Signatures of sneutrino dark matter in an extension of the CMSSM
Shankha Banerjee, Genevi\`eve B\'elanger, Biswarup Mukhopadhyaya and, Pasquale D. Serpico

TL;DR
This paper explores a supersymmetric extension of the CMSSM incorporating right-handed sneutrinos as dark matter candidates, highlighting distinctive signatures like heavy charged particles and promising detection prospects at the LHC and MoEDAL.
Contribution
It introduces the $ ilde u$CMSSM model with right-handed sneutrinos and analyzes its phenomenology, especially the detection potential of long-lived staus at future collider runs.
Findings
Stau masses up to 600 GeV can be probed at the 14 TeV LHC with 1100 fb$^{-1}$.
The model predicts heavy, stable charged particles with distinctive signatures.
Future experiments like MoEDAL can complement collider searches.
Abstract
Current data (LHC direct searches, Higgs mass, dark matter-related bounds) severely affect the constrained minimal SUSY standard model (CMSSM) with neutralinos as dark matter candidates. But the evidence for neutrino masses coming from oscillations requires extending the SM with at least right-handed neutrinos with a Dirac mass term. In turn, this implies extending the CMSSM with right-handed sneutrino superpartners, a scenario we dub CMSSM. These additional states constitute alternative dark matter candidates of the superWIMP type, produced via the decay of the long-lived next-to-lightest SUSY particle (NLSP). Here we consider the interesting and likely case where the NLSP is a : despite the modest extension with respect to the CMSSM this scenario has the distinctive signatures of heavy, stable charged particles. After taking into account the role played by…
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