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Publicação:
Skew-flavored dark matter

dc.contributor.authorAgrawal, Prateek
dc.contributor.authorChacko, Zackaria
dc.contributor.authorFortes, Elaine C. F. S. [UNESP]
dc.contributor.authorKilic, Can
dc.contributor.institutionFermilab
dc.contributor.institutionHarvard University
dc.contributor.institutionUniversity of Maryland
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionUniversity of Texas at Austin
dc.date.accessioned2022-04-29T07:35:48Z
dc.date.available2022-04-29T07:35:48Z
dc.date.issued2016-05-10
dc.description.abstractWe 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.en
dc.description.affiliationFermilab, P.O. Box 500
dc.description.affiliationDepartment of Physics Harvard University
dc.description.affiliationMaryland Center for Fundamental Physics Department of Physics University of Maryland
dc.description.affiliationInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271
dc.description.affiliationTheory Group Department of Physics Texas Cosmology Center University of Texas at Austin
dc.description.affiliationUnespInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipNational Aeronautics and Space Administration
dc.description.sponsorshipNational Science Foundation
dc.description.sponsorshipIdFAPESP: 11/21945-8
dc.description.sponsorshipIdFAPESP: 14/05505-6
dc.description.sponsorshipIdNational Science Foundation: PHY-0855591
dc.description.sponsorshipIdNational Science Foundation: PHY-1066293
dc.description.sponsorshipIdNational Science Foundation: PHY-1216270
dc.description.sponsorshipIdNational Science Foundation: PHY-1315155
dc.description.sponsorshipIdNational Science Foundation: PHY-1315983
dc.description.sponsorshipIdNational Science Foundation: PHY-1316033
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.93.103510
dc.identifier.citationPhysical Review D, v. 93, n. 10, 2016.
dc.identifier.doi10.1103/PhysRevD.93.103510
dc.identifier.issn2470-0029
dc.identifier.issn2470-0010
dc.identifier.scopus2-s2.0-84966440664
dc.identifier.urihttp://hdl.handle.net/11449/228148
dc.language.isoeng
dc.relation.ispartofPhysical Review D
dc.sourceScopus
dc.titleSkew-flavored dark matteren
dc.typeArtigo
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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