A single ~40 eV self-interacting fermion is claimed to fit rotation curves of many galaxies with one adjustable density per galaxy, but fit quality and reported parameter ranges are inconsistent.
S´ anchez Almeida and I
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Modeling dark matter halos with self-interacting fermions: A polytropic approach
A single ~40 eV self-interacting fermion is claimed to fit rotation curves of many galaxies with one adjustable density per galaxy, but fit quality and reported parameter ranges are inconsistent.