Spontaneous Freeze Out of Dark Matter From an Early Thermal Phase Transition
Lucien Heurtier, Herve Partouche

TL;DR
This paper introduces a novel mechanism for dark matter production where particles spontaneously freeze out after a dark phase transition, leading to distinct phenomenological signatures and requiring larger annihilation cross sections than traditional WIMP models.
Contribution
It presents a minimal model with a scalar and fermionic dark matter that undergoes spontaneous mass change during a dark phase transition, affecting relic abundance calculations.
Findings
Dark matter particles become non-relativistic suddenly after the phase transition.
The required annihilation cross section is over an order of magnitude larger than standard WIMP models.
TeV-scale fermionic dark matter could be detectable in upcoming experiments.
Abstract
We propose a new paradigm for the thermal production of dark matter in the early universe, in which dark-matter particles acquire their mass and freeze out spontaneously from the thermal bath after a dark phase transition takes place. The decoupling arises because the dark-matter particles become suddenly non-relativistic and not because of any decay channel becoming kinematically close. We propose a minimal scenario in which a scalar and a fermionic dark-matter are in thermal equilibrium with the Standard-Model bath. We compute the finite temperature corrections to the scalar potential and identify a region of the parameter space where the fermionic dark-matter mass spontaneously jumps over the temperature when the dark phase transition happens. We explore the phenomenological implications of such a model in simple cases and show that the annihilation cross section of dark-matter…
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