Simply split strongly interacting massive particles

Detalhes bibliográficos
Autor(a) principal: Bernal, Nicolas [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/11449/162904
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 chi(1) and chi(2) or real scalars phi(1) and phi(2). 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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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 chi(1) and chi(2) or real scalars phi(1) and phi(2). 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)Spanish MINECOAustrian Academy of SciencesEuropean Union's Horizon research and innovation programUniv Antonio Narino, Ctr Invest, Cra 3 Este 47A-15, Bogota, ColombiaUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, R Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, BrazilAustrian Acad Sci, Inst High Energy Phys, Nikolsdorfer Gasse 18, A-1050 Vienna, AustriaUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, R Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, BrazilFAPESP: 2011/11973-4FAPESP: 2013/01792-8Spanish MINECO: FPA2014-54459-PEuropean Union's Horizon research and innovation program: 674896European Union's Horizon research and innovation program: 690575Amer Physical SocUniv Antonio NarinoUniversidade Estadual Paulista (Unesp)Austrian Acad SciBernal, Nicolas [UNESP]Chu, XiaoyongPradler, Josef2018-11-26T17:34:54Z2018-11-26T17:34:54Z2017-06-20info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article17application/pdfhttp://dx.doi.org/10.1103/PhysRevD.95.115023Physical Review D. College Pk: Amer Physical Soc, v. 95, n. 11, 17 p., 2017.2470-0010http://hdl.handle.net/11449/16290410.1103/PhysRevD.95.115023WOS:000404023000004WOS000404023000004.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,801info:eu-repo/semantics/openAccess2024-01-09T06:28:20Zoai:repositorio.unesp.br:11449/162904Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:32:52.543479Repositório 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, Nicolas [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, Nicolas [UNESP]
author_facet Bernal, Nicolas [UNESP]
Chu, Xiaoyong
Pradler, Josef
author_role author
author2 Chu, Xiaoyong
Pradler, Josef
author2_role author
author
dc.contributor.none.fl_str_mv Univ Antonio Narino
Universidade Estadual Paulista (Unesp)
Austrian Acad Sci
dc.contributor.author.fl_str_mv Bernal, Nicolas [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 chi(1) and chi(2) or real scalars phi(1) and phi(2). 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 2017-06-20
2018-11-26T17:34:54Z
2018-11-26T17:34:54Z
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. College Pk: Amer Physical Soc, v. 95, n. 11, 17 p., 2017.
2470-0010
http://hdl.handle.net/11449/162904
10.1103/PhysRevD.95.115023
WOS:000404023000004
WOS000404023000004.pdf
url http://dx.doi.org/10.1103/PhysRevD.95.115023
http://hdl.handle.net/11449/162904
identifier_str_mv Physical Review D. College Pk: Amer Physical Soc, v. 95, n. 11, 17 p., 2017.
2470-0010
10.1103/PhysRevD.95.115023
WOS:000404023000004
WOS000404023000004.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
1,801
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
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dc.format.none.fl_str_mv 17
application/pdf
dc.publisher.none.fl_str_mv Amer Physical Soc
publisher.none.fl_str_mv Amer Physical Soc
dc.source.none.fl_str_mv Web of Science
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
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repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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