxTable for a TH2D -/// -///-------------------------------------------------------------------------- -/// -/// RESTsoft - Software for Rare Event Searches with TPCs -/// -/// History of developments: -/// -/// 2023-May: Specific methods extracted from TRestAxionSolarFlux -/// Javier Galan -/// 2023-June: TRestAxionSolarHiddenPhotonFlux created by editing TRestAxionSolarQCDFlux -/// Tomas O'Shea -/// -/// \class TRestAxionSolarHiddenPhotonFlux -/// \author Javier Galan -/// -///
-/// - -#include "TRestAxionSolarHiddenPhotonFlux.h" -using namespace std; - -ClassImp(TRestAxionSolarHiddenPhotonFlux); - -/////////////////////////////////////////////// -/// \brief Default constructor -/// -TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux() : TRestAxionSolarFlux() {} - -/////////////////////////////////////////////// -/// \brief Constructor loading data from a config file -/// -/// If no configuration path is defined using TRestMetadata::SetConfigFilePath -/// the path to the config file must be specified using full path, absolute or -/// relative. -/// -/// The default behaviour is that the config file must be specified with -/// full path, absolute or relative. -/// -/// \param cfgFileName A const char* giving the path to an RML file. -/// \param name The name of the specific metadata. It will be used to find the -/// corresponding TRestAxionMagneticField section inside the RML. -/// -TRestAxionSolarHiddenPhotonFlux::TRestAxionSolarHiddenPhotonFlux(const char* cfgFileName, string name) - : TRestAxionSolarFlux(cfgFileName) { - LoadConfigFromFile(fConfigFileName, name); - - if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Info) PrintMetadata(); -} - -/////////////////////////////////////////////// -/// \brief Default destructor -/// -TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} - -/////////////////////////////////////////////// -/// \brief It will load the tables in memory by using the filename information provided -/// inside the metadata members, and calculate the solar flux for a given m. -/// -Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - - if (GetMass() <= 0 ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; - return false; - } - if ( fFluxDataFile == "" ){ - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; - return false; - } - if ( fWidthDataFile == "") { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; - return false; - } - if ( fPlasmaFreqDataFile == "" ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; - return false; - } - - LoadContinuumFluxTable(); - LoadWidthTable(); - LoadPlasmaFreqTable(); - - CalculateSolarFlux(); - - IntegrateSolarFluxes(); - return true; -} - -/////////////////////////////////////////////// -/// \brief A helper method to load the data file containing continuum spectra as a -/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { - if (fFluxDataFile == "") { - RESTError - << "TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable. No solar flux table was defined" - << RESTendl; - return; - } - - string fullPathName = SearchFile((string)fFluxDataFile); - - RESTDebug << "Loading table from file : " << RESTendl; - RESTDebug << "File : " << fullPathName << RESTendl; - - std::vector> fluxTable; - - if (!TRestTools::IsBinaryFile(fFluxDataFile)) { - fluxTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; - } - - TRestTools::ReadBinaryTable(fullPathName, fluxTable); - - if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { - fluxTable.clear(); - RESTError << "LoadContinuumFluxTable. The table does not contain the right number of rows or columns" - << RESTendl; - RESTError << "Table will not be populated" << RESTendl; - } - - for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1D* h = new TH1D(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } - fContinuumTable.push_back(h); - } -} - -/////////////////////////////////////////////// -/// \brief A helper method to load the data file containing resonance width as a -/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { - if (fFluxDataFile == "") { - RESTError << "TRestAxionSolarHiddenPhotonFlux::LoadWidthTable. No width table was defined" - << RESTendl; - return; - } - - string fullPathName = SearchFile((string)fWidthDataFile); - - RESTDebug << "Loading table from file : " << RESTendl; - RESTDebug << "File : " << fullPathName << RESTendl; - - std::vector> fluxTable; - - if (!TRestTools::IsBinaryFile(fWidthDataFile)) { - fluxTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; - } - - TRestTools::ReadBinaryTable(fullPathName, fluxTable); - //RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << RESTendl; - - if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { - fluxTable.clear(); - RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" - << RESTendl; - RESTError << "Table will not be populated" << RESTendl; - } - - for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1D* h = new TH1D(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } - fWidthTable.push_back(h); - } -} - -/////////////////////////////////////////////// -/// \brief A helper method to load the data file containing resonance width as a -/// function of the solar radius. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { - if (fFluxDataFile == "") { - RESTError - << "TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable. No plasma frequency table was defined" - << RESTendl; - return; - } - - string fullPathName = SearchFile((string)fPlasmaFreqDataFile); - - RESTDebug << "Loading table from file : " << RESTendl; - RESTDebug << "File : " << fullPathName << RESTendl; - - std::vector> fluxTable; - - if (!TRestTools::IsBinaryFile(fWidthDataFile)) { - fluxTable.clear(); - RESTError << "File is not in binary format!" << RESTendl; - } - - TRestTools::ReadBinaryTable(fullPathName, fluxTable); - - if (fluxTable.size() != 1000 || fluxTable[0].size() != 1) { - fluxTable.clear(); - RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" - << RESTendl; - RESTError << "Table will not be populated" << RESTendl; - } - - for (unsigned int n = 0; n < fluxTable.size(); n++) { - TH1D* h = new TH1D(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } - fPlasmaFreqTable.push_back(h); - } -} - -/////////////////////////////////////////////// -/// \brief A helper method to calculate the real solar flux spectrum from the 3 tables, the -/// and the hidden photon mass for chi=1. -/// -void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { - if (GetMass() == 0) { - RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; - return; - } - if (fContinuumTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; - return; - } - if (fPlasmaFreqTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; - return; - } - if (fWidthTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; - return; - } - - Double_t mass = GetMass(); - cout << mass << endl; - for (unsigned int n = 0; n < fContinuumTable.size(); n++) { - // m4 * chi2 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - - Double_t wp = fPlasmaFreqTable[n]->GetBinContent(1); - TH1D* hMass = new TH1D(Form("%s_hMass%d", GetName(), n), "hMass", 200, 0, 20); - TH1D* hWg2 = (TH1D*)fWidthTable[n]->Clone(); - hWg2->Multiply(hWg2); // (w G)^2 - - for ( unsigned int c; c < 200; c++ ) { - Double_t wG = fWidthTable[n]->GetBinContent(c+1); - hMass->SetBinContent( c+1, pow(mass,-4) * ( pow( pow(mass,2) - pow(wp,2) , 2 )));// + pow(wG,2) ) ); // m2 - } - - hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 - - TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG - h->Multiply(fContinuumTable[n]); // wG * flux - h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - //h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - - fFluxTable.push_back(h); - } -} - -/////////////////////////////////////////////// -/// \brief It builds a histogram with the continuum spectrum. -/// The flux will be expressed in cm-2 s-1 keV-1. Binned in 100eV steps. -/// -TH1D* TRestAxionSolarHiddenPhotonFlux::GetContinuumSpectrum() { - if (fContinuumHist != nullptr) { - delete fContinuumHist; - fContinuumHist = nullptr; - } - - fContinuumHist = new TH1D("ContinuumHist", "", 200, 0, 20); - for (const auto& x : fFluxTable) { - fContinuumHist->Add(x); - } - - fContinuumHist->SetStats(0); - fContinuumHist->GetXaxis()->SetTitle("Energy [keV]"); - fContinuumHist->GetXaxis()->SetTitleSize(0.05); - fContinuumHist->GetXaxis()->SetLabelSize(0.05); - fContinuumHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); - fContinuumHist->GetYaxis()->SetTitleSize(0.05); - fContinuumHist->GetYaxis()->SetLabelSize(0.05); - - return fContinuumHist; -} - -/////////////////////////////////////////////// -/// \brief Same as GetContinuumSpectrum, the flux will be -/// expressed in cm-2 s-1 keV-1. Binned in 1eV steps. -/// -TH1D* TRestAxionSolarHiddenPhotonFlux::GetTotalSpectrum() { - TH1D* hc = GetContinuumSpectrum(); - - if (fTotalHist != nullptr) { - delete fTotalHist; - fTotalHist = nullptr; - } - - fTotalHist = new TH1D("fTotalHist", "", 20000, 0, 20); - for (int n = 0; n < hc->GetNbinsX(); n++) { - for (int m = 0; m < 100; m++) { - fTotalHist->SetBinContent(n * 100 + 1 + m, hc->GetBinContent(n + 1)); - } - } - - fTotalHist->SetStats(0); - fTotalHist->GetXaxis()->SetTitle("Energy [keV]"); - fTotalHist->GetXaxis()->SetTitleSize(0.05); - fTotalHist->GetXaxis()->SetLabelSize(0.05); - fTotalHist->GetYaxis()->SetTitle("Flux [cm-2 s-1 keV-1]"); - fTotalHist->GetYaxis()->SetTitleSize(0.05); - fTotalHist->GetYaxis()->SetLabelSize(0.05); - - return fTotalHist; -} - -/////////////////////////////////////////////// -/// \brief A helper method to initialize the internal class data members with the -/// integrated flux for each solar ring. It will be called by TRestAxionSolarHiddenPhotonFlux::Initialize. -/// -void TRestAxionSolarHiddenPhotonFlux::IntegrateSolarFluxes() { - fTotalContinuumFlux = 0.0; - for (unsigned int n = 0; n < fFluxTable.size(); n++) { - fTotalContinuumFlux += fFluxTable[n]->Integral() * 0.1; // We integrate in 100eV steps - fFluxTableIntegrals.push_back(fTotalContinuumFlux); - } - - for (unsigned int n = 0; n < fFluxTableIntegrals.size(); n++) - fFluxTableIntegrals[n] /= fTotalContinuumFlux; -} - -/////////////////////////////////////////////// -/// \brief It returns the integrated flux at earth in cm-2 s-1 for the given energy range -/// -Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) { - if (eRange.X() == -1 && eRange.Y() == -1) { - if (GetTotalFlux() == 0) IntegrateSolarFluxes(); - return GetTotalFlux(); - } - - Double_t flux = 0; - fTotalContinuumFlux = 0.0; - for (unsigned int n = 0; n < fFluxTable.size(); n++) { - flux += fFluxTable[n]->Integral(fFluxTable[n]->FindFixBin(eRange.X()), - fFluxTable[n]->FindFixBin(eRange.Y())) * - 0.1; // We integrate in 100eV steps - } - - return flux; -} - -/////////////////////////////////////////////// -/// \brief It returns a random solar radius position and energy according to the -/// flux distributions defined inside the solar tables loaded in the class -/// -std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { - - std::pair result = {0, 0}; - if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } - Double_t rnd = fRandom->Rndm(); - for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { - if (rnd < fFluxTableIntegrals[r]) { - Double_t energy = fFluxTable[r]->GetRandom(); - if (eRange.X() != -1 && eRange.Y() != -1) { - if (energy < eRange.X() || energy > eRange.Y()) return GetRandomEnergyAndRadius(eRange); - } - Double_t radius = ((Double_t)r + fRandom->Rndm()) * 0.001; - std::pair p = {energy, radius}; - return p; - } - } - return result; -} - -/////////////////////////////////////////////// -/// \brief It prints on screen the flux table that has been read from file -/// -void TRestAxionSolarHiddenPhotonFlux::PrintContinuumSolarTable() { - cout << "Continuum solar flux table: " << endl; - cout << "--------------------------- " << endl; - for (unsigned int n = 0; n < fFluxTable.size(); n++) { - for (int m = 0; m < fFluxTable[n]->GetNbinsX(); m++) - cout << fFluxTable[n]->GetBinContent(m + 1) << "\t"; - cout << endl; - cout << endl; - } - cout << endl; -} - -/////////////////////////////////////////////// -/// \brief It prints on screen the integrated solar flux per solar ring -/// -void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { - cout << "Integrated solar flux per solar ring: " << endl; - cout << "--------------------------- " << endl; - /* - for (int n = 0; n < fFluxPerRadius.size(); n++) - cout << "n : " << n << " flux : " << fFluxPerRadius[n] << endl; - cout << endl; - */ -} - -/////////////////////////////////////////////// -/// \brief Prints on screen the information about the metadata members of TRestAxionSolarHiddenPhotonFlux -/// -void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { - TRestAxionSolarFlux::PrintMetadata(); - - RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; - RESTMetadata << "-------" << RESTendl; - RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; - RESTMetadata << "++++++++++++++++++" << RESTendl; - - if (GetVerboseLevel() >= TRestStringOutput::REST_Verbose_Level::REST_Debug) { - PrintContinuumSolarTable(); - PrintIntegratedRingFlux(); - } -} - -/////////////////////////////////////////////// -/// \brief It will create files with spectra to be used -/// in a later ocasion. -/// -void TRestAxionSolarHiddenPhotonFlux::ExportTables(Bool_t ascii) { - string rootFilename = TRestTools::GetFileNameRoot(fFluxDataFile); - - string path = REST_USER_PATH + "/export/"; - - if (!TRestTools::fileExists(path)) { - std::cout << "Creating path: " << path << std::endl; - int z = system(("mkdir -p " + path).c_str()); - if (z != 0) RESTError << "Could not create directory " << path << RESTendl; - } - - if (fFluxTable.size() > 0) { - std::vector> table; - for (const auto& x : fFluxTable) { - std::vector row; - for (int n = 0; n < x->GetNbinsX(); n++) row.push_back(x->GetBinContent(n + 1)); - - table.push_back(row); - } - - if (!ascii) - TRestTools::ExportBinaryTable(path + "/" + rootFilename + ".N200f", table); - else - TRestTools::ExportASCIITable(path + "/" + rootFilename + ".dat", table); - } -} - -/////////////////////////////////////////////// -/// \brief It draws the contents of a .flux file. This method just receives the -/// -TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { - if (fCanvas != nullptr) { - delete fCanvas; - fCanvas = nullptr; - } - fCanvas = new TCanvas("canv", "This is the canvas title", 1200, 500); - fCanvas->Draw(); - - TPad* pad1 = new TPad("pad1", "This is pad1", 0.01, 0.02, 0.99, 0.97); - pad1->Divide(2, 1); - pad1->Draw(); - - pad1->cd(1); - pad1->cd(1)->SetLogy(); - pad1->cd(1)->SetRightMargin(0.09); - pad1->cd(1)->SetLeftMargin(0.15); - pad1->cd(1)->SetBottomMargin(0.15); - - TH1D* ht = GetTotalSpectrum(); - ht->SetLineColor(kBlack); - ht->SetFillStyle(4050); - ht->SetFillColor(kBlue - 10); - - ht->Draw("hist"); - - pad1->cd(2); - pad1->cd(2)->SetRightMargin(0.09); - pad1->cd(2)->SetLeftMargin(0.15); - pad1->cd(2)->SetBottomMargin(0.15); - - ht->Draw("hist"); - - return fCanvas; -} - From 5f91092171b0a7810cbde0cd04a3fd3e75ff6f98 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Fri, 15 Sep 2023 11:02:57 +0000 Subject: [PATCH 33/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionSolarFlux.h | 9 +- inc/TRestAxionSolarHiddenPhotonFlux.h | 2 +- inc/TRestAxionSolarQCDFlux.h | 4 +- .../solarFlux/solarPlotHiddenPhoton.py | 10 +- src/TRestAxionSolarFlux.cxx | 5 +- src/TRestAxionSolarHiddenPhotonFlux.cxx | 114 ++++++++++-------- 6 files changed, 79 insertions(+), 65 deletions(-) diff --git a/inc/TRestAxionSolarFlux.h b/inc/TRestAxionSolarFlux.h index 9a917211..6c740852 100644 --- a/inc/TRestAxionSolarFlux.h +++ b/inc/TRestAxionSolarFlux.h @@ -65,10 +65,13 @@ class TRestAxionSolarFlux : public TRestMetadata { void Initialize(); /// It is required in order to load solar flux tables into memory for specific mass - void InitializeMass( Double_t mass ) { SetMass(mass); Initialize(); } - + void InitializeMass(Double_t mass) { + SetMass(mass); + Initialize(); + } + /// Set mass and reinitialise - void SetMass( Double_t m ) { fMass = m; } //Initialize(); } + void SetMass(Double_t m) { fMass = m; } // Initialize(); } /// It returns the integrated flux at earth in cm-2 s-1 for the given energy range virtual Double_t IntegrateFluxInRange(TVector2 eRange = TVector2(-1, -1)) = 0; diff --git a/inc/TRestAxionSolarHiddenPhotonFlux.h b/inc/TRestAxionSolarHiddenPhotonFlux.h index bdc44040..5a6b0398 100644 --- a/inc/TRestAxionSolarHiddenPhotonFlux.h +++ b/inc/TRestAxionSolarHiddenPhotonFlux.h @@ -73,7 +73,7 @@ class TRestAxionSolarHiddenPhotonFlux : public TRestAxionSolarFlux { void LoadMonoChromaticFluxTable(); void IntegrateSolarFluxes(); - public: + public: /// It returns true if continuum flux spectra was loaded Bool_t isSolarTableLoaded() { return fFluxTable.size() > 0; } diff --git a/inc/TRestAxionSolarQCDFlux.h b/inc/TRestAxionSolarQCDFlux.h index 10db402e..fb99ebb0 100644 --- a/inc/TRestAxionSolarQCDFlux.h +++ b/inc/TRestAxionSolarQCDFlux.h @@ -93,9 +93,7 @@ class TRestAxionSolarQCDFlux : public TRestAxionSolarFlux { Bool_t LoadTables() override; /// It returns the total integrated flux at earth in cm-2 s-1 - Double_t GetTotalFlux() override { - return fTotalContinuumFlux + fTotalMonochromaticFlux; - } + Double_t GetTotalFlux() override { return fTotalContinuumFlux + fTotalMonochromaticFlux; } /// It returns an energy integrated spectrum in cm-2 s-1 keV-1 TH1D* GetEnergySpectrum() override { return GetTotalSpectrum(); } diff --git a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py index c07ac580..5b83b758 100755 --- a/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py +++ b/pipeline/metadata/solarFlux/solarPlotHiddenPhoton.py @@ -44,12 +44,10 @@ parser.add_argument( "--N", dest="samples", type=int, help="The number of generated particles" ) -parser.add_argument( - "--m", dest="mass", type=float, help="Hidden photon mass [eV]" -) +parser.add_argument("--m", dest="mass", type=float, help="Hidden photon mass [eV]") args = parser.parse_args() -mass = 10. # eV +mass = 10.0 # eV if args.mass != None: mass = args.mass @@ -96,7 +94,7 @@ comb_spt = TH2D("comb_spt", "Energy versus solar radius", 20000, 0, 20, 100, 0, 1) for i in range(samples): x = combinedFlux.GetRandomEnergyAndRadius((-1, -1)) - #print(x) + # print(x) comb_spt.Fill(x[0], x[1]) rnd = TRandom3(0) @@ -164,4 +162,4 @@ c1.Print(outfname) print("Generated file : " + outfname) -#exit(0) +# exit(0) diff --git a/src/TRestAxionSolarFlux.cxx b/src/TRestAxionSolarFlux.cxx index f82d9e34..62549922 100644 --- a/src/TRestAxionSolarFlux.cxx +++ b/src/TRestAxionSolarFlux.cxx @@ -134,12 +134,11 @@ void TRestAxionSolarFlux::Initialize() { fSeed = fRandom->TRandom::GetSeed(); } - /////////////////////////////////////////////// /// \brief Initialization of TRestAxionSolarFlux members with specific mass /// -//void TRestAxionSolarFlux::InitializeMass( Double_t mass ) { SetMass(mass); RESTMetadata << GetMass() << RESTendl; } // SetMass calls Initialize - +// void TRestAxionSolarFlux::InitializeMass( Double_t mass ) { SetMass(mass); RESTMetadata << GetMass() << +// RESTendl; } // SetMass calls Initialize /////////////////////////////////////////////// /// \brief It builds a histogram using the contents of the .flux file given diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 0c213f20..f824fd5c 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -184,23 +184,28 @@ TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} /// inside the metadata members, and calculate the solar flux for a given m. /// Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - - if (GetMass() <= 0 ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; - return false; + if (GetMass() <= 0) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" + << RESTendl; + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" + << RESTendl; + return false; + } + if (fFluxDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " + << fFluxDataFile << RESTendl; + return false; } - if ( fFluxDataFile == "" ){ - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; - return false; + if (fWidthDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " + << fWidthDataFile << RESTendl; + return false; } - if ( fWidthDataFile == "") { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; - return false; - } - if ( fPlasmaFreqDataFile == "" ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; - return false; + if (fPlasmaFreqDataFile == "") { + RESTWarning + << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " + << fPlasmaFreqDataFile << RESTendl; + return false; } LoadContinuumFluxTable(); @@ -248,7 +253,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { + h->SetBinContent(m + 1, fluxTable[n][m]); + } fContinuumTable.push_back(h); } } @@ -277,8 +284,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { } TRestTools::ReadBinaryTable(fullPathName, fluxTable); - //RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << RESTendl; - + // RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << + // RESTendl; + if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { fluxTable.clear(); RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" @@ -288,7 +296,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { + h->SetBinContent(m + 1, fluxTable[n][m]); + } fWidthTable.push_back(h); } } @@ -318,7 +328,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { } TRestTools::ReadBinaryTable(fullPathName, fluxTable); - + if (fluxTable.size() != 1000 || fluxTable[0].size() != 1) { fluxTable.clear(); RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" @@ -328,7 +338,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { + h->SetBinContent(m + 1, fluxTable[n][m]); + } fPlasmaFreqTable.push_back(h); } } @@ -341,20 +353,21 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { if (GetMass() == 0) { RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; - } - if (fContinuumTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; - return; } - if (fPlasmaFreqTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; - return; + if (fContinuumTable.size() == 0) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; + return; } - if (fWidthTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; - return; + if (fPlasmaFreqTable.size() == 0) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" + << RESTendl; + return; + } + if (fWidthTable.size() == 0) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; + return; } - + Double_t mass = GetMass(); cout << mass << endl; for (unsigned int n = 0; n < fContinuumTable.size(); n++) { @@ -363,19 +376,21 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { Double_t wp = fPlasmaFreqTable[n]->GetBinContent(1); TH1D* hMass = new TH1D(Form("%s_hMass%d", GetName(), n), "hMass", 200, 0, 20); TH1D* hWg2 = (TH1D*)fWidthTable[n]->Clone(); - hWg2->Multiply(hWg2); // (w G)^2 + hWg2->Multiply(hWg2); // (w G)^2 - for ( unsigned int c = 0; c < 200; c++ ) { - Double_t wG = fWidthTable[n]->GetBinContent(c+1); - hMass->SetBinContent( c+1, pow(mass,-4) * ( pow( pow(mass,2) - pow(wp,2) , 2 )));// + pow(wG,2) ) ); // m2 - } - - hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 + for (unsigned int c = 0; c < 200; c++) { + Double_t wG = fWidthTable[n]->GetBinContent(c + 1); + hMass->SetBinContent( + c + 1, pow(mass, -4) * (pow(pow(mass, 2) - pow(wp, 2), 2))); // + pow(wG,2) ) ); // m2 + } - TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG - h->Multiply(fContinuumTable[n]); // wG * flux - h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - //h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 + + TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG + h->Multiply(fContinuumTable[n]); // wG * flux + h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 + // ) fFluxTable.push_back(h); } @@ -477,9 +492,11 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) /// flux distributions defined inside the solar tables loaded in the class /// std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { - std::pair result = {0, 0}; - if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } + if (!AreTablesLoaded()) { + RESTWarning << "Tables not loaded!!" << RESTendl; + return result; + } Double_t rnd = fRandom->Rndm(); for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { if (rnd < fFluxTableIntegrals[r]) { @@ -529,9 +546,9 @@ void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { TRestAxionSolarFlux::PrintMetadata(); - RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; RESTMetadata << "-------" << RESTendl; RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; RESTMetadata << "++++++++++++++++++" << RESTendl; @@ -610,4 +627,3 @@ TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { return fCanvas; } - From f2ea3420d0d8831de1622ce7fc384c5e879a59f6 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Fri, 15 Sep 2023 15:18:08 +0200 Subject: [PATCH 34/48] commented out redundant 'wG' in calculation --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 114 ++++++++++-------------- 1 file changed, 49 insertions(+), 65 deletions(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index f824fd5c..a59cbc95 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -184,28 +184,23 @@ TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} /// inside the metadata members, and calculate the solar flux for a given m. /// Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - if (GetMass() <= 0) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" - << RESTendl; - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" - << RESTendl; - return false; - } - if (fFluxDataFile == "") { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " - << fFluxDataFile << RESTendl; - return false; + + if (GetMass() <= 0 ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; + return false; } - if (fWidthDataFile == "") { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " - << fWidthDataFile << RESTendl; - return false; + if ( fFluxDataFile == "" ){ + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; + return false; } - if (fPlasmaFreqDataFile == "") { - RESTWarning - << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " - << fPlasmaFreqDataFile << RESTendl; - return false; + if ( fWidthDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; + return false; + } + if ( fPlasmaFreqDataFile == "" ) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; + return false; } LoadContinuumFluxTable(); @@ -253,9 +248,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { - h->SetBinContent(m + 1, fluxTable[n][m]); - } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } fContinuumTable.push_back(h); } } @@ -284,9 +277,8 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { } TRestTools::ReadBinaryTable(fullPathName, fluxTable); - // RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << - // RESTendl; - + //RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << RESTendl; + if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { fluxTable.clear(); RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" @@ -296,9 +288,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { - h->SetBinContent(m + 1, fluxTable[n][m]); - } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } fWidthTable.push_back(h); } } @@ -328,7 +318,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { } TRestTools::ReadBinaryTable(fullPathName, fluxTable); - + if (fluxTable.size() != 1000 || fluxTable[0].size() != 1) { fluxTable.clear(); RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" @@ -338,9 +328,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { - h->SetBinContent(m + 1, fluxTable[n][m]); - } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } fPlasmaFreqTable.push_back(h); } } @@ -353,21 +341,20 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { if (GetMass() == 0) { RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; + } + if (fContinuumTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; + return; } - if (fContinuumTable.size() == 0) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; - return; + if (fPlasmaFreqTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; + return; } - if (fPlasmaFreqTable.size() == 0) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" - << RESTendl; - return; - } - if (fWidthTable.size() == 0) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; - return; + if (fWidthTable.size() == 0 ) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; + return; } - + Double_t mass = GetMass(); cout << mass << endl; for (unsigned int n = 0; n < fContinuumTable.size(); n++) { @@ -376,21 +363,19 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { Double_t wp = fPlasmaFreqTable[n]->GetBinContent(1); TH1D* hMass = new TH1D(Form("%s_hMass%d", GetName(), n), "hMass", 200, 0, 20); TH1D* hWg2 = (TH1D*)fWidthTable[n]->Clone(); - hWg2->Multiply(hWg2); // (w G)^2 + hWg2->Multiply(hWg2); // (w G)^2 - for (unsigned int c = 0; c < 200; c++) { - Double_t wG = fWidthTable[n]->GetBinContent(c + 1); - hMass->SetBinContent( - c + 1, pow(mass, -4) * (pow(pow(mass, 2) - pow(wp, 2), 2))); // + pow(wG,2) ) ); // m2 - } + for ( unsigned int c = 0; c < 200; c++ ) { + //Double_t wG = fWidthTable[n]->GetBinContent(c+1); + hMass->SetBinContent( c+1, pow(mass,-4) * ( pow( pow(mass,2) - pow(wp,2) , 2 )));// + pow(wG,2) ) ); // m2 + } + + hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 - hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 - - TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG - h->Multiply(fContinuumTable[n]); // wG * flux - h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 - // ) + TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG + h->Multiply(fContinuumTable[n]); // wG * flux + h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + //h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) fFluxTable.push_back(h); } @@ -492,11 +477,9 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) /// flux distributions defined inside the solar tables loaded in the class /// std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { + std::pair result = {0, 0}; - if (!AreTablesLoaded()) { - RESTWarning << "Tables not loaded!!" << RESTendl; - return result; - } + if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } Double_t rnd = fRandom->Rndm(); for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { if (rnd < fFluxTableIntegrals[r]) { @@ -546,9 +529,9 @@ void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { TRestAxionSolarFlux::PrintMetadata(); - RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; RESTMetadata << "-------" << RESTendl; RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; RESTMetadata << "++++++++++++++++++" << RESTendl; @@ -627,3 +610,4 @@ TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { return fCanvas; } + From fae682bc6680c4fc0b01282e61c123c9fe03c7ae Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Fri, 15 Sep 2023 13:18:37 +0000 Subject: [PATCH 35/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 114 ++++++++++++++---------- 1 file changed, 65 insertions(+), 49 deletions(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index a59cbc95..64deb8f3 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -184,23 +184,28 @@ TRestAxionSolarHiddenPhotonFlux::~TRestAxionSolarHiddenPhotonFlux() {} /// inside the metadata members, and calculate the solar flux for a given m. /// Bool_t TRestAxionSolarHiddenPhotonFlux::LoadTables() { - - if (GetMass() <= 0 ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" << RESTendl; - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" << RESTendl; - return false; + if (GetMass() <= 0) { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - hidden photon mass not yet defined" + << RESTendl; + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - mass given as " << GetMass() << " eV" + << RESTendl; + return false; + } + if (fFluxDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " + << fFluxDataFile << RESTendl; + return false; } - if ( fFluxDataFile == "" ){ - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - flux table not found!!\n " << fFluxDataFile << RESTendl; - return false; + if (fWidthDataFile == "") { + RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " + << fWidthDataFile << RESTendl; + return false; } - if ( fWidthDataFile == "") { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - width table not found!!\n " << fWidthDataFile << RESTendl; - return false; - } - if ( fPlasmaFreqDataFile == "" ) { - RESTWarning << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " << fPlasmaFreqDataFile << RESTendl; - return false; + if (fPlasmaFreqDataFile == "") { + RESTWarning + << "TRestAxionSolarHiddenPhotonFlux::LoadTables - plasma frequency table not found!!\n " + << fPlasmaFreqDataFile << RESTendl; + return false; } LoadContinuumFluxTable(); @@ -248,7 +253,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadContinuumFluxTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_ContinuumFluxAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { + h->SetBinContent(m + 1, fluxTable[n][m]); + } fContinuumTable.push_back(h); } } @@ -277,8 +284,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { } TRestTools::ReadBinaryTable(fullPathName, fluxTable); - //RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << RESTendl; - + // RESTMetadata << "Width table rows / columns: " << fluxTable.size() << " " << fluxTable[0].size() << + // RESTendl; + if (fluxTable.size() != 1000 || fluxTable[0].size() != 200) { fluxTable.clear(); RESTError << "LoadWidthTable. The table does not contain the right number of rows or columns" @@ -288,7 +296,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadWidthTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_ResonanceWidthAtRadius%d", GetName(), n), "", 200, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { + h->SetBinContent(m + 1, fluxTable[n][m]); + } fWidthTable.push_back(h); } } @@ -318,7 +328,7 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { } TRestTools::ReadBinaryTable(fullPathName, fluxTable); - + if (fluxTable.size() != 1000 || fluxTable[0].size() != 1) { fluxTable.clear(); RESTError << "LoadPlasmaFreqTable. The table does not contain the right number of rows or columns" @@ -328,7 +338,9 @@ void TRestAxionSolarHiddenPhotonFlux::LoadPlasmaFreqTable() { for (unsigned int n = 0; n < fluxTable.size(); n++) { TH1D* h = new TH1D(Form("%s_PlasmaFreqAtRadius%d", GetName(), n), "", 1, 0, 20); - for (unsigned int m = 0; m < fluxTable[n].size(); m++) { h->SetBinContent(m + 1, fluxTable[n][m]); } + for (unsigned int m = 0; m < fluxTable[n].size(); m++) { + h->SetBinContent(m + 1, fluxTable[n][m]); + } fPlasmaFreqTable.push_back(h); } } @@ -341,20 +353,21 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { if (GetMass() == 0) { RESTError << "CalculateSolarFlux. The hidden photon mass is set to zero!" << RESTendl; return; - } - if (fContinuumTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; - return; } - if (fPlasmaFreqTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" << RESTendl; - return; + if (fContinuumTable.size() == 0) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty flux table!" << RESTendl; + return; } - if (fWidthTable.size() == 0 ) { - RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; - return; + if (fPlasmaFreqTable.size() == 0) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty plasma freq table!" + << RESTendl; + return; + } + if (fWidthTable.size() == 0) { + RESTError << "TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux - empty width table!" << RESTendl; + return; } - + Double_t mass = GetMass(); cout << mass << endl; for (unsigned int n = 0; n < fContinuumTable.size(); n++) { @@ -363,19 +376,21 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { Double_t wp = fPlasmaFreqTable[n]->GetBinContent(1); TH1D* hMass = new TH1D(Form("%s_hMass%d", GetName(), n), "hMass", 200, 0, 20); TH1D* hWg2 = (TH1D*)fWidthTable[n]->Clone(); - hWg2->Multiply(hWg2); // (w G)^2 + hWg2->Multiply(hWg2); // (w G)^2 - for ( unsigned int c = 0; c < 200; c++ ) { - //Double_t wG = fWidthTable[n]->GetBinContent(c+1); - hMass->SetBinContent( c+1, pow(mass,-4) * ( pow( pow(mass,2) - pow(wp,2) , 2 )));// + pow(wG,2) ) ); // m2 - } - - hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 + for (unsigned int c = 0; c < 200; c++) { + // Double_t wG = fWidthTable[n]->GetBinContent(c+1); + hMass->SetBinContent( + c + 1, pow(mass, -4) * (pow(pow(mass, 2) - pow(wp, 2), 2))); // + pow(wG,2) ) ); // m2 + } - TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG - h->Multiply(fContinuumTable[n]); // wG * flux - h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - //h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + hMass->Add(hWg2); // (m2 - wp2)^2 + (w G)^2 + + TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG + h->Multiply(fContinuumTable[n]); // wG * flux + h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) + // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 + // ) fFluxTable.push_back(h); } @@ -477,9 +492,11 @@ Double_t TRestAxionSolarHiddenPhotonFlux::IntegrateFluxInRange(TVector2 eRange) /// flux distributions defined inside the solar tables loaded in the class /// std::pair TRestAxionSolarHiddenPhotonFlux::GetRandomEnergyAndRadius(TVector2 eRange) { - std::pair result = {0, 0}; - if (!AreTablesLoaded()) { RESTWarning << "Tables not loaded!!" << RESTendl; return result; } + if (!AreTablesLoaded()) { + RESTWarning << "Tables not loaded!!" << RESTendl; + return result; + } Double_t rnd = fRandom->Rndm(); for (unsigned int r = 0; r < fFluxTableIntegrals.size(); r++) { if (rnd < fFluxTableIntegrals[r]) { @@ -529,9 +546,9 @@ void TRestAxionSolarHiddenPhotonFlux::PrintIntegratedRingFlux() { void TRestAxionSolarHiddenPhotonFlux::PrintMetadata() { TRestAxionSolarFlux::PrintMetadata(); - RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; - RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (flux) : " << fFluxDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (width) : " << fWidthDataFile << RESTendl; + RESTMetadata << " - Solar hidden photon datafile (plasma freq) : " << fPlasmaFreqDataFile << RESTendl; RESTMetadata << "-------" << RESTendl; RESTMetadata << " - Total continuum flux : " << fTotalContinuumFlux << " cm-2 s-1" << RESTendl; RESTMetadata << "++++++++++++++++++" << RESTendl; @@ -610,4 +627,3 @@ TCanvas* TRestAxionSolarHiddenPhotonFlux::DrawSolarFlux() { return fCanvas; } - From 5cab20e09a1c890fe2443a2d2f5972d8080a31ed Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Tue, 26 Sep 2023 09:29:40 +0200 Subject: [PATCH 36/48] created some plots --- flux.png | Bin 19725 -> 32743 bytes flux0.001.png | Bin 0 -> 36954 bytes flux0.01.png | Bin 0 -> 37352 bytes flux0.1.png | Bin 0 -> 37172 bytes flux1.png | Bin 0 -> 30693 bytes flux10.png | Bin 0 -> 32331 bytes flux100.png | Bin 0 -> 36014 bytes flux1000.png | Bin 0 -> 36178 bytes flux20.png | Bin 0 -> 35192 bytes flux30.png | Bin 0 -> 35393 bytes flux50.png | Bin 0 -> 35928 bytes 11 files changed, 0 insertions(+), 0 deletions(-) create mode 100644 flux0.001.png create mode 100644 flux0.01.png create mode 100644 flux0.1.png create mode 100644 flux1.png create mode 100644 flux10.png create mode 100644 flux100.png create mode 100644 flux1000.png create mode 100644 flux20.png create mode 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for more information, see https://pre-commit.ci --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 3 ++- 1 file changed, 2 insertions(+), 1 deletion(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 64deb8f3..87b3360b 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -389,7 +389,8 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG h->Multiply(fContinuumTable[n]); // wG * flux h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2 + // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w + // G)^2 // ) fFluxTable.push_back(h); From 914fa2090024cab4dfbc91a338320325daa02b2b Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Tue, 26 Sep 2023 13:37:33 +0200 Subject: [PATCH 38/48] created HP field code --- inc/TRestAxionHiddenPhotonField.h | 64 ++++ ...TRestAxionField.h => TRestAxionQCDField.h} | 12 +- src/TRestAxionHiddenPhotonField.cxx | 323 ++++++++++++++++++ ...tAxionField.cxx => TRestAxionQCDField.cxx} | 55 +-- 4 files changed, 423 insertions(+), 31 deletions(-) create mode 100644 inc/TRestAxionHiddenPhotonField.h rename inc/{TRestAxionField.h => TRestAxionQCDField.h} (93%) create mode 100644 src/TRestAxionHiddenPhotonField.cxx rename src/{TRestAxionField.cxx => TRestAxionQCDField.cxx} (90%) diff --git a/inc/TRestAxionHiddenPhotonField.h b/inc/TRestAxionHiddenPhotonField.h new file mode 100644 index 00000000..9ea444ed --- /dev/null +++ b/inc/TRestAxionHiddenPhotonField.h @@ -0,0 +1,64 @@ +/************************************************************************* + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +#ifndef _TRestAxionHiddenPhotonField +#define _TRestAxionHiddenPhotonField + +#include "TRestAxionBufferGas.h" + +//! A basic class to define analytical axion-photon conversion calculations for axion helioscopes +class TRestAxionHiddenPhotonField : public TObject { + private: + Bool_t fDebug = false; //! + + void Initialize(); + + /// A pointer to the buffer gas definition + TRestAxionBufferGas* fBufferGas = NULL; //! + + public: + /// momentum difference q, useful in all calculations + Double_t TRestAxionHiddenPhotonField::momentumTransfer( Double_t Ea, Double_t ma, Double_t mg ) { + return sqrt(Ea*Ea - mg*mg) - sqrt(Ea*Ea - ma*ma); + } + + /// It enables/disables debug mode + void SetDebug(Bool_t v) { fDebug = v; } + + /// It assigns a gas buffer medium to the calculation + void AssignBufferGas(TRestAxionBufferGas* buffGas) { fBufferGas = buffGas; } + + /// It assigns a gas buffer medium to the calculation + void SetBufferGas(TRestAxionBufferGas* buffGas) { fBufferGas = buffGas; } + + Double_t GammaTransmissionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, + Double_t mg = 0, Double_t absLength = 0); + + //Double_t PhotonAbsorptionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, + // Double_t mg = 0, Double_t absLength = 0); + + TRestAxionHiddenPhotonField(); + ~TRestAxionHiddenPhotonField(); + + ClassDef(TRestAxionHiddenPhotonField, 2); +}; +#endif diff --git a/inc/TRestAxionField.h b/inc/TRestAxionQCDField.h similarity index 93% rename from inc/TRestAxionField.h rename to inc/TRestAxionQCDField.h index 22662d63..ecfb183d 100644 --- a/inc/TRestAxionField.h +++ b/inc/TRestAxionQCDField.h @@ -20,13 +20,13 @@ * For the list of contributors see $REST_PATH/CREDITS. * *************************************************************************/ -#ifndef _TRestAxionField -#define _TRestAxionField +#ifndef _TRestAxionQCDField +#define _TRestAxionQCDField #include "TRestAxionBufferGas.h" //! A basic class to define analytical axion-photon conversion calculations for axion helioscopes -class TRestAxionField : public TObject { +class TRestAxionQCDField : public TObject { private: Bool_t fDebug = false; //! @@ -57,9 +57,9 @@ class TRestAxionField : public TObject { Double_t AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg = 0, Double_t absLength = 0); - TRestAxionField(); - ~TRestAxionField(); + TRestAxionQCDField(); + ~TRestAxionQCDField(); - ClassDef(TRestAxionField, 2); + ClassDef(TRestAxionQCDField, 2); }; #endif diff --git a/src/TRestAxionHiddenPhotonField.cxx b/src/TRestAxionHiddenPhotonField.cxx new file mode 100644 index 00000000..8236136b --- /dev/null +++ b/src/TRestAxionHiddenPhotonField.cxx @@ -0,0 +1,323 @@ +/************************************************************************* + * This file is part of the REST software framework. * + * * + * Copyright (C) 2016 GIFNA/TREX (University of Zaragoza) * + * For more information see http://gifna.unizar.es/trex * + * * + * REST is free software: you can redistribute it and/or modify * + * it under the terms of the GNU General Public License as published by * + * the Free Software Foundation, either version 3 of the License, or * + * (at your option) any later version. * + * * + * REST is distributed in the hope that it will be useful, * + * but WITHOUT ANY WARRANTY; without even the implied warranty of * + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * + * GNU General Public License for more details. * + * * + * You should have a copy of the GNU General Public License along with * + * REST in $REST_PATH/LICENSE. * + * If not, see http://www.gnu.org/licenses/. * + * For the list of contributors see $REST_PATH/CREDITS. * + *************************************************************************/ + +////////////////////////////////////////////////////////////////////////// +/// TRestAxionHiddenPhotonField is a class used to calculate the axion-photon mixing +/// and determine the probability of the particle being in an axion or photon +/// state. +/// +/// A peculiarity from this class is that it encapsulates internally the high +/// precision calculations using the real precisions types using TRestComplex. +/// It is known that double precision is not good enough in some scenarios. +/// +///-------------------------------------------------------------------------- +/// +/// RESTsoft - Software for Rare Event Searches with TPCs +/// +/// History of developments: +/// +/// 2019-March: First concept and implementation of TRestAxionHiddenPhotonField class. +/// Javier Galan +/// 2023-September: Separation of QCD and HiddenPhoton classes. +/// Tom O'Shea +/// +/// \class TRestAxionHiddenPhotonField +/// \author Javier Galan +/// +///

+/// +#include "TRestAxionHiddenPhotonField.h" + +#include + +#include "TH1F.h" + +#ifdef USE_MPFR +#include "TRestComplex.h" +#endif + +#include + +using namespace std; + +ClassImp(TRestAxionHiddenPhotonField); + +/////////////////////////////////////////////// +/// \brief Default constructor +/// +TRestAxionHiddenPhotonField::TRestAxionHiddenPhotonField() { Initialize(); } + +/////////////////////////////////////////////// +/// \brief Default destructor +/// +TRestAxionHiddenPhotonField::~TRestAxionHiddenPhotonField() {} + +/////////////////////////////////////////////// +/// \brief Initialization of TRestAxionHiddenPhotonField class +/// +/// It sets the default real precision to be used with mpfr types. Now it is 30 digits. +/// So that we can still calculate numbers such as : 1.0 - 1.e-30 +/// +void TRestAxionHiddenPhotonField::Initialize() { +#ifdef USE_MPFR + TRestComplex::SetPrecision(30); +#endif + + fBufferGas = NULL; + + /// MOVED TO TRestAxionHiddenPhotonFieldPropagationProcess class + /// faxion = SetComplexReal(1, 0); + /// fAem = SetComplexReal(0, 0); +} + + +/////////////////////////////////////////////// +/// vacuum conversion probability +/// ie. when photonMass = 0 +Double_t TRestAxionHiddenPhotonField::VacuumConversion(Double_t Lcoh, Double_t Ea, Double_t ma) { + Double_t q = momentumTransfer(Ea, ma, 0.); + return pow(2*sin(q*Lcoh/2), 2); +} + + + +/////////////////////////////////////////////// +/// \brief Performs the calculation of hidden photon - photon conversion probability. +/// +/// If m_gamma (mg) is not given as an argument, i.e. it is equal to zero, then m_gamma +/// will be obtainned from the buffer gas definition. If no buffer gas has been assigned +/// then the medium will be assumed to be vacuum. +/// +/// Ea in keV, ma in eV, Lcoh in mm, mg in eV, absLength in cm-1 +/// +/// The returned value is given for chi = 1 +/// +Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, + Double_t mg, Double_t absLength) { +#ifndef USE_MPFR + RESTWarning + << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" + << RESTendl; + RESTWarning << "TRestAxionHiddenPhotonField::GammaTransmissionProbability will return 0" << RESTendl; + return 0; +#else + mpfr::mpreal hiddenPhotonMass = ma; + mpfr::mpreal cohLength = Lcoh / 1000.; // Default REST units are mm; + + mpfr::mpreal photonMass = mg; + + if (mg == 0 && fBufferGas) photonMass = fBufferGas->GetPhotonMass(Ea); + + RESTDebug << "+--------------------------------------------------------------------------+" << RESTendl; + RESTDebug << " TRestAxionHiddenPhotonField::GammaTransmissionProbability. Parameter summary" << RESTendl; + RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; + RESTDebug << " Hidden photon mass : " << ma << " eV" << RESTendl; + RESTDebug << " Hidden photon energy : " << Ea << " keV" << RESTendl; + RESTDebug << " Lcoh : " << Lcoh << " mm" << RESTendl; + RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; + RESTDebug << "+--------------------------------------------------------------------------+" << RESTendl; + + if (photonMass == 0.0) return VacuumConversion(Lcoh, Ea, ma); + + mpfr::mpreal q = momentumTransfer(Ea, ma, mg) // eV + mpfr::mpreal l = cohLength * REST_Physics::PhMeterIneV; // eV-1 + + mpfr::mpreal Gamma = absLength; // cm-1 + if (absLength == 0 && fBufferGas) Gamma = fBufferGas->GetPhotonAbsorptionLength(Ea); // cm-1 + mpfr::mpreal GammaL = Gamma * cohLength * 100; + Gamma *= 100 / REST_Physics::PhMeterIneV; // eV + + if (fDebug) { + RESTDebug << "+------------------------+" << RESTendl; + RESTDebug << " Intermediate calculations" << RESTendl; + RESTDebug << " q : " << q << " eV" << RESTendl; + RESTDebug << " l : " << l << " eV-1" << RESTendl; + RESTDebug << " ql : " << q*l << RESTendl; + RESTDebug << "Gamma : " << Gamma << RESTendl; + RESTDebug << "GammaL : " << GammaL << RESTendl; + RESTDebug << "+------------------------+" << RESTendl; + } + + mpfr::mpreal MFactor = pow(ma,4)/(pow(ma*ma - mg*mg, 2) + pow(Ea*Gamma, 2)); // all should be in eV + + + if (fDebug) { + RESTDebug << "Mfactor : " << MFactor << RESTendl; + RESTDebug << "cos(ql) : " << cos(q*l) << RESTendl; + RESTDebug << "Exp(-GammaL) : " << exp(-GammaL) << RESTendl; + } + + double sol = + (double)(MFactor * (1 + exp(-GammaL) - 2 * exp(-GammaL / 2) * cos(q*l))); + + RESTDebug << "Axion-photon transmission probability : " << sol << RESTendl; + + return sol; +#endif +} + + + +/////////////////////////////////////////////// +/// \brief Performs the calculation of the photon absorbtion probability in the buffer gas. +/// +/// If not provided as argument, m_g it will be attempted to obtain the value from the buffer gas +/// definition. If no buffer gas has been assigned the medium will be assumed to be vacuum. +/// +/// Ea in keV, ma in eV, Lcoh in mm, mg in eV, absLength in cm-1 +/// +/// The returned value is given for chi = 1 +/// +Double_t TRestAxionHiddenPhotonField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, + Double_t mg, Double_t absLength) { +#ifndef USE_MPFR + RESTWarning + << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFr=ON to your REST compilation" + << RESTendl; + RESTWarning << "TRestAxionHiddenPhotonField::GammaTransmissionProbability will return 0" << RESTendl; + return 0; +#else + mpfr::mpreal axionMass = ma; + mpfr::mpreal cohLength = Lcoh / 1000.; // Default REST units are mm; + + mpfr::mpreal photonMass = mg; + if (mg == 0 && fBufferGas) photonMass = fBufferGas->GetPhotonMass(Ea); + + if (fDebug) { + RESTDebug << "+--------------------------------------------------------------------------+" + << RESTendl; + RESTDebug << " TRestAxionHiddenPhotonField::GammaTransmissionProbability. Parameter summary" << RESTendl; + RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; + RESTDebug << " Axion mass : " << ma << " eV" << RESTendl; + RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; + RESTDebug << " Lcoh : " << Lcoh << " mm" << RESTendl; + RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; + RESTDebug << "+--------------------------------------------------------------------------+" + << RESTendl; + } + + if (ma == 0.0 && photonMass == 0.0) return BLHalfSquared(Bmag, Lcoh); + + mpfr::mpreal q = (ma * ma - photonMass * photonMass) / 2. / Ea / 1000.0; + mpfr::mpreal l = cohLength * REST_Physics::PhMeterIneV; + mpfr::mpreal phi = q * l; + + mpfr::mpreal Gamma = absLength; + if (absLength == 0 && fBufferGas) Gamma = fBufferGas->GetPhotonAbsorptionLength(Ea); // cm-1 + mpfr::mpreal GammaL = Gamma * cohLength * 100; + + if (fDebug) { + RESTDebug << "+------------------------+" << RESTendl; + RESTDebug << " Intermediate calculations" << RESTendl; + RESTDebug << " q : " << q << " eV" << RESTendl; + RESTDebug << " l : " << l << " eV-1" << RESTendl; + RESTDebug << " phi : " << phi << RESTendl; + RESTDebug << "Gamma : " << Gamma << RESTendl; + RESTDebug << "GammaL : " << GammaL << RESTendl; + RESTDebug << "+------------------------+" << RESTendl; + } + + mpfr::mpreal MFactor = phi * phi + GammaL * GammaL / 4.0; + MFactor = 1.0 / MFactor; + + if (fDebug) { + RESTDebug << "Mfactor : " << MFactor << RESTendl; + RESTDebug << "(BL/2)^2 : " << BLHalfSquared(Bmag, Lcoh) << RESTendl; + RESTDebug << "cos(phi) : " << cos(phi) << RESTendl; + RESTDebug << "Exp(-GammaL) : " << exp(-GammaL) << RESTendl; + } + + double sol = (double)(MFactor * BLHalfSquared(Bmag, Lcoh) * GammaL); + + if (fDebug) RESTDebug << "Axion-photon absorption probability : " << sol << RESTendl; + + return sol; +#endif +} + +/// Commented because it uses ComplexReal structure that is moved to TRestAxionHiddenPhotonFieldPropagationProcess class +/* +void TRestAxionHiddenPhotonField::PropagateAxion(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, + Double_t mg, Double_t absLength) { + mpfr::mpreal axionMass = ma; + mpfr::mpreal cohLength = Lcoh / 1000.; // Default REST units are mm; + + mpfr::mpreal photonMass = mg; + if (mg == 0 && fBufferGas) photonMass = fBufferGas->GetPhotonMass(Ea); + + if (fDebug) { + RESTDebug << "+--------------------------------------------------------------------------+" << +RESTendl; RESTDebug << " TRestAxionHiddenPhotonField::GammaTransmissionProbability. Parameter summary" << +RESTendl; RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; RESTDebug << " Axion mass : " << +ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; RESTDebug << " Lcoh : " +<< Lcoh << " mm" << RESTendl; RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; RESTDebug << +"+--------------------------------------------------------------------------+" << RESTendl; + } + + mpfr::mpreal q = (ma * ma - photonMass * photonMass) / 2. / Ea / 1000.0; + mpfr::mpreal l = cohLength * PhMeterIneV; + mpfr::mpreal phi = q * l; + + mpfr::mpreal Gamma = absLength; + if (absLength == 0 && fBufferGas) Gamma = fBufferGas->GetPhotonAbsorptionLength(Ea); // cm-1 + mpfr::mpreal GammaL = Gamma * cohLength * 100; + + if (fDebug) { + RESTDebug << "+------------------------+" << RESTendl; + RESTDebug << " Intermediate calculations" << RESTendl; + RESTDebug << " q : " << q << " eV" << RESTendl; + RESTDebug << " l : " << l << " eV-1" << RESTendl; + RESTDebug << " phi : " << phi << RESTendl; + RESTDebug << "Gamma : " << Gamma << RESTendl; + RESTDebug << "GammaL : " << GammaL << RESTendl; + RESTDebug << "+------------------------+" << RESTendl; + } + + mpfr::mpreal bl = BL(Bmag, Lcoh); + + /// We have now calculated the main quantities BL, QL, and GammaL + + ComplexReal I = SetComplexReal(0, 1); + ComplexReal ExpPhi = SetComplexReal(cos(-phi), sin(-phi)); + + ComplexReal Bcomplex = SetComplexReal(BL(Bmag, Lcoh), 0); + ComplexReal Qcomplex = SetComplexReal(phi, -GammaL / 2); + + ComplexReal Bterm = ComplexCocient(Bcomplex, Qcomplex); + Bterm = ComplexProduct(I, Bterm); + + mpfr::mpreal ExpGamma = exp(-GammaL / 2.); + Double_t ExpGammaDouble = TMath::Exp((Double_t)-GammaL / 2.); + + cout.precision(30); + + if (fDebug) { + cout << "ExpGamma : " << ExpGamma << RESTendl; + cout << "ExpGammaDouble : " << ExpGammaDouble << RESTendl; + RESTDebug << "(BL/2)^2 : " << BLHalfSquared(Bmag, Lcoh) << RESTendl; + RESTDebug << "cos(phi) : " << cos(phi) << RESTendl; + RESTDebug << "Exp(-GammaL) : " << exp(-GammaL) << RESTendl; + } + + // if (fDebug) RESTDebug << "Axion-photon absorption probability : " << sol << RESTendl; +} +*/ diff --git a/src/TRestAxionField.cxx b/src/TRestAxionQCDField.cxx similarity index 90% rename from src/TRestAxionField.cxx rename to src/TRestAxionQCDField.cxx index a5cb8b94..744c5e4d 100644 --- a/src/TRestAxionField.cxx +++ b/src/TRestAxionQCDField.cxx @@ -21,7 +21,7 @@ *************************************************************************/ ////////////////////////////////////////////////////////////////////////// -/// TRestAxionField is a class used to calculate the axion-photon mixing +/// TRestAxionQCDField is a class used to calculate the axion-photon mixing /// and determine the probability of the particle being in an axion or photon /// state. /// @@ -35,15 +35,17 @@ /// /// History of developments: /// -/// 2019-March: First concept and implementation of TRestAxionField class. +/// 2019-March: First concept and implementation of TRestAxionQCDField class. /// Javier Galan +/// 2023-September: Separation of QCD and HiddenPhoton classes. +/// Tom O'Shea /// -/// \class TRestAxionField +/// \class TRestAxionQCDField /// \author Javier Galan /// ///
/// -#include "TRestAxionField.h" +#include "TRestAxionQCDField.h" #include @@ -57,32 +59,32 @@ using namespace std; -ClassImp(TRestAxionField); +ClassImp(TRestAxionQCDField); /////////////////////////////////////////////// /// \brief Default constructor /// -TRestAxionField::TRestAxionField() { Initialize(); } +TRestAxionQCDField::TRestAxionQCDField() { Initialize(); } /////////////////////////////////////////////// /// \brief Default destructor /// -TRestAxionField::~TRestAxionField() {} +TRestAxionQCDField::~TRestAxionQCDField() {} /////////////////////////////////////////////// -/// \brief Initialization of TRestAxionField class +/// \brief Initialization of TRestAxionQCDField class /// /// It sets the default real precision to be used with mpfr types. Now it is 30 digits. /// So that we can still calculate numbers such as : 1.0 - 1.e-30 /// -void TRestAxionField::Initialize() { +void TRestAxionQCDField::Initialize() { #ifdef USE_MPFR TRestComplex::SetPrecision(30); #endif fBufferGas = NULL; - /// MOVED TO TRestAxionFieldPropagationProcess class + /// MOVED TO TRestAxionQCDFieldPropagationProcess class /// faxion = SetComplexReal(1, 0); /// fAem = SetComplexReal(0, 0); } @@ -93,7 +95,7 @@ void TRestAxionField::Initialize() { /// `Lcoh` should be expressed in `mm`, and `Bmag` in `T`. /// The result will be given for an axion-photon coupling of 10^{-10} GeV^{-1} /// -double TRestAxionField::BL(Double_t Bmag, Double_t Lcoh) { +double TRestAxionQCDField::BL(Double_t Bmag, Double_t Lcoh) { Double_t lengthInMeters = Lcoh / 1000.; Double_t tm = REST_Physics::lightSpeed / REST_Physics::naturalElectron * 1.0e-9; // GeV @@ -109,7 +111,7 @@ double TRestAxionField::BL(Double_t Bmag, Double_t Lcoh) { /// `Lcoh` should be expressed in `mm`, and `Bmag` in `T`. /// The result will be given for an axion-photon coupling of 10^{-10} GeV^{-1} /// -double TRestAxionField::BLHalfSquared(Double_t Bmag, Double_t Lcoh) // (BL/2)**2 +double TRestAxionQCDField::BLHalfSquared(Double_t Bmag, Double_t Lcoh) // (BL/2)**2 { Double_t lengthInMeters = Lcoh / 1000.; @@ -134,13 +136,13 @@ double TRestAxionField::BLHalfSquared(Double_t Bmag, Double_t Lcoh) // (BL/2)** /// /// The returned value is given for g_ag = 10^-10 GeV-1 /// -Double_t TRestAxionField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, +Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" << RESTendl; - RESTWarning << "TRestAxionField::GammaTransmissionProbability will return 0" << RESTendl; + RESTWarning << "TRestAxionQCDField::GammaTransmissionProbability will return 0" << RESTendl; return 0; #else mpfr::mpreal axionMass = ma; @@ -151,7 +153,7 @@ Double_t TRestAxionField::GammaTransmissionProbability(Double_t Bmag, Double_t L if (mg == 0 && fBufferGas) photonMass = fBufferGas->GetPhotonMass(Ea); RESTDebug << "+--------------------------------------------------------------------------+" << RESTendl; - RESTDebug << " TRestAxionField::GammaTransmissionProbability. Parameter summary" << RESTendl; + RESTDebug << " TRestAxionQCDField::GammaTransmissionProbability. Parameter summary" << RESTendl; RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; RESTDebug << " Axion mass : " << ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; @@ -218,14 +220,14 @@ Double_t TRestAxionField::GammaTransmissionProbability(Double_t Bmag, Double_t L /// to solve the problem with a density profile. TOBE implemented in a new method if needed, where /// Gamma is not constant and \integral{q(z)} is integrated at each step. /// -Double_t TRestAxionField::GammaTransmissionProbability(std::vector Bmag, Double_t deltaL, +Double_t TRestAxionQCDField::GammaTransmissionProbability(std::vector Bmag, Double_t deltaL, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" << RESTendl; - RESTWarning << "TRestAxionField::GammaTransmissionProbability will return 0" << RESTendl; + RESTWarning << "TRestAxionQCDField::GammaTransmissionProbability will return 0" << RESTendl; return 0; #else mpfr::mpreal axionMass = ma; @@ -242,7 +244,7 @@ Double_t TRestAxionField::GammaTransmissionProbability(std::vector Bma if (Bmag.size() > 0) fieldAverage = std::accumulate(Bmag.begin(), Bmag.end(), 0.0) / Bmag.size(); RESTDebug << "+--------------------------------------------------------------------------+" << RESTendl; - RESTDebug << " TRestAxionField::GammaTransmissionProbability. Parameter summary" << RESTendl; + RESTDebug << " TRestAxionQCDField::GammaTransmissionProbability. Parameter summary" << RESTendl; RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; RESTDebug << " Axion mass : " << ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; @@ -317,6 +319,7 @@ Double_t TRestAxionField::GammaTransmissionProbability(std::vector Bma #endif } +/* /////////////////////////////////////////////// /// \brief Performs the calculation of axion-photon absorption probability using directly /// equation (18) from van Bibber, Phys Rev D Part Fields. 1989. @@ -330,13 +333,13 @@ Double_t TRestAxionField::GammaTransmissionProbability(std::vector Bma /// /// The returned value is given for g_ag = 10^-10 GeV-1 /// -Double_t TRestAxionField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, +Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning - << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFr=ON to your REST compilation" + << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" << RESTendl; - RESTWarning << "TRestAxionField::GammaTransmissionProbability will return 0" << RESTendl; + RESTWarning << "TRestAxionQCDField::AxionAbsorptionProbability will return 0" << RESTendl; return 0; #else mpfr::mpreal axionMass = ma; @@ -348,7 +351,7 @@ Double_t TRestAxionField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lco if (fDebug) { RESTDebug << "+--------------------------------------------------------------------------+" << RESTendl; - RESTDebug << " TRestAxionField::GammaTransmissionProbability. Parameter summary" << RESTendl; + RESTDebug << " TRestAxionQCDField::GammaTransmissionProbability. Parameter summary" << RESTendl; RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; RESTDebug << " Axion mass : " << ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; @@ -397,9 +400,11 @@ Double_t TRestAxionField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lco #endif } -/// Commented because it uses ComplexReal structure that is moved to TRestAxionFieldPropagationProcess class +*/ + +/// Commented because it uses ComplexReal structure that is moved to TRestAxionQCDFieldPropagationProcess class /* -void TRestAxionField::PropagateAxion(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, +void TRestAxionQCDField::PropagateAxion(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { mpfr::mpreal axionMass = ma; mpfr::mpreal cohLength = Lcoh / 1000.; // Default REST units are mm; @@ -409,7 +414,7 @@ void TRestAxionField::PropagateAxion(Double_t Bmag, Double_t Lcoh, Double_t Ea, if (fDebug) { RESTDebug << "+--------------------------------------------------------------------------+" << -RESTendl; RESTDebug << " TRestAxionField::GammaTransmissionProbability. Parameter summary" << +RESTendl; RESTDebug << " TRestAxionQCDField::GammaTransmissionProbability. Parameter summary" << RESTendl; RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; RESTDebug << " Axion mass : " << ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; RESTDebug << " Lcoh : " << Lcoh << " mm" << RESTendl; RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; RESTDebug << From 3e3b9358ea7a73ee2b4ee2cb91caf1b83045b851 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Wed, 27 Sep 2023 10:51:33 +0200 Subject: [PATCH 39/48] continued work on HP field --- inc/TRestAxionFieldPropagationProcess.h | 4 ++-- inc/TRestAxionHiddenPhotonField.h | 9 ++++---- inc/TRestAxionLikelihood.h | 4 ++-- src/TRestAxionFieldPropagationProcess.cxx | 2 +- src/TRestAxionHiddenPhotonField.cxx | 27 ++++++++++++++++------- src/TRestAxionLikelihood.cxx | 2 +- src/TRestAxionQCDField.cxx | 4 ++-- 7 files changed, 32 insertions(+), 20 deletions(-) diff --git a/inc/TRestAxionFieldPropagationProcess.h b/inc/TRestAxionFieldPropagationProcess.h index c12e3ac8..89461739 100644 --- a/inc/TRestAxionFieldPropagationProcess.h +++ b/inc/TRestAxionFieldPropagationProcess.h @@ -25,7 +25,7 @@ #include "TRestAxionEvent.h" #include "TRestAxionEventProcess.h" -#include "TRestAxionField.h" +#include "TRestAxionQCDField.h" #include "TRestAxionMagneticField.h" #include "TRestPhysics.h" #include "TVector3.h" @@ -44,7 +44,7 @@ class TRestAxionFieldPropagationProcess : public TRestAxionEventProcess { TRestAxionMagneticField* fMagneticField = nullptr; //! /// A pointer to TRestAxionField that implements probability calculations - TRestAxionField* fAxionField = nullptr; //! + TRestAxionQCDField* fAxionField = nullptr; //! /// A pointer to TRestBufferGas given to TRestAxionField to perform calculations in a particular gas TRestAxionBufferGas* fBufferGas = nullptr; //! diff --git a/inc/TRestAxionHiddenPhotonField.h b/inc/TRestAxionHiddenPhotonField.h index 9ea444ed..e910c7bd 100644 --- a/inc/TRestAxionHiddenPhotonField.h +++ b/inc/TRestAxionHiddenPhotonField.h @@ -36,10 +36,11 @@ class TRestAxionHiddenPhotonField : public TObject { TRestAxionBufferGas* fBufferGas = NULL; //! public: - /// momentum difference q, useful in all calculations - Double_t TRestAxionHiddenPhotonField::momentumTransfer( Double_t Ea, Double_t ma, Double_t mg ) { - return sqrt(Ea*Ea - mg*mg) - sqrt(Ea*Ea - ma*ma); - } + /// momentum difference q + Double_t momentumTransfer( Double_t Ea, Double_t ma, Double_t mg ); + + /// vacuum conversion probability + Double_t VacuumConversion(Double_t Lcoh, Double_t Ea, Double_t ma); /// It enables/disables debug mode void SetDebug(Bool_t v) { fDebug = v; } diff --git a/inc/TRestAxionLikelihood.h b/inc/TRestAxionLikelihood.h index 055bb819..5ed94db8 100644 --- a/inc/TRestAxionLikelihood.h +++ b/inc/TRestAxionLikelihood.h @@ -27,7 +27,7 @@ #include "TRandom3.h" #include "TRestAxionBufferGas.h" -#include "TRestAxionField.h" +#include "TRestAxionQCDField.h" #include "TRestAxionSolarModel.h" #include "TRestAxionSpectrum.h" @@ -62,7 +62,7 @@ class TRestAxionLikelihood : public TRestMetadata { Double_t fLastStepDensity = 0.; //-> - TRestAxionField* fAxionField; //! + TRestAxionQCDField* fAxionField; //! TRestAxionBufferGas* fBufferGas; //! TRestAxionSpectrum* fAxionSpectrum; //! diff --git a/src/TRestAxionFieldPropagationProcess.cxx b/src/TRestAxionFieldPropagationProcess.cxx index e7de98b3..03021654 100644 --- a/src/TRestAxionFieldPropagationProcess.cxx +++ b/src/TRestAxionFieldPropagationProcess.cxx @@ -171,7 +171,7 @@ void TRestAxionFieldPropagationProcess::InitProcess() { } if (!fAxionField) { - fAxionField = new TRestAxionField(); + fAxionField = new TRestAxionQCDField(); fBufferGas = (TRestAxionBufferGas*)this->GetMetadata("TRestAxionBufferGas"); if (fBufferGas) diff --git a/src/TRestAxionHiddenPhotonField.cxx b/src/TRestAxionHiddenPhotonField.cxx index 8236136b..17261911 100644 --- a/src/TRestAxionHiddenPhotonField.cxx +++ b/src/TRestAxionHiddenPhotonField.cxx @@ -87,14 +87,25 @@ void TRestAxionHiddenPhotonField::Initialize() { /// MOVED TO TRestAxionHiddenPhotonFieldPropagationProcess class /// faxion = SetComplexReal(1, 0); /// fAem = SetComplexReal(0, 0); + } + + +/////////////////////////////////////////////// +/// momentum difference q in eV, useful in all calculations +/// Ea in keV, ma in eV, mg in eV +Double_t TRestAxionHiddenPhotonField::momentumTransfer( Double_t Ea, Double_t ma, Double_t mg ) { + Ea *= 1000; // [eV] Ea is given in keV + return sqrt(Ea*Ea - mg*mg) - sqrt(Ea*Ea - ma*ma); //[eV] } /////////////////////////////////////////////// /// vacuum conversion probability /// ie. when photonMass = 0 +/// Ea in keV, ma in eV, Lcoh in mm Double_t TRestAxionHiddenPhotonField::VacuumConversion(Double_t Lcoh, Double_t Ea, Double_t ma) { - Double_t q = momentumTransfer(Ea, ma, 0.); + Lcoh *= REST_Physics::PhMeterIneV / 1000; // [eV-1] + Double_t q = momentumTransfer(Ea, ma, 0.); // [eV] return pow(2*sin(q*Lcoh/2), 2); } @@ -120,10 +131,10 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh RESTWarning << "TRestAxionHiddenPhotonField::GammaTransmissionProbability will return 0" << RESTendl; return 0; #else - mpfr::mpreal hiddenPhotonMass = ma; - mpfr::mpreal cohLength = Lcoh / 1000.; // Default REST units are mm; + mpfr::mpreal hiddenPhotonMass = ma; // [eV] + mpfr::mpreal cohLength = Lcoh / 1000.; // [m] Default REST units are mm - mpfr::mpreal photonMass = mg; + mpfr::mpreal photonMass = mg; // [eV] if (mg == 0 && fBufferGas) photonMass = fBufferGas->GetPhotonMass(Ea); @@ -133,12 +144,11 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh RESTDebug << " Hidden photon mass : " << ma << " eV" << RESTendl; RESTDebug << " Hidden photon energy : " << Ea << " keV" << RESTendl; RESTDebug << " Lcoh : " << Lcoh << " mm" << RESTendl; - RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; RESTDebug << "+--------------------------------------------------------------------------+" << RESTendl; if (photonMass == 0.0) return VacuumConversion(Lcoh, Ea, ma); - mpfr::mpreal q = momentumTransfer(Ea, ma, mg) // eV + mpfr::mpreal q = momentumTransfer(Ea, ma, mg); // eV mpfr::mpreal l = cohLength * REST_Physics::PhMeterIneV; // eV-1 mpfr::mpreal Gamma = absLength; // cm-1 @@ -152,7 +162,7 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh RESTDebug << " q : " << q << " eV" << RESTendl; RESTDebug << " l : " << l << " eV-1" << RESTendl; RESTDebug << " ql : " << q*l << RESTendl; - RESTDebug << "Gamma : " << Gamma << RESTendl; + RESTDebug << "Gamma : " << Gamma << " eV" << RESTendl; RESTDebug << "GammaL : " << GammaL << RESTendl; RESTDebug << "+------------------------+" << RESTendl; } @@ -176,7 +186,7 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh } - +/* /////////////////////////////////////////////// /// \brief Performs the calculation of the photon absorbtion probability in the buffer gas. /// @@ -253,6 +263,7 @@ Double_t TRestAxionHiddenPhotonField::AxionAbsorptionProbability(Double_t Bmag, return sol; #endif } +*/ /// Commented because it uses ComplexReal structure that is moved to TRestAxionHiddenPhotonFieldPropagationProcess class /* diff --git a/src/TRestAxionLikelihood.cxx b/src/TRestAxionLikelihood.cxx index f5d26c17..4f9b9e74 100644 --- a/src/TRestAxionLikelihood.cxx +++ b/src/TRestAxionLikelihood.cxx @@ -84,7 +84,7 @@ void TRestAxionLikelihood::Initialize() { fBufferGas = new TRestAxionBufferGas(); // Conversion probabilities as defined by van Bibber paper - fAxionField = new TRestAxionField(); + fAxionField = new TRestAxionQCDField(); fAxionField->AssignBufferGas(fBufferGas); diff --git a/src/TRestAxionQCDField.cxx b/src/TRestAxionQCDField.cxx index 744c5e4d..30d06e2f 100644 --- a/src/TRestAxionQCDField.cxx +++ b/src/TRestAxionQCDField.cxx @@ -319,7 +319,7 @@ Double_t TRestAxionQCDField::GammaTransmissionProbability(std::vector #endif } -/* + /////////////////////////////////////////////// /// \brief Performs the calculation of axion-photon absorption probability using directly /// equation (18) from van Bibber, Phys Rev D Part Fields. 1989. @@ -400,7 +400,7 @@ Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t #endif } -*/ + /// Commented because it uses ComplexReal structure that is moved to TRestAxionQCDFieldPropagationProcess class /* From d9b1946b0c42f0cc89f354b6538d496ffc328e65 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Wed, 27 Sep 2023 08:58:18 +0000 Subject: [PATCH 40/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- inc/TRestAxionFieldPropagationProcess.h | 2 +- inc/TRestAxionHiddenPhotonField.h | 16 +++--- inc/TRestAxionLikelihood.h | 2 +- src/TRestAxionHiddenPhotonField.cxx | 65 +++++++++++-------------- src/TRestAxionQCDField.cxx | 18 +++---- src/TRestAxionSolarHiddenPhotonFlux.cxx | 4 +- 6 files changed, 48 insertions(+), 59 deletions(-) diff --git a/inc/TRestAxionFieldPropagationProcess.h b/inc/TRestAxionFieldPropagationProcess.h index 89461739..8313bf50 100644 --- a/inc/TRestAxionFieldPropagationProcess.h +++ b/inc/TRestAxionFieldPropagationProcess.h @@ -25,8 +25,8 @@ #include "TRestAxionEvent.h" #include "TRestAxionEventProcess.h" -#include "TRestAxionQCDField.h" #include "TRestAxionMagneticField.h" +#include "TRestAxionQCDField.h" #include "TRestPhysics.h" #include "TVector3.h" #include "TVectorD.h" diff --git a/inc/TRestAxionHiddenPhotonField.h b/inc/TRestAxionHiddenPhotonField.h index e910c7bd..0db3630e 100644 --- a/inc/TRestAxionHiddenPhotonField.h +++ b/inc/TRestAxionHiddenPhotonField.h @@ -36,11 +36,11 @@ class TRestAxionHiddenPhotonField : public TObject { TRestAxionBufferGas* fBufferGas = NULL; //! public: - /// momentum difference q - Double_t momentumTransfer( Double_t Ea, Double_t ma, Double_t mg ); + /// momentum difference q + Double_t momentumTransfer(Double_t Ea, Double_t ma, Double_t mg); - /// vacuum conversion probability - Double_t VacuumConversion(Double_t Lcoh, Double_t Ea, Double_t ma); + /// vacuum conversion probability + Double_t VacuumConversion(Double_t Lcoh, Double_t Ea, Double_t ma); /// It enables/disables debug mode void SetDebug(Bool_t v) { fDebug = v; } @@ -51,11 +51,11 @@ class TRestAxionHiddenPhotonField : public TObject { /// It assigns a gas buffer medium to the calculation void SetBufferGas(TRestAxionBufferGas* buffGas) { fBufferGas = buffGas; } - Double_t GammaTransmissionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg = 0, Double_t absLength = 0); + Double_t GammaTransmissionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg = 0, + Double_t absLength = 0); - //Double_t PhotonAbsorptionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, - // Double_t mg = 0, Double_t absLength = 0); + // Double_t PhotonAbsorptionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, + // Double_t mg = 0, Double_t absLength = 0); TRestAxionHiddenPhotonField(); ~TRestAxionHiddenPhotonField(); diff --git a/inc/TRestAxionLikelihood.h b/inc/TRestAxionLikelihood.h index 5ed94db8..a542d1c9 100644 --- a/inc/TRestAxionLikelihood.h +++ b/inc/TRestAxionLikelihood.h @@ -62,7 +62,7 @@ class TRestAxionLikelihood : public TRestMetadata { Double_t fLastStepDensity = 0.; //-> - TRestAxionQCDField* fAxionField; //! + TRestAxionQCDField* fAxionField; //! TRestAxionBufferGas* fBufferGas; //! TRestAxionSpectrum* fAxionSpectrum; //! diff --git a/src/TRestAxionHiddenPhotonField.cxx b/src/TRestAxionHiddenPhotonField.cxx index 17261911..7c0d9560 100644 --- a/src/TRestAxionHiddenPhotonField.cxx +++ b/src/TRestAxionHiddenPhotonField.cxx @@ -87,30 +87,26 @@ void TRestAxionHiddenPhotonField::Initialize() { /// MOVED TO TRestAxionHiddenPhotonFieldPropagationProcess class /// faxion = SetComplexReal(1, 0); /// fAem = SetComplexReal(0, 0); - } - +} /////////////////////////////////////////////// /// momentum difference q in eV, useful in all calculations /// Ea in keV, ma in eV, mg in eV -Double_t TRestAxionHiddenPhotonField::momentumTransfer( Double_t Ea, Double_t ma, Double_t mg ) { - Ea *= 1000; // [eV] Ea is given in keV - return sqrt(Ea*Ea - mg*mg) - sqrt(Ea*Ea - ma*ma); //[eV] +Double_t TRestAxionHiddenPhotonField::momentumTransfer(Double_t Ea, Double_t ma, Double_t mg) { + Ea *= 1000; // [eV] Ea is given in keV + return sqrt(Ea * Ea - mg * mg) - sqrt(Ea * Ea - ma * ma); //[eV] } - /////////////////////////////////////////////// /// vacuum conversion probability /// ie. when photonMass = 0 /// Ea in keV, ma in eV, Lcoh in mm Double_t TRestAxionHiddenPhotonField::VacuumConversion(Double_t Lcoh, Double_t Ea, Double_t ma) { - Lcoh *= REST_Physics::PhMeterIneV / 1000; // [eV-1] - Double_t q = momentumTransfer(Ea, ma, 0.); // [eV] - return pow(2*sin(q*Lcoh/2), 2); + Lcoh *= REST_Physics::PhMeterIneV / 1000; // [eV-1] + Double_t q = momentumTransfer(Ea, ma, 0.); // [eV] + return pow(2 * sin(q * Lcoh / 2), 2); } - - /////////////////////////////////////////////// /// \brief Performs the calculation of hidden photon - photon conversion probability. /// @@ -123,7 +119,7 @@ Double_t TRestAxionHiddenPhotonField::VacuumConversion(Double_t Lcoh, Double_t E /// The returned value is given for chi = 1 /// Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg, Double_t absLength) { + Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" @@ -131,10 +127,10 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh RESTWarning << "TRestAxionHiddenPhotonField::GammaTransmissionProbability will return 0" << RESTendl; return 0; #else - mpfr::mpreal hiddenPhotonMass = ma; // [eV] + mpfr::mpreal hiddenPhotonMass = ma; // [eV] mpfr::mpreal cohLength = Lcoh / 1000.; // [m] Default REST units are mm - mpfr::mpreal photonMass = mg; // [eV] + mpfr::mpreal photonMass = mg; // [eV] if (mg == 0 && fBufferGas) photonMass = fBufferGas->GetPhotonMass(Ea); @@ -148,36 +144,35 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh if (photonMass == 0.0) return VacuumConversion(Lcoh, Ea, ma); - mpfr::mpreal q = momentumTransfer(Ea, ma, mg); // eV - mpfr::mpreal l = cohLength * REST_Physics::PhMeterIneV; // eV-1 + mpfr::mpreal q = momentumTransfer(Ea, ma, mg); // eV + mpfr::mpreal l = cohLength * REST_Physics::PhMeterIneV; // eV-1 - mpfr::mpreal Gamma = absLength; // cm-1 + mpfr::mpreal Gamma = absLength; // cm-1 if (absLength == 0 && fBufferGas) Gamma = fBufferGas->GetPhotonAbsorptionLength(Ea); // cm-1 mpfr::mpreal GammaL = Gamma * cohLength * 100; - Gamma *= 100 / REST_Physics::PhMeterIneV; // eV + Gamma *= 100 / REST_Physics::PhMeterIneV; // eV if (fDebug) { RESTDebug << "+------------------------+" << RESTendl; RESTDebug << " Intermediate calculations" << RESTendl; RESTDebug << " q : " << q << " eV" << RESTendl; RESTDebug << " l : " << l << " eV-1" << RESTendl; - RESTDebug << " ql : " << q*l << RESTendl; + RESTDebug << " ql : " << q * l << RESTendl; RESTDebug << "Gamma : " << Gamma << " eV" << RESTendl; RESTDebug << "GammaL : " << GammaL << RESTendl; RESTDebug << "+------------------------+" << RESTendl; } - mpfr::mpreal MFactor = pow(ma,4)/(pow(ma*ma - mg*mg, 2) + pow(Ea*Gamma, 2)); // all should be in eV - + mpfr::mpreal MFactor = + pow(ma, 4) / (pow(ma * ma - mg * mg, 2) + pow(Ea * Gamma, 2)); // all should be in eV if (fDebug) { RESTDebug << "Mfactor : " << MFactor << RESTendl; - RESTDebug << "cos(ql) : " << cos(q*l) << RESTendl; + RESTDebug << "cos(ql) : " << cos(q * l) << RESTendl; RESTDebug << "Exp(-GammaL) : " << exp(-GammaL) << RESTendl; } - double sol = - (double)(MFactor * (1 + exp(-GammaL) - 2 * exp(-GammaL / 2) * cos(q*l))); + double sol = (double)(MFactor * (1 + exp(-GammaL) - 2 * exp(-GammaL / 2) * cos(q * l))); RESTDebug << "Axion-photon transmission probability : " << sol << RESTendl; @@ -185,7 +180,6 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh #endif } - /* /////////////////////////////////////////////// /// \brief Performs the calculation of the photon absorbtion probability in the buffer gas. @@ -197,10 +191,8 @@ Double_t TRestAxionHiddenPhotonField::GammaTransmissionProbability(Double_t Lcoh /// /// The returned value is given for chi = 1 /// -Double_t TRestAxionHiddenPhotonField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg, Double_t absLength) { -#ifndef USE_MPFR - RESTWarning +Double_t TRestAxionHiddenPhotonField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, +Double_t ma, Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFr=ON to your REST compilation" << RESTendl; RESTWarning << "TRestAxionHiddenPhotonField::GammaTransmissionProbability will return 0" << RESTendl; @@ -215,13 +207,11 @@ Double_t TRestAxionHiddenPhotonField::AxionAbsorptionProbability(Double_t Bmag, if (fDebug) { RESTDebug << "+--------------------------------------------------------------------------+" << RESTendl; - RESTDebug << " TRestAxionHiddenPhotonField::GammaTransmissionProbability. Parameter summary" << RESTendl; - RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; - RESTDebug << " Axion mass : " << ma << " eV" << RESTendl; - RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; - RESTDebug << " Lcoh : " << Lcoh << " mm" << RESTendl; - RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; - RESTDebug << "+--------------------------------------------------------------------------+" + RESTDebug << " TRestAxionHiddenPhotonField::GammaTransmissionProbability. Parameter summary" << +RESTendl; RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; RESTDebug << " Axion mass : " << +ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; RESTDebug << " Lcoh : " +<< Lcoh << " mm" << RESTendl; RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; RESTDebug << +"+--------------------------------------------------------------------------+" << RESTendl; } @@ -265,7 +255,8 @@ Double_t TRestAxionHiddenPhotonField::AxionAbsorptionProbability(Double_t Bmag, } */ -/// Commented because it uses ComplexReal structure that is moved to TRestAxionHiddenPhotonFieldPropagationProcess class +/// Commented because it uses ComplexReal structure that is moved to +/// TRestAxionHiddenPhotonFieldPropagationProcess class /* void TRestAxionHiddenPhotonField::PropagateAxion(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { diff --git a/src/TRestAxionQCDField.cxx b/src/TRestAxionQCDField.cxx index 30d06e2f..b77f2886 100644 --- a/src/TRestAxionQCDField.cxx +++ b/src/TRestAxionQCDField.cxx @@ -136,8 +136,8 @@ double TRestAxionQCDField::BLHalfSquared(Double_t Bmag, Double_t Lcoh) // (BL/2 /// /// The returned value is given for g_ag = 10^-10 GeV-1 /// -Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg, Double_t absLength) { +Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, + Double_t ma, Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" @@ -221,8 +221,8 @@ Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t Bmag, Double_ /// Gamma is not constant and \integral{q(z)} is integrated at each step. /// Double_t TRestAxionQCDField::GammaTransmissionProbability(std::vector Bmag, Double_t deltaL, - Double_t Ea, Double_t ma, Double_t mg, - Double_t absLength) { + Double_t Ea, Double_t ma, Double_t mg, + Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" @@ -319,7 +319,6 @@ Double_t TRestAxionQCDField::GammaTransmissionProbability(std::vector #endif } - /////////////////////////////////////////////// /// \brief Performs the calculation of axion-photon absorption probability using directly /// equation (18) from van Bibber, Phys Rev D Part Fields. 1989. @@ -333,8 +332,8 @@ Double_t TRestAxionQCDField::GammaTransmissionProbability(std::vector /// /// The returned value is given for g_ag = 10^-10 GeV-1 /// -Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg, Double_t absLength) { +Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, + Double_t ma, Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" @@ -400,9 +399,8 @@ Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t #endif } - - -/// Commented because it uses ComplexReal structure that is moved to TRestAxionQCDFieldPropagationProcess class +/// Commented because it uses ComplexReal structure that is moved to TRestAxionQCDFieldPropagationProcess +/// class /* void TRestAxionQCDField::PropagateAxion(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 87b3360b..b0a234bf 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -389,8 +389,8 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG h->Multiply(fContinuumTable[n]); // wG * flux h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + (w - // G)^2 + // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + + // (w G)^2 // ) fFluxTable.push_back(h); From 60274a150e904cf69f375e3662be648facb42711 Mon Sep 17 00:00:00 2001 From: tomasoshea Date: Wed, 27 Sep 2023 11:07:37 +0200 Subject: [PATCH 41/48] moved images --- flux.png | Bin 32743 -> 0 bytes .../SolarHiddenPhotonFlux/flux0.001.png | Bin .../SolarHiddenPhotonFlux/flux0.01.png | Bin .../SolarHiddenPhotonFlux/flux0.1.png | Bin .../SolarHiddenPhotonFlux/flux1.png | Bin .../SolarHiddenPhotonFlux/flux10.png | Bin .../SolarHiddenPhotonFlux/flux100.png | Bin .../SolarHiddenPhotonFlux/flux1000.png | Bin .../SolarHiddenPhotonFlux/flux20.png | Bin .../SolarHiddenPhotonFlux/flux30.png | Bin .../SolarHiddenPhotonFlux/flux50.png | Bin 11 files changed, 0 insertions(+), 0 deletions(-) delete mode 100644 flux.png rename flux0.001.png => images/SolarHiddenPhotonFlux/flux0.001.png (100%) rename flux0.01.png => 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zF6smK{eu(SRFLXZyn0EWK8ADe#{g!9x(na+#ue)M(rrw+e;|Cby0@8CJzIFv!~h0A z{%^j5u|2OM{`UlZXi9mYqkz7E0HCD_$PLjSa>Iw-kOu|@Vgcl5|ChP_|KwM1B(C8R W0|B}6nSi$uNI^ygQX*yY`TqmsV$ Date: Wed, 27 Sep 2023 09:08:25 +0000 Subject: [PATCH 42/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index b0a234bf..178f4cb5 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -389,8 +389,8 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG h->Multiply(fContinuumTable[n]); // wG * flux h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + - // (w G)^2 + // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 + // + (w G)^2 // ) fFluxTable.push_back(h); From 4ee82fc3e3ae009f445db5833c2a325957c68947 Mon Sep 17 00:00:00 2001 From: Javier Galan Date: Tue, 3 Oct 2023 08:36:05 +0200 Subject: [PATCH 43/48] Update src/TRestAxionSolarHiddenPhotonFlux.cxx MIME-Version: 1.0 Content-Type: text/plain; charset=UTF-8 Content-Transfer-Encoding: 8bit Co-authored-by: Juan Antonio García <80903717+juanangp@users.noreply.github.com> --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 7 +++---- 1 file changed, 3 insertions(+), 4 deletions(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 178f4cb5..7884b94d 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -389,10 +389,9 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG h->Multiply(fContinuumTable[n]); // wG * flux h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - // h->Scale(pow(mass, 4)); // m4 * wG * flux / ( (m2 - wp2)^2 - // + (w G)^2 - // ) - + + // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2) + // h->Scale(pow(mass, 4)); fFluxTable.push_back(h); } } From 1e9d52f5fafb448cd4cdef1e63db2696929fd6a6 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Tue, 3 Oct 2023 06:36:14 +0000 Subject: [PATCH 44/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- src/TRestAxionSolarHiddenPhotonFlux.cxx | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/src/TRestAxionSolarHiddenPhotonFlux.cxx b/src/TRestAxionSolarHiddenPhotonFlux.cxx index 7884b94d..66ffa0ec 100644 --- a/src/TRestAxionSolarHiddenPhotonFlux.cxx +++ b/src/TRestAxionSolarHiddenPhotonFlux.cxx @@ -389,7 +389,7 @@ void TRestAxionSolarHiddenPhotonFlux::CalculateSolarFlux() { TH1D* h = (TH1D*)fWidthTable[n]->Clone(); // wG h->Multiply(fContinuumTable[n]); // wG * flux h->Divide(hMass); // wG * flux / ( (m2 - wp2)^2 + (w G)^2 ) - + // m4 * wG * flux / ( (m2 - wp2)^2 + (w G)^2) // h->Scale(pow(mass, 4)); fFluxTable.push_back(h); From 3bb32600a25e74957a6b613969f1245a0b0091f5 Mon Sep 17 00:00:00 2001 From: Javier Galan Date: Sun, 21 Jan 2024 13:52:51 +0100 Subject: [PATCH 45/48] TRestAxionQCDField fixing conflicts --- src/TRestAxionQCDField.cxx | 31 +++---------------------------- 1 file changed, 3 insertions(+), 28 deletions(-) diff --git a/src/TRestAxionQCDField.cxx b/src/TRestAxionQCDField.cxx index c2ce782f..af766fe3 100644 --- a/src/TRestAxionQCDField.cxx +++ b/src/TRestAxionQCDField.cxx @@ -344,12 +344,7 @@ Double_t TRestAxionQCDField::GammaTransmissionProbability(std::vector /// /// The returned value is given for g_ag = 10^-10 GeV-1 /// -<<<<<<< HEAD:src/TRestAxionQCDField.cxx -Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, - Double_t ma, Double_t mg, Double_t absLength) { -======= -Double_t TRestAxionField::AxionAbsorptionProbability(Double_t ma, Double_t mg, Double_t absLength) { ->>>>>>> master:src/TRestAxionField.cxx +Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t ma, Double_t mg, Double_t absLength) { #ifndef USE_MPFR RESTWarning << "MPFR libraries not linked to REST libraries. Try adding -DREST_MPFR=ON to your REST compilation" @@ -415,38 +410,19 @@ Double_t TRestAxionField::AxionAbsorptionProbability(Double_t ma, Double_t mg, D #endif } -<<<<<<< HEAD:src/TRestAxionQCDField.cxx -/// Commented because it uses ComplexReal structure that is moved to TRestAxionQCDFieldPropagationProcess -/// class -/* -void TRestAxionQCDField::PropagateAxion(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg, Double_t absLength) { - mpfr::mpreal axionMass = ma; - mpfr::mpreal cohLength = Lcoh / 1000.; // Default REST units are mm; -======= /////////////////////////////////////////////// /// \brief On top of calculating the axion absorption probability it will assign new values /// for the magnetic field (Bmag/T), coherence length (Lcoh/mm) and axion energy (Ea/keV). /// -Double_t TRestAxionField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, +Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { fBmag = Bmag; fLcoh = Lcoh; fEa = Ea; ->>>>>>> master:src/TRestAxionField.cxx return AxionAbsorptionProbability(ma, mg, absLength); } -<<<<<<< HEAD:src/TRestAxionQCDField.cxx - if (fDebug) { - RESTDebug << "+--------------------------------------------------------------------------+" << -RESTendl; RESTDebug << " TRestAxionQCDField::GammaTransmissionProbability. Parameter summary" << -RESTendl; RESTDebug << " Photon mass : " << photonMass << " eV" << RESTendl; RESTDebug << " Axion mass : " << -ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << RESTendl; RESTDebug << " Lcoh : " -<< Lcoh << " mm" << RESTendl; RESTDebug << " Bmag : " << Bmag << " T" << RESTendl; RESTDebug << -"+--------------------------------------------------------------------------+" << RESTendl; -======= /////////////////////////////////////////////// /// \brief Performs the calculation of the FWHM for the axion-photon conversion probability /// computed in `TRestAxionField::GammaTransmissionProbability`. @@ -459,7 +435,7 @@ ma << " eV" << RESTendl; RESTDebug << " Axion energy : " << Ea << " keV" << REST /// IMPORTANT: In the case that the buffer gas is not defined, this method will return the mass at which the /// probability reaches half of the maximum **vacuum** probability. /// -Double_t TRestAxionField::GammaTransmissionFWHM(Double_t step) { +Double_t TRestAxionQCDField::GammaTransmissionFWHM(Double_t step) { Double_t maxMass = 10; // 10eV is the maximum mass (exit condition) Double_t resonanceMass = 0; @@ -476,7 +452,6 @@ Double_t TRestAxionField::GammaTransmissionFWHM(Double_t step) { << RESTendl; return maxMass; } ->>>>>>> master:src/TRestAxionField.cxx } Double_t fwhm = scanMass - resonanceMass; From ca1961aff218d70cfd69f8bbc35c56c5f56ecf28 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Sun, 21 Jan 2024 12:53:02 +0000 Subject: [PATCH 46/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- src/TRestAxionQCDField.cxx | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/src/TRestAxionQCDField.cxx b/src/TRestAxionQCDField.cxx index af766fe3..e83006cb 100644 --- a/src/TRestAxionQCDField.cxx +++ b/src/TRestAxionQCDField.cxx @@ -414,8 +414,8 @@ Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t ma, Double_t mg /// \brief On top of calculating the axion absorption probability it will assign new values /// for the magnetic field (Bmag/T), coherence length (Lcoh/mm) and axion energy (Ea/keV). /// -Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg, Double_t absLength) { +Double_t TRestAxionQCDField::AxionAbsorptionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, + Double_t ma, Double_t mg, Double_t absLength) { fBmag = Bmag; fLcoh = Lcoh; fEa = Ea; From 7205cecd4d32e901531bb3ce017ec0f0eb3ef596 Mon Sep 17 00:00:00 2001 From: Javier Galan Date: Sun, 21 Jan 2024 13:57:12 +0100 Subject: [PATCH 47/48] TRestAxionQCDField. Fixing compilation issues --- src/TRestAxionQCDField.cxx | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/src/TRestAxionQCDField.cxx b/src/TRestAxionQCDField.cxx index e83006cb..72605e90 100644 --- a/src/TRestAxionQCDField.cxx +++ b/src/TRestAxionQCDField.cxx @@ -204,7 +204,7 @@ Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t ma, Double_t /// \brief On top of calculating the gamma transmission probability it will assign new values /// for the magnetic field (Bmag/T), coherence length (Lcoh/mm) and axion energy (Ea/keV). /// -Double_t TRestAxionField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, +Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, Double_t mg, Double_t absLength) { fBmag = Bmag; fLcoh = Lcoh; @@ -483,7 +483,7 @@ Double_t TRestAxionQCDField::GammaTransmissionFWHM(Double_t step) { /// /// For additional info see PR: https://github.com/rest-for-physics/axionlib/pull/78 /// -std::vector> TRestAxionField::GetMassDensityScanning(std::string gasName, +std::vector> TRestAxionQCDField::GetMassDensityScanning(std::string gasName, double maMax, double rampDown) { std::vector> massDensityPairs; From b05d3f3e2b8b8bd013d2f449b9e886abd1763786 Mon Sep 17 00:00:00 2001 From: "pre-commit-ci[bot]" <66853113+pre-commit-ci[bot]@users.noreply.github.com> Date: Sun, 21 Jan 2024 12:57:32 +0000 Subject: [PATCH 48/48] [pre-commit.ci] auto fixes from pre-commit.com hooks for more information, see https://pre-commit.ci --- src/TRestAxionQCDField.cxx | 8 ++++---- 1 file changed, 4 insertions(+), 4 deletions(-) diff --git a/src/TRestAxionQCDField.cxx b/src/TRestAxionQCDField.cxx index 72605e90..6a5c5f3a 100644 --- a/src/TRestAxionQCDField.cxx +++ b/src/TRestAxionQCDField.cxx @@ -204,8 +204,8 @@ Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t ma, Double_t /// \brief On top of calculating the gamma transmission probability it will assign new values /// for the magnetic field (Bmag/T), coherence length (Lcoh/mm) and axion energy (Ea/keV). /// -Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, Double_t ma, - Double_t mg, Double_t absLength) { +Double_t TRestAxionQCDField::GammaTransmissionProbability(Double_t Bmag, Double_t Lcoh, Double_t Ea, + Double_t ma, Double_t mg, Double_t absLength) { fBmag = Bmag; fLcoh = Lcoh; fEa = Ea; @@ -484,8 +484,8 @@ Double_t TRestAxionQCDField::GammaTransmissionFWHM(Double_t step) { /// For additional info see PR: https://github.com/rest-for-physics/axionlib/pull/78 /// std::vector> TRestAxionQCDField::GetMassDensityScanning(std::string gasName, - double maMax, - double rampDown) { + double maMax, + double rampDown) { std::vector> massDensityPairs; // Storing the gas pointer, if there was one