pith. machine review for the scientific record. sign in

arxiv: 1611.06746 · v2 · submitted 2016-11-21 · ✦ hep-ph · astro-ph.CO

Recognition: unknown

Implications of Two-component Dark Matter Induced by Forbidden Channels and Thermal Freeze-out

Authors on Pith no claims yet
classification ✦ hep-ph astro-ph.CO
keywords darkmatterfreeze-outchannelscomponentforbiddensymmetrytwo-component
0
0 comments X
read the original abstract

We consider a model of two-component dark matter based on a hidden $U(1)_D$ symmetry, in which relic densities of the dark matter are determined by forbidden channels and thermal freeze-out. The hidden $U(1)_D$ symmetry is spontaneously broken to a residual $\mathbb{Z}_4$ symmetry, and the lightest $\mathbb{Z}_4$ charged particle can be a dark matter candidate. Moreover, depending on the mass hierarchy in the dark sector, we have two-component dark matter. We show that the relic density of the lighter dark matter component can be determined by forbidden annihilation channels which require larger couplings compared to the normal freeze-out mechanism. As a result, a large self-interaction of the lighter dark matter component can be induced, which may solve small scale problems of $\Lambda$CDM model. On the other hand, the heavier dark matter component is produced by normal freeze-out mechanism. We find that interesting implications emerge between the two dark matter components in this framework. We explore detectabilities of these dark matter particles and show some parameter space can be tested by the SHiP experiment.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraining dark matter self-interaction from kinetic heating in neutron stars

    hep-ph 2026-04 unverdicted novelty 4.0

    Observation of neutron stars at 1000-1200 K could constrain asymmetric dark matter self-interaction cross-sections by two orders of magnitude beyond bullet cluster limits.