Published January 9, 2024 | Version v1
Dataset Open

Datasets used in "Global LHC constraints on electroweak-inos with SModelS v2.3"

  • 1. Univ. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, Grenoble, France
  • 2. Centro de Ciencias Naturais e Humanas, UFABC, Santo Andre, Brazil
  • 3. HEPHY/OEAW and University of Vienna, Vienna, Austria
  • 4. Université de Lyon, CNRS/IN2P3, Institut de Physique des 2 Infinis de Lyon, Villeurbanne, France

Description

Input SLHA and SModelS output (.smodels and .py) files from the paper "Global LHC constraints on electroweak-inos with SModelS v2.3". The datasets comprises 18247 electroweak-ino scan points and can be used to reproduce results in sections 4 and 5, and in appendix B.

  • ewino_slhaFiles.tar.gz : input SLHA files including mass spectra, decay tables and cross sections.
  • ewino_smodels_mmg10.tar.gz : SModelS outputs with a minmassgap of 10 GeV (value used for the results presented in the main text, used for Figures 12-21). All the 18247 scan points present in the directory were obtained using this minmassgap.
  • ewino_smodels_mmg05.tar.gz : SModelS outputs with a minmassgap of 5 GeV (value used in appendix B, used for Figures 23 and 24). All the 18247 scan points present in the directory were obtained using this minmassgap.
  • ewino_smodels_mmg15.tar.gz : SModelS outputs with a minmassgap of 15 GeV (value used in appendix B, used for Figures 23 and 24). Only the points with a mass difference between the next-to-lightest neutralino and the lightest neutralino, or the next-to-lightest neutralino and the lightest chargino, or the lightest chargino and the lightest neutralino comprised between 10 and 15 GeV were computed using this minmassgap. This corresponds to 1732 scan points, which are listed in the summary.txt present in the compressed directory. The results for the remaining points were obtained using a minmassgap of 10 GeV.
  • ewino_smodels_mmg20.tar.gz : SModelS outputs with a minmassgap of 20 GeV (value used in appendix B, used for Figures 23 and 24). Only the points with a mass difference between the next-to-lightest neutralino and the lightest neutralino, or the next-to-lightest neutralino and the lightest chargino, or the lightest chargino and the lightest neutralino comprised between 15 and 20 GeV were computed using this minmassgap. This corresponds to 870 scan points, which are listed in the summary.txt present in the compressed directory. The results for the remaining points were obtained using a minmassgap of 15 or 10 GeV (depending on the mass difference condition mentioned in the previous paragraph).
  • combinability_matrix.py: python dictionnary modelling the combinability matrix (Figure 11).

Notes (English)

MMA is supported by the French Agence Nationale de la Recherche (ANR) under grant ANR-21-CE31-0023 (PRCI SLDNP). SN is supported by the Austrian Science Fund (FWF) under grant number I 5767-N. TP is supported by the Initiatives de Recherche à Grenoble Alpes (IRGA) ANR-15-IDEX-02 project no. G7H-IRG21B26 (APM@LHC). AL is supported by FAPESP grant no. 2018/25225-9 and 2021/01089-1. The work presented here was, moreover, supported in part by the IN2P3 master project “Théorie – BSMGA”.

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Additional details

Related works

Continues
Publication: arXiv:2306.17676 (arXiv)
Dataset: 10.5281/zenodo.8275263 (DOI)

Funding

Statistically Learning Dispersed New Physics at the LHC 15767
FWF Austrian Science Fund
SLDNP – Statistically Learning Dispersed New Physics at the LHC ANR-21-CE31-0023
Agence Nationale de la Recherche
UGA – IDEX UGA ANR-15-IDEX-0002
Agence Nationale de la Recherche