![]() ![]() ![]() Or in small numbers, in very dense DM minihalos at $z\sim 15-40$, and, in our Interest are: at high red-shifts, Population III stars that form in isolation, On the nucleon-Dark Matter interaction cross section. Observable signatures of DM gravitationally trapped inside a star, or anotherĬompact astrophysical object, have been used to forecast stringent constraints Probes has become more and more evident, especially in view of null resultsįrom direct detection and particle production experiments. ![]() Download a PDF of the paper titled Multicomponent multiscatter capture of Dark Matter, by Cosmin Ilie and 1 other authors Download PDF Abstract: In recent years, the usefulness of astrophysical objects as Dark Matter (DM) ![]()
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