TL;DR
This paper explores the complex velocity and angular dependence of dark matter self-interactions mediated by a light particle, providing new analytic tools and mapping the full parameter space relevant for cosmic structure formation.
Contribution
It introduces a method to analyze the velocity and angular dependence of dark matter self-scattering in complex regimes, extending beyond simple models.
Findings
Mapped the parameter space of dark matter self-interactions
Derived a new analytic formula for resonant s-wave scattering
Linked self-interactions to Sommerfeld enhancements in indirect detection
Abstract
Dark matter (DM) self-interactions have important implications for the formation and evolution of structure, from dwarf galaxies to clusters of galaxies. We study the dynamics of self-interacting DM via a light mediator, focusing on the quantum resonant regime where the scattering cross section has a non-trivial velocity dependence. While there are long-standing indications that observations of small scale structure in the Universe are not in accord with the predictions of collisionless DM, theoretical study and simulations of DM self-interactions have focused on parameter regimes with simple analytic solutions for the scattering cross section, with constant or classical velocity (and no angular) dependence. We devise a method that allows us to explore the velocity and angular dependence of self-scattering more broadly, in the strongly-coupled resonant and classical regimes where many…
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