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Collider constraints on electroweakinos in the presence of a light gravitino

  • GAMBIT Collaboration
  • University of Oslo
  • Monash University
  • King's College London
  • University of Glasgow
  • University College London
  • University of Queensland
  • Simon Fraser University
  • Karlsruhe Institute of Technology
  • Universite Claude Bernard Lyon 1
  • CERN
  • University of California at Los Angeles
  • University of Bonn
  • Australian National University
  • RWTH Aachen University
  • Telenor ASA
  • University of Adelaide
  • Zhengzhou University
  • CAS - Institute of Theoretical Physics

Research output: Contribution to journalArticlepeer-review

11 Citations (Scopus)

Abstract

Using the GAMBIT global fitting framework, we constrain the MSSM with an eV-scale gravitino as the lightest supersymmetric particle, and the six electroweakinos (neutralinos and charginos) as the only other light new states. We combine 15 ATLAS and 12 CMS searches at 13 TeV, along with a large collection of ATLAS and CMS measurements of Standard Model signatures. This model, which we refer to as the G~ -EWMSSM, exhibits quite varied collider phenomenology due to its many permitted electroweakino production processes and decay modes. Characteristic G~ -EWMSSM signal events have two or more Standard Model bosons and missing energy due to the escaping gravitinos. While much of the G~ -EWMSSM parameter space is excluded, we find several viable parameter regions that predict phenomenologically rich scenarios with multiple neutralinos and charginos within the kinematic reach of the LHC during Run 3, or the High Luminosity LHC. In particular, we identify scenarios with Higgsino-dominated electroweakinos as light as 140 GeV that are consistent with our combined set of collider searches and measurements. The full set of G~ -EWMSSM parameter samples and GAMBIT input files generated for this work is available via Zenodo.

Original languageEnglish
Article number493
JournalEuropean Physical Journal C
Volume83
Issue number6
DOIs
Publication statusPublished - Jun 2023

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