Please use this identifier to cite or link to this item: http://hdl.handle.net/11452/34284
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dc.contributor.authorÖzdal, Özer-
dc.date.accessioned2023-10-11T07:54:33Z-
dc.date.available2023-10-11T07:54:33Z-
dc.date.issued2018-03-06-
dc.identifier.citationAltın, Z. vd. (2018). ''Muon g-2 in an alternative quasi-Yukawa unification with a less fine-tuned seesaw mechanism''. Physical Review D., 97(5).en_US
dc.identifier.issn2470-0010-
dc.identifier.issn2470-0029-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.97.055007-
dc.identifier.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.97.055007-
dc.identifier.urihttp://hdl.handle.net/11452/34284-
dc.description.abstractWe explore the low-scale implications of the Pati-Salam Model including the TeV scale right-handed neutrinos interacting and mixing with the MSSM fields through the inverse seesaw (IS) mechanism in light of the ninon anomalous magnetic moment (muon g - 2) resolution and highlight the solutions which are compatible with the quasi-Yukawa unification condition (QYU). We find that the presence of the right-handed neutrinos causes heavy smuons as m((mu) over bar) greater than or similar to 800 GeV in order to avoid tachyonic staus at the low scale. On the other hand, the sneutrinos can be as light as about 100 GeV, and along with the light charginos of mass less than or similar to 400 GeV, they can yield such large contributions to muon g - 2 that the discrepancy between the experiment and the theory can be resolved. These solutions also require m((chi) over bar1)(+/-) less than or similar to 400 GeV and in m((chi) over bar1)(0) less than or similar to 200. We also discuss such light chargino and neutralino along with the light stau (m((tau) over bar) 200 GeV) in the light of current LHC results. Besides, the gluino mass lies in a range similar to[2.5-3.5] TeV, which is tested in near future experiments. In addition, the model predicts relatively light Higgsinos (mu less than or similar to 700 GeV); hence, the second chargino mass is also light enough (less than or similar to 700 GeV) to contribute to muon g - 2. Light Higgsinos also yield less fine-tuning at the electroweak scale, and the regions compatible with muon g - 2 restrict Delta(EW) less than or similar to 100 strictly, and this region also satisfies the QYU condition. In addition, the ratios among the Yukawa couplings should be 1.8 less than or similar to y(t)/y(b) less than or similar to 2.6, y(tau)/y(b) similar to 1.3 to yield correct fermion masses. Even though the righthanded neutrino Yukawa coupling can be varied freely, the solutions bound its range to 0.8 less than or similar to y(tau)/y(b) <= 1.7.en_US
dc.language.isoenen_US
dc.publisherAmer Phyicalen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.rightsAtıf Gayri Ticari Türetilemez 4.0 Uluslararasıtr_TR
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectAstronomy & astrophysicsen_US
dc.subjectPhysicsen_US
dc.subjectTop-quark-massen_US
dc.subjectGrand unificationen_US
dc.subjectInverse seesawen_US
dc.subjectDark-matteren_US
dc.subjectHiggsen_US
dc.subjectModelen_US
dc.subjectPredictionsen_US
dc.subjectExtensionsen_US
dc.subjectBreakingen_US
dc.subjectMomenten_US
dc.titleMuon g-2 in an alternative quasi-Yukawa unification with a less fine-tuned seesaw mechanismen_US
dc.typeArticleen_US
dc.identifier.wos000426749800005tr_TR
dc.identifier.scopus2-s2.0-85044871425tr_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.volume97tr_TR
dc.identifier.issue5tr_TR
dc.relation.journalPhysical Review D.en_US
dc.contributor.buuauthorAltın, Zafer-
dc.contributor.buuauthorÜn, Cem Salih-
dc.contributor.researcheridN-3421-2014tr_TR
dc.relation.collaborationYurt dışıtr_TR
dc.subject.wosAstronomy & astrophysicsen_US
dc.subject.wosPhysics, particles & fieldsen_US
dc.indexed.wosSCIEen_US
dc.indexed.scopusScopusen_US
dc.indexed.pubmedPubMeden_US
dc.wos.quartileQ1 (Astronomy & astrophysics)en_US
dc.wos.quartileQ2 (Physics, particles & fields)en_US
dc.contributor.scopusid57193712940tr_TR
dc.contributor.scopusid55325758100tr_TR
dc.subject.scopusHiggs Bosons; Supersymmetry; Higgsen_US
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