Z(2) SIMP dark matter

Detalhes bibliográficos
Autor(a) principal: Bernal, Nicolas [UNESP]
Data de Publicação: 2016
Outros Autores: Chu, Xiaoyong
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1475-7516/2016/01/006
http://hdl.handle.net/11449/161194
Resumo: Dark matter with strong self-interactions provides a compelling solution to several small-scale structure puzzles. Under the assumption that the coupling between dark matter and the Standard Model particles is suppressed, such strongly interacting massive particles (SIMPs) allow for a successful thermal freeze-out through N-to-N' processes, where N dark matter particles annihilate to N' of them. In the most common scenarios, where dark matter stability is guaranteed by a Z(2) symmetry, the seemingly leading annihilating channel, i.e. 3-to- 2 process, is forbidden, so the 4-to-2 one dominate the production of the dark matter relic density. Moreover, cosmological observations require that the dark matter sector is colder than the thermal bath of Standard Model particles, a condition that can be dynamically generated via a small portal between dark matter and Standard Model particles, a la freeze-in. This scenario is exempli fied in the context of the Singlet Scalar dark matter model.
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spelling Z(2) SIMP dark matterdark matter theoryparticle physics - cosmology connectionDark matter with strong self-interactions provides a compelling solution to several small-scale structure puzzles. Under the assumption that the coupling between dark matter and the Standard Model particles is suppressed, such strongly interacting massive particles (SIMPs) allow for a successful thermal freeze-out through N-to-N' processes, where N dark matter particles annihilate to N' of them. In the most common scenarios, where dark matter stability is guaranteed by a Z(2) symmetry, the seemingly leading annihilating channel, i.e. 3-to- 2 process, is forbidden, so the 4-to-2 one dominate the production of the dark matter relic density. Moreover, cosmological observations require that the dark matter sector is colder than the thermal bath of Standard Model particles, a condition that can be dynamically generated via a small portal between dark matter and Standard Model particles, a la freeze-in. This scenario is exempli fied in the context of the Singlet Scalar dark matter model.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Univ Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Pamplona 145, BR-01405 Sao Paulo, BrazilICTP Int Ctr Theoret Phys, Str Costiera 11, I-34014 Trieste, ItalyUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Pamplona 145, BR-01405 Sao Paulo, BrazilFAPESP: 2011/11973-4FAPESP: 2013/01792-8Iop Publishing LtdUniversidade Estadual Paulista (Unesp)ICTP Int Ctr Theoret PhysBernal, Nicolas [UNESP]Chu, Xiaoyong2018-11-26T16:19:30Z2018-11-26T16:19:30Z2016-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article19application/pdfhttp://dx.doi.org/10.1088/1475-7516/2016/01/006Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 1, 19 p., 2016.1475-7516http://hdl.handle.net/11449/16119410.1088/1475-7516/2016/01/006WOS:000369734300006WOS000369734300006.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal Of Cosmology And Astroparticle Physics1,089info:eu-repo/semantics/openAccess2023-11-17T06:10:34Zoai:repositorio.unesp.br:11449/161194Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T17:55:36.915928Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Z(2) SIMP dark matter
title Z(2) SIMP dark matter
spellingShingle Z(2) SIMP dark matter
Bernal, Nicolas [UNESP]
dark matter theory
particle physics - cosmology connection
title_short Z(2) SIMP dark matter
title_full Z(2) SIMP dark matter
title_fullStr Z(2) SIMP dark matter
title_full_unstemmed Z(2) SIMP dark matter
title_sort Z(2) SIMP dark matter
author Bernal, Nicolas [UNESP]
author_facet Bernal, Nicolas [UNESP]
Chu, Xiaoyong
author_role author
author2 Chu, Xiaoyong
author2_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
ICTP Int Ctr Theoret Phys
dc.contributor.author.fl_str_mv Bernal, Nicolas [UNESP]
Chu, Xiaoyong
dc.subject.por.fl_str_mv dark matter theory
particle physics - cosmology connection
topic dark matter theory
particle physics - cosmology connection
description Dark matter with strong self-interactions provides a compelling solution to several small-scale structure puzzles. Under the assumption that the coupling between dark matter and the Standard Model particles is suppressed, such strongly interacting massive particles (SIMPs) allow for a successful thermal freeze-out through N-to-N' processes, where N dark matter particles annihilate to N' of them. In the most common scenarios, where dark matter stability is guaranteed by a Z(2) symmetry, the seemingly leading annihilating channel, i.e. 3-to- 2 process, is forbidden, so the 4-to-2 one dominate the production of the dark matter relic density. Moreover, cosmological observations require that the dark matter sector is colder than the thermal bath of Standard Model particles, a condition that can be dynamically generated via a small portal between dark matter and Standard Model particles, a la freeze-in. This scenario is exempli fied in the context of the Singlet Scalar dark matter model.
publishDate 2016
dc.date.none.fl_str_mv 2016-01-01
2018-11-26T16:19:30Z
2018-11-26T16:19:30Z
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/10.1088/1475-7516/2016/01/006
Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 1, 19 p., 2016.
1475-7516
http://hdl.handle.net/11449/161194
10.1088/1475-7516/2016/01/006
WOS:000369734300006
WOS000369734300006.pdf
url http://dx.doi.org/10.1088/1475-7516/2016/01/006
http://hdl.handle.net/11449/161194
identifier_str_mv Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 1, 19 p., 2016.
1475-7516
10.1088/1475-7516/2016/01/006
WOS:000369734300006
WOS000369734300006.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal Of Cosmology And Astroparticle Physics
1,089
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 19
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing Ltd
publisher.none.fl_str_mv Iop Publishing Ltd
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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