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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 Natl Accelerator Lab
dc.contributor.institutionHarvard Univ
dc.contributor.institutionUniv Maryland
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionUniv Texas Austin
dc.date.accessioned2018-11-26T16:33:00Z
dc.date.available2018-11-26T16:33:00Z
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 Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA
dc.description.affiliationHarvard Univ, Dept Phys, Cambridge, MA 02138 USA
dc.description.affiliationUniv Maryland, Dept Phys, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, SP, Brazil
dc.description.affiliationUniv Texas Austin, Dept Phys, Theory Grp, Austin, TX 78712 USA
dc.description.affiliationUniv Texas Austin, Texas Cosmol Ctr, Austin, TX 78712 USA
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, SP, Brazil
dc.description.sponsorshipUnited States Department of Energy
dc.description.sponsorshipNational Science Foundation (NSF)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipNational Science Foundation
dc.description.sponsorshipNSF
dc.description.sponsorshipIdUnited States Department of Energy: De-AC02-07CH11359
dc.description.sponsorshipIdNational Science Foundation (NSF): PHY-1315155
dc.description.sponsorshipIdFAPESP: 14/05505-6
dc.description.sponsorshipIdFAPESP: 11/21945-8
dc.description.sponsorshipIdNational Science Foundation: PHY-1315983
dc.description.sponsorshipIdNational Science Foundation: PHY-1316033
dc.description.sponsorshipIdNSF: PHY-0855591
dc.description.sponsorshipIdNSF: PHY-1216270
dc.description.sponsorshipIdNSF: PHY-1066293
dc.format.extent10
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.93.103510
dc.identifier.citationPhysical Review D. College Pk: Amer Physical Soc, v. 93, n. 10, 10 p., 2016.
dc.identifier.doi10.1103/PhysRevD.93.103510
dc.identifier.fileWOS000376005900003.pdf
dc.identifier.issn2470-0010
dc.identifier.urihttp://hdl.handle.net/11449/161504
dc.identifier.wosWOS:000376005900003
dc.language.isoeng
dc.publisherAmer Physical Soc
dc.relation.ispartofPhysical Review D
dc.relation.ispartofsjr1,801
dc.rights.accessRightsAcesso aberto
dc.sourceWeb of Science
dc.titleSkew-flavored dark matteren
dc.typeArtigo
dcterms.licensehttp://publish.aps.org/authors/transfer-of-copyright-agreement
dcterms.rightsHolderAmer Physical Soc
dspace.entity.typePublication
unesp.author.orcid0000-0001-9947-0632[1]
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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