Publicação: Skew-flavored dark matter
dc.contributor.author | Agrawal, Prateek | |
dc.contributor.author | Chacko, Zackaria | |
dc.contributor.author | Fortes, Elaine C. F. S. [UNESP] | |
dc.contributor.author | Kilic, Can | |
dc.contributor.institution | Fermilab | |
dc.contributor.institution | Harvard University | |
dc.contributor.institution | University of Maryland | |
dc.contributor.institution | Universidade Estadual Paulista (UNESP) | |
dc.contributor.institution | University of Texas at Austin | |
dc.date.accessioned | 2022-04-29T07:35:48Z | |
dc.date.available | 2022-04-29T07:35:48Z | |
dc.date.issued | 2016-05-10 | |
dc.description.abstract | 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. | en |
dc.description.affiliation | Fermilab, P.O. Box 500 | |
dc.description.affiliation | Department of Physics Harvard University | |
dc.description.affiliation | Maryland Center for Fundamental Physics Department of Physics University of Maryland | |
dc.description.affiliation | Instituto de Fisica Teorica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271 | |
dc.description.affiliation | Theory Group Department of Physics Texas Cosmology Center University of Texas at Austin | |
dc.description.affiliationUnesp | Instituto de Fisica Teorica Universidade Estadual Paulista, Rua Dr. Bento Teobaldo Ferraz 271 | |
dc.description.sponsorship | Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) | |
dc.description.sponsorship | National Aeronautics and Space Administration | |
dc.description.sponsorship | National Science Foundation | |
dc.description.sponsorshipId | FAPESP: 11/21945-8 | |
dc.description.sponsorshipId | FAPESP: 14/05505-6 | |
dc.description.sponsorshipId | National Science Foundation: PHY-0855591 | |
dc.description.sponsorshipId | National Science Foundation: PHY-1066293 | |
dc.description.sponsorshipId | National Science Foundation: PHY-1216270 | |
dc.description.sponsorshipId | National Science Foundation: PHY-1315155 | |
dc.description.sponsorshipId | National Science Foundation: PHY-1315983 | |
dc.description.sponsorshipId | National Science Foundation: PHY-1316033 | |
dc.identifier | http://dx.doi.org/10.1103/PhysRevD.93.103510 | |
dc.identifier.citation | Physical Review D, v. 93, n. 10, 2016. | |
dc.identifier.doi | 10.1103/PhysRevD.93.103510 | |
dc.identifier.issn | 2470-0029 | |
dc.identifier.issn | 2470-0010 | |
dc.identifier.scopus | 2-s2.0-84966440664 | |
dc.identifier.uri | http://hdl.handle.net/11449/228148 | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review D | |
dc.source | Scopus | |
dc.title | Skew-flavored dark matter | en |
dc.type | Artigo | |
dspace.entity.type | Publication | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |