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2018

On the evolution process of two-component dark matter in the Sun

Chen, Chian-Shu, Lin, Yen-Hsun

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We introduce dark matter (DM) evolution process in the Sun under a two-component DM (2DM) scenario.

Both DM species $\chi$ and $\xi$ with masses heavier than 1 GeV are considered.
In this picture, both species could be captured by the Sun through DM-nucleus scattering and DM self-scatterings, e.g.
$\chi\chi$ and $\xi\xi$ collisions.

On the evolution process of two-component dark matter in the Sun · Around

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