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Publicação:
The warped dark sector

dc.contributor.authorBrax, Philippe
dc.contributor.authorFichet, Sylvain [UNESP]
dc.contributor.authorTanedo, Philip
dc.contributor.institutionCNRS
dc.contributor.institutionCalifornia Institute of Technology
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionUniversity of California
dc.date.accessioned2020-12-12T01:41:00Z
dc.date.available2020-12-12T01:41:00Z
dc.date.issued2019-11-10
dc.description.abstractFive-dimensional braneworld constructions in anti-de Sitter space naturally lead to dark sector scenarios in which parts of the dark sector vanish at high 4d momentum or temperature. In the language of modified gravity, such feature implies a new mechanism for hiding light scalars, as well as the possibility of UV-completing chameleon-like effective theories. In the language of dark matter phenomenology, the high-energy behavior of the mediator sector changes dark matter observational complementarity. A multitude of signatures—including exotic ones—are present from laboratory to cosmological scales, including long-range forces with non-integer behavior, periodic signals at colliders, “soft bombs” events well-known from conformal theories, as well as a dark phase transition and a typically small amount of dark radiation.en
dc.description.affiliationInstitut de Physique Théorique Université Paris-Saclay CEA CNRS
dc.description.affiliationWalter Burke Institute for Theoretical Physics California Institute of Technology
dc.description.affiliationICTP-SAIFR & IFT-UNESP, R. Dr. Bento Teobaldo Ferraz 271
dc.description.affiliationDepartment of Physics & Astronomy University of California
dc.description.affiliationUnespICTP-SAIFR & IFT-UNESP, R. Dr. Bento Teobaldo Ferraz 271
dc.description.sponsorshipEuropean Cooperation in Science and Technology
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipHorizon 2020 Framework Programme
dc.description.sponsorshipSeattle Foundation
dc.description.sponsorshipU.S. Department of Energy
dc.description.sponsorshipIdFAPESP: 2011/11973
dc.description.sponsorshipIdFAPESP: 2014/21477-2
dc.description.sponsorshipIdFAPESP: 2018/11721-4
dc.description.sponsorshipIdHorizon 2020 Framework Programme: 690575
dc.description.sponsorshipIdU.S. Department of Energy: DE-SC/0008541
dc.identifierhttp://dx.doi.org/10.1016/j.physletb.2019.135012
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 798.
dc.identifier.doi10.1016/j.physletb.2019.135012
dc.identifier.issn0370-2693
dc.identifier.scopus2-s2.0-85073157252
dc.identifier.urihttp://hdl.handle.net/11449/199479
dc.language.isoeng
dc.relation.ispartofPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
dc.sourceScopus
dc.titleThe warped dark sectoren
dc.typeArtigo
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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