arXiv:1807.04964·v2·High Energy Physics — Phenomenology
Right sneutrino with masses as non-thermal dark matter
Avirup Ghosh🇮🇳 · Tanmoy Mondal🇮🇳 · Biswarup Mukhopadhyaya🇮🇳
Abstract
We consider MSSM with right-chiral neutrino superfields with Majorana masses, where the lightest right-handed sneutrino dominated scalars constitutes non-thermal dark matter (DM). The masses are subject to severe constraints coming from freeze-in relic density of such DM candidates as well as from sterile neutrino . In addition, big-bang Nucleosynthesis and of the next-to-lightest superparticle shrink the viable parameter space of such a scenario. We examine various mass terms for families other than that masses are difficult to reconcile with a right-sneutrino DM, unless there is either (a) a hierarchy of about 3 orders of magnitudes among various supersymmetry-breaking mass parameters, or, (b) strong cancellation between the higgsino mass and the trilinear supersymmetry breaking mass parameter for sneutrinos.
Comments: 15 pages, 12 figure, 1 Table, Version matches the version published in Physical Review D