Langevin simulation of dark matter kinetic equilibration

Abstract

Recently it has been questioned, notably in the context of the scalar singlet dark matter model with $m_{\phi }^{}\simeq 60$ GeV, how efficiently kinetic equilibrium is maintained if freeze-out dynamics is pushed down to low temperatures by resonant effects. We outline how Langevin simulations can be employed for addressing the non-equilibrium momentum distribution of non-relativistic particles in a cosmological background. For a scalar singlet mass $m_{\phi }^{}\simeq 60$ GeV, these simulations suggest that kinetic equilibrium is a good approximation down to $T\sim 1$ GeV, with the deviation first manifesting itself as a red-tilted spectrum. This reduces the annihilation cross section, confirming findings from other methods that a somewhat larger ($<20\%$) coupling than in equilibrium is needed for obtaining the correct abundance.

arXiv comment15 pages. v2: clarifications added

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