Z(2) SIMP dark matter
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Outros Autores: | |
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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Repositório Institucional da UNESP |
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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 |
|
_version_ |
1808128875865047040 |