Please use this identifier to cite or link to this item: http://hdl.handle.net/11452/30478
Full metadata record
DC FieldValueLanguage
dc.contributor.authorHebbar, Aditya-
dc.contributor.authorShafi, Qaisar-
dc.date.accessioned2023-01-16T11:54:49Z-
dc.date.available2023-01-16T11:54:49Z-
dc.date.issued2017-06-22-
dc.identifier.citationHebbar, A. vd. (2017). ''Light higgsinos, heavy gluino, and b-tau quasi-yukawa unification: Prospects for finding the gluino at the LHC''. Physical Review D, 95(11).en_US
dc.identifier.issn2470-0010-
dc.identifier.issn2470-0029-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.95.115026-
dc.identifier.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.95.115026-
dc.identifier.urihttp://hdl.handle.net/11452/30478-
dc.description.abstractA wide variety of unified models predict asymptotic relations at M-GUT between the b quark and tau lepton Yukawa couplings. Within the framework of supersymmetric SU(4) x SU(2)(L) x SU(2)(R), we explore regions of the parameter space that are compatible with b-tau quasi Yukawa Unification, Higgsinos being the lightest supersymmetric particles (less than or similar to 1 TeV) accompanied by a relatively low level of fine-tuning determined by the parameter Delta(EW)(less than or similar to 200). Among the colored sparticles, the stop weighs more than 1.5 TeV or so, whereas the squarks of the first two families are significantly heavier, approaching 10 TeV in some cases. The gluino mass is estimated to lie in the 2-4 TeV range which raises the important question: Will the LHC find the gluino?en_US
dc.description.sponsorshipUnited States Department of Energy (DOE) - DE-SC0013880en_US
dc.description.sponsorshipNational Science Foundation (NSF) - OCI-1053575en_US
dc.language.isoenen_US
dc.publisherAmer Phyicalen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectAstronomy & astrophysicsen_US
dc.subjectPhysicsen_US
dc.subjectTop-quark-massen_US
dc.subjectSupersymmetry-breakingen_US
dc.subjectSusyen_US
dc.subjectPredictionsen_US
dc.subjectMatteren_US
dc.subjectModelen_US
dc.subjectGaugeen_US
dc.titleLight higgsinos, heavy gluino, and b-tau quasi-yukawa unification: Prospects for finding the gluino at the LHCen_US
dc.typeArticleen_US
dc.identifier.wos000404023800005tr_TR
dc.identifier.scopus2-s2.0-85022344312tr_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.volume95tr_TR
dc.identifier.issue11tr_TR
dc.relation.journalPhysical Review Den_US
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.wos.quartileQ1en_US
dc.contributor.scopusid55325758100tr_TR
dc.subject.scopusHiggs Bosons; Supersymmetry; Higgsen_US
Appears in Collections:Scopus
Web of Science

Files in This Item:
There are no files associated with this item.


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.