Simply split strongly interacting massive particles

Detalhes bibliográficos
Autor(a) principal: Bernal, Nicolás [UNESP]
Data de Publicação: 2017
Outros Autores: Chu, Xiaoyong, Pradler, Josef
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.
id UNSP_9d08df74899a8d57b280d67039db2605
oai_identifier_str oai:repositorio.unesp.br:11449/228359
network_acronym_str UNSP
network_name_str Repositório Institucional da UNESP
repository_id_str 2946
spelling 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