Light stops and fine-tuning in MSSM

dc.contributor.buuauthorCici, Ali
dc.contributor.buuauthorKırca, Zerrin
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.orcid0000-0001-5217-9290tr_TR
dc.contributor.researcheridAAH-8661-2021tr_TR
dc.contributor.researcheridN-3421-2014tr_TR
dc.contributor.scopusid57193713979tr_TR
dc.contributor.scopusid6508185203tr_TR
dc.contributor.scopusid55325758100tr_TR
dc.date.accessioned2023-10-04T08:34:05Z
dc.date.available2023-10-04T08:34:05Z
dc.date.issued2018-01-13
dc.description.abstractWe discuss the fine-tuning issue within the MSSM framework. Following the idea that the fine-tuning can measure effects of some missing mechanism, we impose non-universal gaugino masses at the GUT scale, and explore the low scale implications. We realize that the fine-tuning parametrized with Δ EW can be as low as zero. We consider the stop mass with a special importance and focus on the mass scales as mt~≤ 700 GeV, which are excluded by the current experiments when the stop decays into a neutralino along with a top quark or a chargino along with a bottom quark. We find that the stop mass can be as low as about 250 GeV with Δ EW∼ 50. We find that the solutions in this region can be exluded only up to 60 % when stop decays into a neutralino-top quark, and 50 % when it decays into a chargino-b quark. Setting 65 % CL to be potential exclusion and 95 % to be pure exclusion limit such solutions will be tested in near future experiments, which are conducted with higher luminosity. In addition to stop, the region with low fine-tuning and light stops predicts masses for the other supersymmetric particles such as mb~≳ 700 GeV, mτ~≳ 1 TeV, mχ~1±≳120 GeV. The details for the mass scales and decay rates are also provided by tables of benchmark points.en_US
dc.identifier.citationCici, A. vd. (2018). ''Light stops and fine-tuning in MSSM''. European Physical Journal C., 78(1).en_US
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.issue1tr_TR
dc.identifier.scopus2-s2.0-85041025557tr_TR
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-018-5549-y
dc.identifier.urihttps://link.springer.com/article/10.1140/epjc/s10052-018-5549-y
dc.identifier.urihttp://hdl.handle.net/11452/34196
dc.identifier.volume78tr_TR
dc.identifier.wos000423203200004
dc.indexed.scopusScopusen_US
dc.indexed.wosSCIEen_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.journalEuropean Physical Journal C.en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergitr_TR
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectPhysicsen_US
dc.subjectGev higgsen_US
dc.subjectL. modelen_US
dc.subjectSusy B.en_US
dc.subjectBreakingen_US
dc.subjectSphenoen_US
dc.subject.scopusHiggs Bosons; Supersymmetry; Higgsen_US
dc.subject.wosPhysics, particles & fieldsen_US
dc.titleLight stops and fine-tuning in MSSMen_US
dc.typeArticle
dc.wos.quartileQ1en_US

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