Freeze-in produced dark matter in the ultra-relativistic regime
arXiv:2012.09083 · doi:10.1088/1475-7516/2021/03/075
Abstract
When dark matter particles only feebly interact with plasma constituents in the early universe, they never reach thermal equilibrium. As opposed to the freeze-out mechanism, where the dark matter abundance is determined at , the energy density of a feebly interacting state builds up and increases over . In this work, we address the impact of the high-temperature regime on the dark matter production rate, where the dark and Standard Model particles are ultra-relativistic and nearly light-like. In this setting, multiple soft scatterings, as well as processes, are found to give a large contribution to the production rate. Within the model we consider in this work, namely a Majorana fermion dark matter of mass accompanied by a heavier scalar with mass splitting which shares interactions with the visible sector, the energy density can be dramatically underestimated when neglecting the high-temperature dynamics. We find that the overall effective and high-temperature contributions to dark-matter production give (20\%) corrections for () to the Born production rate with in-vacuum masses and matrix elements. We also assess the impact of bound-state effects on the late-time annihilations of the heavier scalar, in the context of the super-WIMP mechanism.
43 pages, 14 figures, journal version
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