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Sneutrino dark matter, constraints and perspectives

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dc.contributor.authorRose, L. D.
dc.contributor.authorKhalil, S.
dc.contributor.authorKing, S. J. D.
dc.contributor.authorKulkarni, S.
dc.contributor.authorMarzo, C.
dc.contributor.authorMoretti, S.
dc.contributor.authorUn, C. S.
dc.contributor.buuauthorÜN, CEM SALİH
dc.contributor.departmentFizik Bölümü
dc.contributor.orcid0000-0002-0595-8803
dc.contributor.scopusid55325758100
dc.date.accessioned2025-08-06T23:03:05Z
dc.date.issued2018-01-01
dc.description.abstractThe prevalent Dark Matter (DM) candidate of the (B − L) Supersymmetric Standard Model (BLSSM) is the Right Handed (RH) sneutrino. In this work we assess the ability of ground and space based experiments to establish the nature of this particle, through indirect and collider detection.
dc.identifier.endpage426
dc.identifier.isbn[9791096879076]
dc.identifier.scopus2-s2.0-85088703083
dc.identifier.startpage423
dc.identifier.urihttps://hdl.handle.net/11452/53608
dc.indexed.scopusScopus
dc.language.isoen
dc.publisherARISF
dc.relation.journalProceedings of the 53rd Rencontres De Moriond 2018 Electroweak Interactions and Unified Theories Ew 2018
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.titleSneutrino dark matter, constraints and perspectives
dc.typeconferenceObject
dc.type.subtypeConference Paper
dspace.entity.typePublication
local.contributor.departmentFizik Bölümü
local.indexed.atScopus
relation.isAuthorOfPublication0c6ad07c-f6f6-4949-a2f0-e288af6b9411
relation.isAuthorOfPublication.latestForDiscovery0c6ad07c-f6f6-4949-a2f0-e288af6b9411

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