Publication:
Muon g − 2, Dark Matter, and Lepton Flavor Violation in SUSY-GUT’s

dc.contributor.authorGómez, M.E.
dc.contributor.authorLola, S.
dc.contributor.authorShafi, Q.
dc.contributor.authorTiwari, A.
dc.contributor.authorÜn, C.S.
dc.contributor.buuauthorÜN, CEM SALİH
dc.contributor.departmentFen Edebiyat Fakültesi
dc.contributor.departmentFizik Ana Bilim Dalı
dc.contributor.orcid0000-0002-0595-8803
dc.contributor.scopusid55325758100
dc.date.accessioned2025-05-13T06:29:30Z
dc.date.issued2023-01-01
dc.description.abstractWe perform an analysis of the predictions of several supersymmetric Grand Unified Theories (GUTs) for Dark Matter and the measurements of the muon anomalous magnetic moment (muon g − 2) consistent with possible Lepton Flavor Violating (LFV) signal in charged lepton decays. Each GUT predicts different Dark Matter (DM) scenarios, which can be used to classify SUSY models and contrast their predictions with experimental evidences. We find that models arising from SU(4)c × SU(2)L × SU(2)R can predict DM of cosmological interest while explaining the observed value of the muon g − 2. Furthermore, we show that when this framework is extended with a simple type 1 seesaw mechanism to explain neutrino masses, many models also predict charged LFV decays that can be observed in current experiments.
dc.identifier.doi10.31526/LHEP.2023.381
dc.identifier.issn2632-2714
dc.identifier.scopus2-s2.0-85159212996
dc.identifier.urihttps://hdl.handle.net/11452/51626
dc.identifier.volume2023
dc.indexed.scopusScopus
dc.language.isoen
dc.publisherAndromeda Publishing And Academic Services LTD
dc.relation.journalLetters in High Energy Physics
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectSupersymmetry
dc.subjectPhenomenology
dc.subject.scopusLepton; Muon; Physics
dc.titleMuon g − 2, Dark Matter, and Lepton Flavor Violation in SUSY-GUT’s
dc.typeArticle
dspace.entity.typePublication
local.contributor.departmentFen Edebiyat Fakültesi/Fizik Ana Bilim Dalı
relation.isAuthorOfPublication0c6ad07c-f6f6-4949-a2f0-e288af6b9411
relation.isAuthorOfPublication.latestForDiscovery0c6ad07c-f6f6-4949-a2f0-e288af6b9411

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