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Neutralino dark matter and other LHC predictions from quasi Yukawa unification

dc.contributor.authorShafi, Qaisar
dc.contributor.authorTanyıldızı, Suekrue Hanif
dc.contributor.buuauthorUn, Cem Salih
dc.contributor.departmentFen Edebiyat Fakültesi
dc.contributor.departmentFizik Bölümü
dc.contributor.orcid0000-0002-0595-8803
dc.contributor.researcheridN-3421-2014
dc.contributor.scopusid55325758100
dc.date.accessioned2023-10-06T05:47:22Z
dc.date.available2023-10-06T05:47:22Z
dc.date.issued2015-11-01
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.
dc.description.sponsorshipUnited States Department of Energy (DOE) (DE-SC0013880)
dc.description.sponsorshipRussian Foundation for Basic Research (RFBR) (14-02-00494-a)
dc.description.sponsorshipNational Science Foundation (NSF) (OCI-1053575)
dc.identifier.citationShafi, Q. vd. (2015). "Neutralino dark matter and other LHC predictions from quasi Yukawa unification". Nuclear Physics B, 900, 400-411.
dc.identifier.doi10.1016/j.nuclphysb.2015.09.019
dc.identifier.endpage411
dc.identifier.issn0550-3213
dc.identifier.scopus2-s2.0-84955469655
dc.identifier.startpage400
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.identifier.volume900
dc.identifier.wos000364323000015
dc.indexed.wosSCIE
dc.language.isoen
dc.publisherElsevier
dc.relation.collaborationYurt dışı
dc.relation.collaborationYurt içi
dc.relation.journalNuclear Physics B
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi
dc.relation.tubitakMFAG-114F461
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectLeft-right symmetry
dc.subjectSupersymmetry-breaking
dc.subjectGrand unification
dc.subjectModel
dc.subjectPhysics
dc.subject.scopusHiggs bosons; Supersymmetry; Higgs
dc.subject.wosPhysics, Particles & Fields
dc.titleNeutralino dark matter and other LHC predictions from quasi Yukawa unification
dc.typeArticle
dc.wos.quartileQ2
dspace.entity.typePublication
local.contributor.departmentFen Edebiyat Fakültesi/Fizik Bölümü
local.indexed.atScopus
local.indexed.atWOS

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