Skew-flavored dark matter

Detalhes bibliográficos
Autor(a) principal: Agrawal, Prateek
Data de Publicação: 2016
Outros Autores: Chacko, Zackaria, Fortes, Elaine C. F. S. [UNESP], Kilic, Can
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.93.103510
http://hdl.handle.net/11449/228148
Resumo: We explore a novel flavor structure in the interactions of dark matter with the Standard Model. We consider theories in which both the dark matter candidate, and the particles that mediate its interactions with the Standard Model fields, carry flavor quantum numbers. The interactions are skewed in flavor space, so that a dark matter particle does not directly couple to the Standard Model matter fields of the same flavor, but only to the other two flavors. This framework respects minimal flavor violation and is, therefore, naturally consistent with flavor constraints. We study the phenomenology of a benchmark model in which dark matter couples to right-handed charged leptons. In large regions of parameter space, the dark matter can emerge as a thermal relic, while remaining consistent with the constraints from direct and indirect detection. The collider signatures of this scenario include events with multiple leptons and missing energy. These events exhibit a characteristic flavor pattern that may allow this class of models to be distinguished from other theories of dark matter.
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spelling Skew-flavored dark matterWe explore a novel flavor structure in the interactions of dark matter with the Standard Model. We consider theories in which both the dark matter candidate, and the particles that mediate its interactions with the Standard Model fields, carry flavor quantum numbers. The interactions are skewed in flavor space, so that a dark matter particle does not directly couple to the Standard Model matter fields of the same flavor, but only to the other two flavors. This framework respects minimal flavor violation and is, therefore, naturally consistent with flavor constraints. We study the phenomenology of a benchmark model in which dark matter couples to right-handed charged leptons. In large regions of parameter space, the dark matter can emerge as a thermal relic, while remaining consistent with the constraints from direct and indirect detection. The collider signatures of this scenario include events with multiple leptons and missing energy. These events exhibit a characteristic flavor pattern that may allow this class of models to be distinguished from other theories of dark matter.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)National Aeronautics and Space AdministrationNational Science FoundationFermilab, P.O. Box 500Department of Physics Harvard UniversityMaryland Center for Fundamental Physics Department of Physics University of MarylandInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271Theory Group Department of Physics Texas Cosmology Center University of Texas at AustinInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271FAPESP: 11/21945-8FAPESP: 14/05505-6National Science Foundation: PHY-0855591National Science Foundation: PHY-1066293National Science Foundation: PHY-1216270National Science Foundation: PHY-1315155National Science Foundation: PHY-1315983National Science Foundation: PHY-1316033FermilabHarvard UniversityUniversity of MarylandUniversidade Estadual Paulista (UNESP)University of Texas at AustinAgrawal, PrateekChacko, ZackariaFortes, Elaine C. F. S. [UNESP]Kilic, Can2022-04-29T07:35:48Z2022-04-29T07:35:48Z2016-05-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.93.103510Physical Review D, v. 93, n. 10, 2016.2470-00292470-0010http://hdl.handle.net/11449/22814810.1103/PhysRevD.93.1035102-s2.0-84966440664Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T07:35:48Zoai:repositorio.unesp.br:11449/228148Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-29T07:35:48Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Skew-flavored dark matter
title Skew-flavored dark matter
spellingShingle Skew-flavored dark matter
Agrawal, Prateek
title_short Skew-flavored dark matter
title_full Skew-flavored dark matter
title_fullStr Skew-flavored dark matter
title_full_unstemmed Skew-flavored dark matter
title_sort Skew-flavored dark matter
author Agrawal, Prateek
author_facet Agrawal, Prateek
Chacko, Zackaria
Fortes, Elaine C. F. S. [UNESP]
Kilic, Can
author_role author
author2 Chacko, Zackaria
Fortes, Elaine C. F. S. [UNESP]
Kilic, Can
author2_role author
author
author
dc.contributor.none.fl_str_mv Fermilab
Harvard University
University of Maryland
Universidade Estadual Paulista (UNESP)
University of Texas at Austin
dc.contributor.author.fl_str_mv Agrawal, Prateek
Chacko, Zackaria
Fortes, Elaine C. F. S. [UNESP]
Kilic, Can
description We explore a novel flavor structure in the interactions of dark matter with the Standard Model. We consider theories in which both the dark matter candidate, and the particles that mediate its interactions with the Standard Model fields, carry flavor quantum numbers. The interactions are skewed in flavor space, so that a dark matter particle does not directly couple to the Standard Model matter fields of the same flavor, but only to the other two flavors. This framework respects minimal flavor violation and is, therefore, naturally consistent with flavor constraints. We study the phenomenology of a benchmark model in which dark matter couples to right-handed charged leptons. In large regions of parameter space, the dark matter can emerge as a thermal relic, while remaining consistent with the constraints from direct and indirect detection. The collider signatures of this scenario include events with multiple leptons and missing energy. These events exhibit a characteristic flavor pattern that may allow this class of models to be distinguished from other theories of dark matter.
publishDate 2016
dc.date.none.fl_str_mv 2016-05-10
2022-04-29T07:35:48Z
2022-04-29T07:35:48Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.93.103510
Physical Review D, v. 93, n. 10, 2016.
2470-0029
2470-0010
http://hdl.handle.net/11449/228148
10.1103/PhysRevD.93.103510
2-s2.0-84966440664
url http://dx.doi.org/10.1103/PhysRevD.93.103510
http://hdl.handle.net/11449/228148
identifier_str_mv Physical Review D, v. 93, n. 10, 2016.
2470-0029
2470-0010
10.1103/PhysRevD.93.103510
2-s2.0-84966440664
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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