Brown dwarfs modeled with a self-interacting dark matter fluid component show modified radii and second-order Love numbers due to core accumulation.
Carmichael,Improved radius determinations for the transiting brown dwarf population in the era of Gaia and TESS, MNRAS519(2023) 5177 [2212.02502]
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Self-Interacting Dark Matter in Brown Dwarfs
Brown dwarfs modeled with a self-interacting dark matter fluid component show modified radii and second-order Love numbers due to core accumulation.