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Model characterization and dark matter in the secluded U(1)' model

dc.contributor.authorHiçyilmaz, Yaşar
dc.contributor.authorSelbuz, Levent
dc.contributor.authorSolmaz, Levent
dc.contributor.buuauthorÜn, Cem Salih
dc.contributor.buuauthorÜN, CEM SALİH
dc.contributor.departmentFen Edebiyat Fakültesi
dc.contributor.departmentFizik Ana Bilim Dalı
dc.contributor.orcid0000-0002-0595-8803
dc.contributor.researcheridN-3421-2014
dc.date.accessioned2024-11-25T06:07:03Z
dc.date.available2024-11-25T06:07:03Z
dc.date.issued2022-03-29
dc.description.abstractWe consider a class of U(1)'-extended minimal supersymmetric extension of the Standard Model (MSSM) in which the U(1)' symmetry is broken by vacuum expectation values of four MSSM singlet fields. While one MSSM singlet field interacts with the MSSM Higgs fields, three of them interact only with each other in forming a secluded sector. Assigning universal U(1)' charges for three families, the anomaly cancellation condition requires exotic fields which are assumed to be heavy and decoupled. We discuss a variety of U(1)' charge assignments and anomaly cancellation, Z'/Z hierarchy, neutralinos, charginos and the Higgs sector. We find that the typical spectra involve two CP-odd Higgs bosons lighter than about 200 GeV and 600 GeV respectively, which are mostly formed by the MSSM singlet fields. If the relic density of dark matter is saturated only by a neutralino, compatible solutions predict LSP neutralinos formed by the MSSM singlet fields in the mass scales below about 600 GeV, while it is possible to realize MSSM neutralino LSP above these mass scales. One can classify the implications in three scenarios. Scenario I involves NLSP charginos, while Scenario II involves charginos which do not participate coannihilation processes with the LSP neutralino. These two scenarios predict MSSM singlet LSP neutralinos, while Scenario I leads to larger scattering cross sections of dark matter. Scenario III has the solutions in which the MSSM neutralinos are considerably involved in LSP decomposition which yields very large scattering cross section excluded by the direct detection experiments.
dc.description.sponsorshipBalikesir Üniversitesi BAP-2017/198
dc.description.sponsorshipMinistry of Science and Innovation, Spain (MICINN) Spanish Government PID2019-107844 GB-C22
dc.identifier.doi10.1103/PhysRevD.105.055029
dc.identifier.issn2470-0010
dc.identifier.issue5
dc.identifier.scopus2-s2.0-85128278485
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.105.055029
dc.identifier.urihttps://hdl.handle.net/11452/48398
dc.identifier.volume105
dc.identifier.wos000783936600002
dc.indexed.wosWOS.SCI
dc.language.isoen
dc.publisherAmer Physical Soc
dc.relation.journalPhysical Review D
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi
dc.relation.tubitakTUBITAK
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectSymmetry-breaking
dc.subjectBoson mass
dc.subjectGauge
dc.subjectUnification
dc.subjectDynamics
dc.subjectSpheno
dc.subjectFlavor
dc.subjectE6
dc.subjectScience & technology
dc.subjectPhysical sciences
dc.subjectPhysics, particles & fields
dc.subjectAstronomy & astrophysics
dc.subjectPhysics
dc.titleModel characterization and dark matter in the secluded U(1)' model
dc.typeArticle
dspace.entity.typePublication
local.contributor.departmentFen Edebiyat Fakültesi/Fizik Ana Bilim Dalı
local.indexed.atWOS
local.indexed.atScopus
relation.isAuthorOfPublication0c6ad07c-f6f6-4949-a2f0-e288af6b9411
relation.isAuthorOfPublication.latestForDiscovery0c6ad07c-f6f6-4949-a2f0-e288af6b9411

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