A new empirical dark matter profile ρ_DM = μ Φ_b² / c⁴ with μ = K M_b^{-3/2} fits SPARC galaxy rotation curves and resolves core-cusp and diversity problems using only baryonic data.
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Resolving the Core-Cusp and Diversity Problems with a Baryon-Correlated Dark Matter Profile
A new empirical dark matter profile ρ_DM = μ Φ_b² / c⁴ with μ = K M_b^{-3/2} fits SPARC galaxy rotation curves and resolves core-cusp and diversity problems using only baryonic data.