Sánchez Almeida,Constraints on dark matter models from the stellar cores observed in ultra-faint dwarf galaxies: Self-interacting dark matter, A&A704(2025) A210 [2510.05682]

· 2025 · arXiv 2510.05682

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astro-ph.SR · 2026-05-14 · unverdicted · novelty 3.0

Brown dwarfs modeled with a self-interacting dark matter fluid component show modified radii and second-order Love numbers due to core accumulation.

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Self-Interacting Dark Matter in Brown Dwarfs astro-ph.SR · 2026-05-14 · unverdicted · none · ref 23
Brown dwarfs modeled with a self-interacting dark matter fluid component show modified radii and second-order Love numbers due to core accumulation.