Implications of the Intriguing Constant Inner Mass Surface Density Observed in Dark Matter Halos
It has long been known that the observed mass surface density of cored dark matter (DM) halos is approximately constant, independently of the galaxy mass (i.e., ρ c r c ≃ constant, with ρ c and r c being the central volume density and the radius of the core, respectively). Here, we review the evidence supporting this empirical fact as well as its
Sánchez Almeida, Jorge
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2025