Multicomponent multiscatter capture of Dark Matter
Cosmin Ilie, Caleb Levy

TL;DR
This paper extends the formalism of dark matter capture to multicomponent astrophysical objects, specifically applying it to Population III stars to evaluate how helium influences dark matter capture rates, enhancing their utility as probes.
Contribution
It introduces a multicomponent capture formalism and applies it to Population III stars, highlighting the impact of helium on dark matter capture rates.
Findings
Heavier helium nuclei increase capture rates in Pop III stars.
Multicomponent formalism improves dark matter detection prospects.
Capture rate enhancement strengthens Pop III stars as dark matter probes.
Abstract
In recent years, the usefulness of astrophysical objects as Dark Matter (DM) probes has become more and more evident, especially in view of null results from direct detection and particle production experiments. The potentially observable signatures of DM gravitationally trapped inside a star, or another compact astrophysical object, have been used to forecast stringent constraints on the nucleon-Dark Matter interaction cross section. Currently, the probes of interest are: at high red-shifts, Population III stars that form in isolation, or in small numbers, in very dense DM minihalos at , and, in our own Milky Way, neutron stars, white dwarfs, brown dwarfs, exoplanets, etc. Of those, only neutron stars are single-component objects, and, as such, they are the only objects for which the common assumption made in the literature of single-component capture, i.e. capture of DM…
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