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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/15349
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dc.contributor.authorMondal, Tanmoy-
dc.date.accessioned2024-08-22T06:57:44Z-
dc.date.available2024-08-22T06:57:44Z-
dc.date.issued2019-02-
dc.identifier.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.035018-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/15349-
dc.description.abstractWe consider the minimal supersymmetric standard model (MSSM) with right-chiral neutrino superfields with Majorana masses, where the lightest right-handed sneutrino dominated scalars constitutes nonthermal dark matter (DM). The Δ⁢𝐿=2 masses are subject to severe constraints coming from freeze-in relic density of such DM candidates as well as from sterile neutrino freeze-in. In addition, big bang nucleosynthesis and freeze-out of the next-to-lightest superparticle shrink the viable parameter space of such a scenario. We examine various Δ⁢𝐿=2 mass terms for families other than that corresponding to the LSP sneutrino. Δ⁢𝐿=2 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.en_US
dc.language.isoenen_US
dc.publisherAPSen_US
dc.subjectPhysicsen_US
dc.subjectMinimal supersymmetric standard model (MSSM)en_US
dc.titleRight sneutrino with Δ⁢𝐿��=2 masses as nonthermal dark matteren_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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