Abstract

Supersymmetric models with Dirac instead of Majorana gaugino masses have distinct phenomenological consequences. In this paper, we investigate the electroweakino sector of the Minimal Dirac Gaugino Supersymmetric Standard Model (MDGSSM) with regards to dark matter (DM) and collider constraints. We delineate the parameter space where the lightest neutralino of the MDGSSM is a viable DM candidate, that makes for at least part of the observed relic abundance while evading constraints from DM direct detection, LEP and low-energy data, and LHC Higgs measurements. The collider phenomenology of the thus emerging scenarios is characterised by the richer electroweakino spectrum as compared to the Minimal Supersymmetric Standard Model (MSSM) -6 neutralinos and 3 charginos instead of 4 and 2 in the MSSM, naturally small mass splittings, and the frequent presence of long-lived particles, both charginos and/or neutralinos. Reinterpreting ATLAS and CMS analyses with the help of SmodelS and MadAnalysis 5, we discuss the sensitivity of existing LHC searches for new physics to these scenarios and show which cases can be constrained and which escape detection. Finally, we propose a set of benchmark points which can be useful for further studies, designing dedicated experimental analyses and/or investigating the potential of future experiments.

Highlights

  • Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, 53 Avenue des Martyrs, 38026 Grenoble, France

  • We investigated the electroweakino sector of the Minimal Dirac Gaugino Supersymmetric Standard Model

  • The Minimal Dirac Gaugino Supersymmetric Standard Model (MDGSSM) can be defined as the minimal Dirac gaugino extension of the Minimal Supersymmetric Standard Model (MSSM): to introduce Dirac gauginos (DG) masses, one adjoint chiral superfield is added for each gauge group, but nothing else

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Summary

Introduction

Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, 53 Avenue des Martyrs, 38026 Grenoble, France. For comparison with [97,98,99], in Figure 1 we reproduce Fig. 6 from [98] (same as Fig. 1 in [99]) with our code by taking the MSSM-limit of our model; we add Majorana gaugino masses for the wino fixed at M2 = 200 GeV and scan over values for the bino mass of

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