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 ℤ2 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, à la freeze-in. This scenario is exemplified in the context of the Singlet Scalar dark matter model.
Highlights
In the most common scenarios, where dark matter stability is guaranteed by a Z2 symmetry, the seemingly leading annihilating channel, i.e. 3to-2 process, is forbidden, so the 4-to-2 one dominate the production of the dark matter relic density
There has been a large amount of research on the singlet scalar dark matter (DM) model, most of them focused on the WIMP scenario, where the singlet S mixes relatively strongly with the Higgs and undergoes a thermal freeze-out
The collisionless cold dark matter (DM) paradigm has been highly successful in accounting for large scale structure of the Universe
Summary
View the article online for updates and enhancements. - Production regimes for Self-Interacting Dark Matter Nicolás Bernal, Xiaoyong Chu, Camilo Garcia-Cely et al. View the article online for updates and enhancements. - Production regimes for Self-Interacting Dark Matter Nicolás Bernal, Xiaoyong Chu, Camilo Garcia-Cely et al. - WIMP and SIMP dark matter from the spontaneous breaking of a global group Nicolás Bernal, Camilo Garcia-Cely and Rogério Rosenfeld. - Fermi Bubbles under Dark Matter Scrutiny Part II: Particle Physics Analysis Wei-Chih Huang, Alfredo Urbano and Wei Xue. - Velocity Dependence from Resonant SelfInteracting Dark Matter Xiaoyong Chu et al. - Phenomenology of self-interacting dark matter in a matter-dominated universe Nicolás Bernal et al. This content was downloaded from IP address 186.217.236.55 on 19/06/2019 at 17:00
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