Charged higgs boson in MSSM and beyond

dc.contributor.authorHıçyılmaz, Yaşar
dc.contributor.authorSelbuz, Levent
dc.contributor.authorSolmaz, Levent
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.accessioned2023-11-09T12:00:44Z
dc.date.available2023-11-09T12:00:44Z
dc.date.issued2018-06-27
dc.description.abstractWe conduct a numerical study over the constrained MSSM (CMSSM), next-to-MSSM (NMSSM) and U(1) extended MSSM (UMSSM) to probe the allowed mass ranges of the charged Higgs boson and its dominant decay patterns, which might come into prominence in the near future collider experiments. We present results obtained from a limited scan for CMSSM as a basis and compare its predictions with the extended models. We observe within our data that a wide mass range is allowed as 0.5(1) less than or similar to m(H)(+/-) less than or similar to 17 TeV in UMSSM (NMSSM). We find that the dominant decay channel is mostly (H-+/- -> tb) such that BR(H-+/- -> tb) similar to 80%. While this mode remains dominant over the whole allowed parameter space of CMSSM, we realize some special domains in the NMSSM and UMSSM, in which BR(H-+/- -> tb) less than or similar to 10%. In this context, the decay patterns of the charged Higgs can play a significant role to distinguish among the SUSY models. In addition to the tb decay mode, we find that the narrow mass scale in CMSSM allows only the decay modes for the charged Higgs boson to tau nu (similar to 16%), and their supersymmetric partners (tau) over tilde(nu) over tilde (similar to 13%). On the other hand, it is possible to realize the mode in NMSSM and UMSSM in which the charged Higgs boson decays into a chargino and neutralino pair up to about 25%. This decay mode requires nonuniversal boundary conditions within the MSSM framework to be available, since CMSSM yields BR(H-+/- -> (chi) over tilde (1)(0)<(chi(+/-)(1))over tilde>) less than or similar to. 1%. It can also be probed in the near future collider experiments through the missing energy and CP-violation measurements. Moreover, the chargino mass is realized as m((chi) over tilde1)(+/-) TeV in NMSSM and UMSSM, and these solutions will be likely tested soon in collider experiments through the chargino-neutralino production. Focusing on the chargino-neutralino decay patterns, we also present tables which list the possible ranges for the charged Higgs production and decay modes.en_US
dc.description.sponsorshipBalıkesir Üniversitesi - BAP-2017/142 - BAP-2017/174tr_TR
dc.description.sponsorshipAnkara Üniversitesi - 17B0443004tr_TR
dc.identifier.citationÜn, C. S. vd. (2018). ''Charged higgs boson in MSSM and beyond''. Physical Review D., 97(11).en_US
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.issue11tr_TR
dc.identifier.scopus2-s2.0-85049726103tr_TR
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.97.115041
dc.identifier.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.97.115041
dc.identifier.urihttp://hdl.handle.net/11452/34827
dc.identifier.volume97tr_TR
dc.identifier.wos000436558600001
dc.indexed.scopusScopusen_US
dc.indexed.wosSCIEen_US
dc.language.isoenen_US
dc.publisherAmer Phyical Socen_US
dc.relation.collaborationYurt içitr_TR
dc.relation.journalPhysical Review D.en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergitr_TR
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectAstronomy & astrophysicsen_US
dc.subjectPhysicsen_US
dc.subjectStandard modelen_US
dc.subjectRoot-s=13 teven_US
dc.subjectSearchen_US
dc.subjectSupersymmetryen_US
dc.subjectSusyen_US
dc.subjectPhenomenologyen_US
dc.subjectAssociationen_US
dc.subjectExtensionen_US
dc.subjectLighten_US
dc.subjectDecayen_US
dc.subject.scopusHiggs Bosons; Supersymmetry; Higgsen_US
dc.subject.wosAstronomy & astrophysicsen_US
dc.subject.wosPhysics, particles & fieldsen_US
dc.titleCharged higgs boson in MSSM and beyonden_US
dc.typeArticle
dc.wos.quartileQ1 (Astronomy & astrophysics)en_US
dc.wos.quartileQ2 (Physics, particles & fields)en_US

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