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This repo contains the code, files, and runcards required to reproduce and analyse the PDF fits in the presence of New Physics presented in [arXiv:2307.10370](https://arxiv.org/pdf/2307.10370.pdf).

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PBSP_PDFs_newphysics

This repo contains the code, files, and runcards required to reproduce and analyse the PDF fits in the presence of New Physics presented in arXiv:2307.10370.

Instructions

1. Install NNPDF4.0

Our analysis makes use of the NNPDF4.0 methodology (arXiv:2109.02653, arXiv:2109.02671), so make sure to install it first by following the instructions given in here.

2. Running contaminated fits

Preparing data and theory predictions

Before launching a contaminated fit, you will need to ensure that the C-factors, FK-tables, commondata, systype and plotting files are all in the correct place. This can be achieved using:

cp -r files_for_commondata/* /path/to/miniconda3/envs/contamination-dev/share/NNPDF/data/commondata/.
cp -r files_for_theory/* /path/to/miniconda3/envs/contamination-dev/share/NNPDF/data/theory_num/.

where theory_num is the appropriate theory you would like to work with (e.g. theory_53, theory_200) and contamination-dev is the name of the conda environment of your NNPDF4.0 installation.

You will also need to copy and paste the filters.yaml file to the correct location, via:

cp filters.yaml /path/to/nnpdf/installation/nnpdf/validphys2/src/validphys/cuts/.

Launching contaminated fits

The code for launching contaminated fits is contained in the code folder. Running the code follows the standard NNPDF pipeline (which can be found here), with a small modification in the first step.

Instead of running vp-setupfit on a runcard first, you should run:

validphys example_contamination.yaml -x contamination_provider.py

The example_contamination.yaml file is the basic runcard for the contaminated fit, together with some additional namespaces. Executing the above command will do the following:

  • Create new SMEFT C-factor files in the correct directory, scaled to the required user-specified values.
  • Write a new runcard with the C-factor names changed to appropriate scaled names, allowing the scaled values to be used.
  • Launch vp-setupfit.
  • Launch vp-rebuild-data to build the correct commondata.
  • Remove the runcard containing the SMEFT C-factors, and replace it with a SM runcard.

After this, the pipeline is identical to a normal NNPDF fit. Run n3fit, evolven3fit and postfit as described here).

3. Analysing contaminated fits

The code for analysing contaminated fits is contained in the analysis_code folder. Run the code via the command:

validphys example_analysis.yaml -x analysis_provider.py

The example_analysis.yaml file contains all the information needed for the analysis. A validphys report will be produced from the analysis which can be uploaded to the server and shared.

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This repo contains the code, files, and runcards required to reproduce and analyse the PDF fits in the presence of New Physics presented in [arXiv:2307.10370](https://arxiv.org/pdf/2307.10370.pdf).

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