dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.contributor | ICTP Int Ctr Theoret Phys | |
dc.date.accessioned | 2018-11-26T16:19:30Z | |
dc.date.available | 2018-11-26T16:19:30Z | |
dc.date.created | 2018-11-26T16:19:30Z | |
dc.date.issued | 2016-01-01 | |
dc.identifier | Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 1, 19 p., 2016. | |
dc.identifier | 1475-7516 | |
dc.identifier | http://hdl.handle.net/11449/161194 | |
dc.identifier | 10.1088/1475-7516/2016/01/006 | |
dc.identifier | WOS:000369734300006 | |
dc.identifier | WOS000369734300006.pdf | |
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. | |
dc.language | eng | |
dc.publisher | Iop Publishing Ltd | |
dc.relation | Journal Of Cosmology And Astroparticle Physics | |
dc.relation | 1,089 | |
dc.rights | 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 | |
dc.type | Artículos de revistas | |