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Paper detail

Asymmetric Dark Matter Stars

We study the possibility of asymmetric dark matter with self-interactions forming compact stable objects. We solve the Tolman-Oppenheimer-Volkoff equation and find the mass-radius relation of such "dark stars", their density profile and their Chandrasekhar mass limit. We consider fermionic asymmetric dark matter with Yukawa-type self-interactions appropriate for solving the well known problems of the collisionless dark matter paradigm. We find that in several cases the relativistic effects are significant.

preprint2015arXivOpen access
Chris KouvarisNiklas Grønlund Nielsen
hep-phastro-ph.HE
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Chris KouvarisNiklas Grønlund Nielsen

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