Freezing-in a hot bath: resonances, medium effects and phase transitions
Torsten Bringmann, Saniya Heeba, Felix Kahlhoefer, Kristian, Vangsnes

TL;DR
This paper improves the theoretical and computational modeling of dark matter freeze-in production, incorporating medium effects, phase transitions, and resonances, and provides the most accurate calculations to date for scalar singlet dark matter.
Contribution
It introduces a new formulation for freeze-in production that includes plasma effects, phase transition impacts, and resonance complications, along with an updated computational tool.
Findings
Most accurate calculation of scalar singlet dark matter abundance.
Freeze-in couplings potentially testable at the LHC.
Enhanced computational framework for high-temperature dark matter production.
Abstract
Relic density calculations of dark matter freezing out from the primordial plasma have reached a high level of sophistication, with several numerical tools readily available that match the observationally required accuracy. Dark matter production via the freeze-in mechanism, on the other hand, is sensitive to much higher temperatures than in the freeze-out case, implying both technical and computational difficulties when aiming for the same level of precision. We revisit the formulation of freeze-in production in a way that facilitates the inclusion of in-medium corrections like plasma effects and the spin statistics of relativistic quantum gases, as well as the temperature dependence of dark matter production rates induced by the electroweak and strong phase transitions, and we discuss in detail the additional complications arising in the presence of -channel resonances. We…
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