Please use this identifier to cite or link to this item: http://hdl.handle.net/11452/34231
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dc.contributor.authorShafi, Qaisar-
dc.contributor.authorTanyıldızı, Suekrue Hanif-
dc.date.accessioned2023-10-06T05:47:22Z-
dc.date.available2023-10-06T05:47:22Z-
dc.date.issued2015-11-01-
dc.identifier.citationShafi, Q. vd. (2015). "Neutralino dark matter and other LHC predictions from quasi Yukawa unification". Nuclear Physics B, 900, 400-411.en_US
dc.identifier.issn0550-3213-
dc.identifier.urihttps://doi.org/10.1016/j.nuclphysb.2015.09.019-
dc.identifier.urihttps://www.sciencedirect.com/science/article/pii/S0550321315003387-
dc.identifier.urihttp://hdl.handle.net/11452/34231-
dc.description.abstractWe explore the dark matter and LHC implications of t - b - tau quasi Yukawa unification in the framework of supersymmetric models based on the gauge symmetry G = SU(4)(c) x SU(2)(L) x SU(2)(R). The deviation from exact Yukawa unification is quantified by a dimensionless parameter C(vertical bar C vertical bar less than or similar to 0.2), such that the Yukawa couplings at M-GUT are related by yt : yb : y tau = vertical bar 1 + C vertical bar : vertical bar 1 -C vertical bar : vertical bar 1 + 3C vertical bar. In contrast to earlier studies which focused on universal gaugino masses, we consider non-universal gaugino masses at M-GUT that are compatible with the gauge symmetry G. Our results reveal a variety of neutralino dark matter scenarios consistent with the observations. These include stau and chargino coannihilation scenarios, the A-resonance scenario, as well as Higgsino dark matter solutions which are more readily probed by direct detection searches. The gluino mass is found to be less than or similar to 4 TeV, the stop mass is greater than or similar to 2 TeV, while the first two family squarks and sleptons are of order 4-5 TeV and 3 TeV respectively.en_US
dc.description.sponsorshipUnited States Department of Energy (DOE) (DE-SC0013880)en_US
dc.description.sponsorshipRussian Foundation for Basic Research (RFBR) (14-02-00494-a)en_US
dc.description.sponsorshipNational Science Foundation (NSF) (OCI-1053575)en_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.rightsinfo:eu-repo/semantics/openAccess*
dc.rightsAtıf Gayri Ticari Türetilemez 4.0 Uluslararasıtr_TR
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectLeft-right symmetryen_US
dc.subjectSupersymmetry-breakingen_US
dc.subjectGrand unificationen_US
dc.subjectModelen_US
dc.subjectPhysicsen_US
dc.titleNeutralino dark matter and other LHC predictions from quasi Yukawa unificationen_US
dc.typeArticleen_US
dc.identifier.wos000364323000015tr_TR
dc.identifier.scopus2-s2.0-84955469655tr_TR
dc.relation.tubitakMFAG-114F461tr_TR
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergitr_TR
dc.contributor.departmentUludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü.tr_TR
dc.contributor.orcid0000-0002-0595-8803tr_TR
dc.identifier.startpage400tr_TR
dc.identifier.endpage411tr_TR
dc.identifier.volume900tr_TR
dc.relation.journalNuclear Physics Ben_US
dc.contributor.buuauthorUn, Cem Salih-
dc.contributor.researcheridN-3421-2014tr_TR
dc.relation.collaborationYurt dışıtr_TR
dc.relation.collaborationYurt içitr_TR
dc.subject.wosPhysics, Particles & Fieldsen_US
dc.indexed.wosSCIEen_US
dc.indexed.scopusScopusen_US
dc.wos.quartileQ2en_US
dc.contributor.scopusid55325758100tr_TR
dc.subject.scopusHiggs bosons; Supersymmetry; Higgsen_US
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