Simply split strongly interacting massive particles
Autor(a) principal: | |
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Data de Publicação: | 2017 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.95.115023 http://hdl.handle.net/11449/228359 |
Resumo: | Dark matter which interacts strongly with itself, but only feebly with the Standard Model, is a possibility that has been entertained to solve apparent small-scale structure problems that are pertinent to the noninteracting cold dark matter paradigm. In this paper, we study the simple case in which the self-scattering rate today is regulated by kinematics and/or the abundance ratio, through the mass splitting of nearly degenerate pseudo-Dirac fermions χ1 and χ2 or real scalars φ1 and φ2. We calculate the relic density of these states in a scenario where self-scattering proceeds through off-diagonal couplings with a vector particle V (dark photon) and where the abundance is set through number-depleting 4-to-2 reactions in the hidden sector, or, alternatively, via freeze-in. We study the implications of the considered models and their prospect of solving astrophysical small-scale structure problems. We also show how the introduction of the (meta)stable heavier state may be probed in future dark matter searches. |
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Simply split strongly interacting massive particlesDark matter which interacts strongly with itself, but only feebly with the Standard Model, is a possibility that has been entertained to solve apparent small-scale structure problems that are pertinent to the noninteracting cold dark matter paradigm. In this paper, we study the simple case in which the self-scattering rate today is regulated by kinematics and/or the abundance ratio, through the mass splitting of nearly degenerate pseudo-Dirac fermions χ1 and χ2 or real scalars φ1 and φ2. We calculate the relic density of these states in a scenario where self-scattering proceeds through off-diagonal couplings with a vector particle V (dark photon) and where the abundance is set through number-depleting 4-to-2 reactions in the hidden sector, or, alternatively, via freeze-in. We study the implications of the considered models and their prospect of solving astrophysical small-scale structure problems. We also show how the introduction of the (meta)stable heavier state may be probed in future dark matter searches.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Ministerio de Economía y CompetitividadAustrian Academy of SciencesCentro de Investigaciones Universidad Antonio Nariño, Cra 3 Este # 47A-15ICTP South American Institute of Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271Institute of High Energy Physics Austrian Academy of Sciences, Nikolsdorfer Gasse 18ICTP South American Institute of Fundamental Research Instituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271FAPESP: 2011/11973-4FAPESP: 2013/01792-8Ministerio de Economía y Competitividad: FPA2014-54459-PUniversidad Antonio NariñoUniversidade Estadual Paulista (UNESP)Austrian Academy of SciencesBernal, Nicolás [UNESP]Chu, XiaoyongPradler, Josef2022-04-29T08:09:41Z2022-04-29T08:09:41Z2017-06-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.95.115023Physical Review D, v. 95, n. 11, 2017.2470-00292470-0010http://hdl.handle.net/11449/22835910.1103/PhysRevD.95.1150232-s2.0-85022342015Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T08:09:41Zoai:repositorio.unesp.br:11449/228359Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T17:03:19.140558Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Simply split strongly interacting massive particles |
title |
Simply split strongly interacting massive particles |
spellingShingle |
Simply split strongly interacting massive particles Bernal, Nicolás [UNESP] |
title_short |
Simply split strongly interacting massive particles |
title_full |
Simply split strongly interacting massive particles |
title_fullStr |
Simply split strongly interacting massive particles |
title_full_unstemmed |
Simply split strongly interacting massive particles |
title_sort |
Simply split strongly interacting massive particles |
author |
Bernal, Nicolás [UNESP] |
author_facet |
Bernal, Nicolás [UNESP] Chu, Xiaoyong Pradler, Josef |
author_role |
author |
author2 |
Chu, Xiaoyong Pradler, Josef |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
Universidad Antonio Nariño Universidade Estadual Paulista (UNESP) Austrian Academy of Sciences |
dc.contributor.author.fl_str_mv |
Bernal, Nicolás [UNESP] Chu, Xiaoyong Pradler, Josef |
description |
Dark matter which interacts strongly with itself, but only feebly with the Standard Model, is a possibility that has been entertained to solve apparent small-scale structure problems that are pertinent to the noninteracting cold dark matter paradigm. In this paper, we study the simple case in which the self-scattering rate today is regulated by kinematics and/or the abundance ratio, through the mass splitting of nearly degenerate pseudo-Dirac fermions χ1 and χ2 or real scalars φ1 and φ2. We calculate the relic density of these states in a scenario where self-scattering proceeds through off-diagonal couplings with a vector particle V (dark photon) and where the abundance is set through number-depleting 4-to-2 reactions in the hidden sector, or, alternatively, via freeze-in. We study the implications of the considered models and their prospect of solving astrophysical small-scale structure problems. We also show how the introduction of the (meta)stable heavier state may be probed in future dark matter searches. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-06-01 2022-04-29T08:09:41Z 2022-04-29T08:09:41Z |
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/10.1103/PhysRevD.95.115023 Physical Review D, v. 95, n. 11, 2017. 2470-0029 2470-0010 http://hdl.handle.net/11449/228359 10.1103/PhysRevD.95.115023 2-s2.0-85022342015 |
url |
http://dx.doi.org/10.1103/PhysRevD.95.115023 http://hdl.handle.net/11449/228359 |
identifier_str_mv |
Physical Review D, v. 95, n. 11, 2017. 2470-0029 2470-0010 10.1103/PhysRevD.95.115023 2-s2.0-85022342015 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D |
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_ |
1808128746681532416 |