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.
Color-Mass-to- Light Ratio Relations for Disk Galaxies
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.