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Z(2) SIMP dark matter

dc.contributor.authorBernal, Nicolas [UNESP]
dc.contributor.authorChu, Xiaoyong
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionICTP Int Ctr Theoret Phys
dc.date.accessioned2018-11-26T16:19:30Z
dc.date.available2018-11-26T16:19:30Z
dc.date.issued2016-01-01
dc.description.abstractDark 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.en
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Pamplona 145, BR-01405 Sao Paulo, Brazil
dc.description.affiliationICTP Int Ctr Theoret Phys, Str Costiera 11, I-34014 Trieste, Italy
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Pamplona 145, BR-01405 Sao Paulo, Brazil
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipIdFAPESP: 2011/11973-4
dc.description.sponsorshipIdFAPESP: 2013/01792-8
dc.format.extent19
dc.identifierhttp://dx.doi.org/10.1088/1475-7516/2016/01/006
dc.identifier.citationJournal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 1, 19 p., 2016.
dc.identifier.doi10.1088/1475-7516/2016/01/006
dc.identifier.fileWOS000369734300006.pdf
dc.identifier.issn1475-7516
dc.identifier.urihttp://hdl.handle.net/11449/161194
dc.identifier.wosWOS:000369734300006
dc.language.isoeng
dc.publisherIop Publishing Ltd
dc.relation.ispartofJournal Of Cosmology And Astroparticle Physics
dc.relation.ispartofsjr1,089
dc.rights.accessRightsAcesso aberto
dc.sourceWeb of Science
dc.subjectdark matter theory
dc.subjectparticle physics - cosmology connection
dc.titleZ(2) SIMP dark matteren
dc.typeArtigo
dcterms.licensehttp://iopscience.iop.org/page/copyright
dcterms.rightsHolderIop Publishing Ltd
dspace.entity.typePublication
unesp.author.orcid0000-0003-1069-490X[1]
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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