Muon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSM

dc.contributor.authorBabu, Kaladi S.
dc.contributor.authorGogoladze, Ilia G.
dc.contributor.authorShafi, Qaisar
dc.contributor.buuauthorÜn, Cem Salih
dc.contributor.departmentUludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü.tr_TR
dc.contributor.orcid0000-0002-0595-8803tr_TR
dc.contributor.researcheridN-3421-2014tr_TR
dc.contributor.scopusid55325758100tr_TR
dc.date.accessioned2022-09-08T08:15:27Z
dc.date.available2022-09-08T08:15:27Z
dc.date.issued2014-12-16
dc.description.abstractWe discuss the sparticle (and Higgs) spectrum in a class of flavor symmetry-based minimal super-symmetric standard models, referred to here as sMSSM. In this framework the supersymmetry breaking Lagrangian takes the most general form consistent with a grand unified symmetry such as SO(10) and a non-Abelian flavor symmetry acting on the three families with either a 2+1 or a 3 family assignment. Models based on gauged SU(2) and SO(3) flavor symmetry, as well as non-Abelian discrete symmetries such as S-3 and A(4), have been suggested which fall into this category. These models describe supersymmetry breaking in terms of seven phenomenological parameters. The soft supersymmetry breaking masses at M-GUT of all sfermions of the first two families are equal in sMSSM, which differ in general from the corresponding third family mass. In such a framework we show that the muon g - 2 anomaly, the observed Higgs boson mass of similar to 125 GeV, and the observed relic neutralino dark matter abundance can be simultaneously accommodated. The resolution of the muon g - 2 anomaly in particular yields the result that the first two generation squark masses, as well the gluino mass, should be less than or similar to 2 TeV, which will be tested at LHC14.en_US
dc.description.sponsorshipUnited States Department of Energy (DOE) (de-sc0010108) (DE-FG02-91ER40626)en_US
dc.description.sponsorshipNational Science Foundation (NSF) (OCI-1053575)en_US
dc.description.sponsorshipRustaveli National Science Foundation (31/98)en_US
dc.description.sponsorshipUnited States Department of Energy (DOE) (de-sc0010137)en_US
dc.description.sponsorshipNational Science Foundation (NSF) (PHY-1342611)en_US
dc.identifier.citationBabu, K. S. vd. (2014). "Muon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSM". Physical Review D , 90(11).en_US
dc.identifier.issn1550-7998
dc.identifier.issn1550-2368
dc.identifier.issue11tr_TR
dc.identifier.scopus2-s2.0-84918767610tr_TR
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.90.116002
dc.identifier.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.90.116002
dc.identifier.urihttp://hdl.handle.net/11452/28554
dc.identifier.volume90tr_TR
dc.identifier.wos000348730800012
dc.indexed.scopusScopusen_US
dc.indexed.wosSCIEen_US
dc.language.isoenen_US
dc.publisherAmer Physicalen_US
dc.relation.collaborationYurt dışıtr_TR
dc.relation.journalPhysical Review Den_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergitr_TR
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectFamily symmetryen_US
dc.subjectUnified theoriesen_US
dc.subjectFermion massesen_US
dc.subjectBreakingen_US
dc.subjectSupersymmetryen_US
dc.subjectPredictionsen_US
dc.subjectUnificationen_US
dc.subjectModelsen_US
dc.subjectMinimaen_US
dc.subjectAstronomy & astrophysicsen_US
dc.subjectPhysicsen_US
dc.subject.scopusHiggs Bosons; Supersymmetry; Higgsen_US
dc.subject.wosAstronomy & astrophysicsen_US
dc.subject.wosPhysics, particles & fieldsen_US
dc.titleMuon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSMen_US
dc.typeArticle
dc.wos.quartileQ1en_US

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