Dark matter self-interactions from a general spin-0 mediator
Abstract
Dark matter particles interacting via the exchange of very light spin-0 mediators can have large self-interaction rates and obtain their relic abundance from thermal freeze-out. At the same time, these models face strong bounds from direct and indirect probes of dark matter as well as a number of constraints on the properties of the mediator. We investigate whether these constraints can be consistent with having observable effects from dark matter self-interactions in astrophysical systems. For the case of a mediator with purely scalar couplings we point out the highly relevant impact of low-threshold direct detection experiments like CRESST-II, which essentially rule out the simplest realization of this model. These constraints can be significantly relaxed if the mediator has CP-violating couplings, but then the model faces strong constraints from CMB measurements, which can only be avoided in special regions of parameter space.
Cite
@article{arxiv.1704.02149,
title = {Dark matter self-interactions from a general spin-0 mediator},
author = {Felix Kahlhoefer and Kai Schmidt-Hoberg and Sebastian Wild},
journal= {arXiv preprint arXiv:1704.02149},
year = {2017}
}
Comments
20 pages, 5 figures + appendices. v2: Matches published version. v3: fixed typographical mistake in eq. (2.8). v4: fixed typographical mistake in eq. (C.4)