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/11449/162904 |
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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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 |
eu_rights_str_mv |
openAccess |
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 |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
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1808129435534098432 |