Publicação: Z(2) SIMP dark matter
dc.contributor.author | Bernal, Nicolas [UNESP] | |
dc.contributor.author | Chu, Xiaoyong | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.contributor.institution | ICTP Int Ctr Theoret Phys | |
dc.date.accessioned | 2018-11-26T16:19:30Z | |
dc.date.available | 2018-11-26T16:19:30Z | |
dc.date.issued | 2016-01-01 | |
dc.description.abstract | 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. | en |
dc.description.affiliation | Univ Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Pamplona 145, BR-01405 Sao Paulo, Brazil | |
dc.description.affiliation | ICTP Int Ctr Theoret Phys, Str Costiera 11, I-34014 Trieste, Italy | |
dc.description.affiliationUnesp | Univ Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Rua Pamplona 145, BR-01405 Sao Paulo, Brazil | |
dc.description.sponsorship | Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) | |
dc.description.sponsorshipId | FAPESP: 2011/11973-4 | |
dc.description.sponsorshipId | FAPESP: 2013/01792-8 | |
dc.format.extent | 19 | |
dc.identifier | http://dx.doi.org/10.1088/1475-7516/2016/01/006 | |
dc.identifier.citation | Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 1, 19 p., 2016. | |
dc.identifier.doi | 10.1088/1475-7516/2016/01/006 | |
dc.identifier.file | WOS000369734300006.pdf | |
dc.identifier.issn | 1475-7516 | |
dc.identifier.uri | http://hdl.handle.net/11449/161194 | |
dc.identifier.wos | WOS:000369734300006 | |
dc.language.iso | eng | |
dc.publisher | Iop Publishing Ltd | |
dc.relation.ispartof | Journal Of Cosmology And Astroparticle Physics | |
dc.relation.ispartofsjr | 1,089 | |
dc.rights.accessRights | Acesso aberto | |
dc.source | Web of Science | |
dc.subject | dark matter theory | |
dc.subject | particle physics - cosmology connection | |
dc.title | Z(2) SIMP dark matter | en |
dc.type | Artigo | |
dcterms.license | http://iopscience.iop.org/page/copyright | |
dcterms.rightsHolder | Iop Publishing Ltd | |
dspace.entity.type | Publication | |
unesp.author.orcid | 0000-0003-1069-490X[1] | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |
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