The domain of a cannibal dark matter
Abstract
We consider a scenario in which the dark matter is alone in a hidden sector and consists of a real scalar particle with a manifest or spontaneously broken symmetry, at a temperature which differs from the one of the visible sector, . While similar models with general couplings have already been studied in the literature, the special case of a model with spontaneous symmetry breaking constitutes a non-trivial limit of these results, since it features vanishing tree-level amplitudes for the processes with at threshold, thus making the cross-section governing dark-matter freeze-out velocity suppressed. We carefully determine the thermally averaged dark-matter annihilation cross-section in this scenario, including the possible effects of one-loop corrections and Bose-Einstein statistics, while also reporting our results in the domain of thermal dark matter candidates, vs. with being the hidden-sector temperature at decoupling. We show that for fixed quartic coupling, due to entropy conservation, the thermal candidates lie along a curve with anomalous scaling . Furthermore, we demonstrate that this scaling is valid for a broad class of cannibal DM scenarios, with or without symmetry breaking. In addition, we also discuss the relevant cosmological and astrophysical constraints.
Keywords
Cite
@article{arxiv.2212.09759,
title = {The domain of a cannibal dark matter},
author = {Marco Hufnagel and Michel H. G. Tytgat},
journal= {arXiv preprint arXiv:2212.09759},
year = {2023}
}
Comments
26 pages, 6 figures; v2: added discussion on domain-wall formation, matches published version