The warped dark sector
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1016/j.physletb.2019.135012 http://hdl.handle.net/11449/199479 |
Resumo: | Five-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. |
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Repositório Institucional da UNESP |
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The warped dark sectorFive-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.European Cooperation in Science and TechnologyFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Horizon 2020 Framework ProgrammeSeattle FoundationU.S. Department of EnergyInstitut de Physique Théorique Université Paris-Saclay CEA CNRSWalter Burke Institute for Theoretical Physics California Institute of TechnologyICTP-SAIFR & IFT-UNESP, R. Dr. Bento Teobaldo Ferraz 271Department of Physics & Astronomy University of CaliforniaICTP-SAIFR & IFT-UNESP, R. Dr. Bento Teobaldo Ferraz 271FAPESP: 2011/11973FAPESP: 2014/21477-2FAPESP: 2018/11721-4Horizon 2020 Framework Programme: 690575U.S. Department of Energy: DE-SC/0008541CNRSCalifornia Institute of TechnologyUniversidade Estadual Paulista (Unesp)University of CaliforniaBrax, PhilippeFichet, Sylvain [UNESP]Tanedo, Philip2020-12-12T01:41:00Z2020-12-12T01:41:00Z2019-11-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1016/j.physletb.2019.135012Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 798.0370-2693http://hdl.handle.net/11449/19947910.1016/j.physletb.2019.1350122-s2.0-85073157252Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physicsinfo:eu-repo/semantics/openAccess2021-10-23T07:21:23Zoai:repositorio.unesp.br:11449/199479Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:35:49.180987Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
The warped dark sector |
title |
The warped dark sector |
spellingShingle |
The warped dark sector Brax, Philippe |
title_short |
The warped dark sector |
title_full |
The warped dark sector |
title_fullStr |
The warped dark sector |
title_full_unstemmed |
The warped dark sector |
title_sort |
The warped dark sector |
author |
Brax, Philippe |
author_facet |
Brax, Philippe Fichet, Sylvain [UNESP] Tanedo, Philip |
author_role |
author |
author2 |
Fichet, Sylvain [UNESP] Tanedo, Philip |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
CNRS California Institute of Technology Universidade Estadual Paulista (Unesp) University of California |
dc.contributor.author.fl_str_mv |
Brax, Philippe Fichet, Sylvain [UNESP] Tanedo, Philip |
description |
Five-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. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-11-10 2020-12-12T01:41:00Z 2020-12-12T01:41:00Z |
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/10.1016/j.physletb.2019.135012 Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 798. 0370-2693 http://hdl.handle.net/11449/199479 10.1016/j.physletb.2019.135012 2-s2.0-85073157252 |
url |
http://dx.doi.org/10.1016/j.physletb.2019.135012 http://hdl.handle.net/11449/199479 |
identifier_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 798. 0370-2693 10.1016/j.physletb.2019.135012 2-s2.0-85073157252 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
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) |
repository.mail.fl_str_mv |
|
_version_ |
1808128385504772096 |