Light mixed sneutrinos as thermal dark matter
G. Belanger, M. Kakizaki, E. K. Park, S. Kraml, A. Pukhov

TL;DR
This paper explores the potential of light mixed sneutrinos in supersymmetric models with Dirac neutrino masses to serve as viable thermal dark matter candidates, analyzing their detection prospects and collider signatures.
Contribution
It provides a detailed analysis of light sneutrino dark matter within MSSM+$ ilde u_R$ models, highlighting their viability and phenomenological implications.
Findings
Light sneutrinos below 10 GeV can be viable dark matter candidates.
Implications for direct and indirect detection are discussed with uncertainties.
Collider phenomenology of light sneutrino dark matter is analyzed.
Abstract
In supersymmetric models with Dirac neutrino masses, a left-right mixed sneutrino can be a viable dark matter candidate. We examine the MSSM+ parameter space where this is the case with particular emphasis on light sneutrinos with masses below 10 GeV. We discuss implications for direct and indirect dark matter searches, including the relevant uncertainties, as well as consequences for collider phenomenology.
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