Dark-Matter Spontaneous Freeze Out
Résumé
We consider the possibility that thermalized dark-matter particles acquire their mass thanks to the
spontaneous breaking of a symmetry below some critical temperature. We describe the regime where a
freeze out mechanism takes place shortly after the onset of the phase transition, while the dark-matter
mass has not yet reached its final constant value. For such a “spontaneous freeze out” to yield the correct relic density, the present-time cross section of annihilation of the dark matter into Standard-Model states has to be one or two orders of magnitude larger than in the case of a constant dark-matter mass.