Halo density profiles and baryon physics

摘要: The radial dependence of the pseudo phase-space density, ρ(r)/σ 3(r) is studied. We find that density for halos consisting both dark matter and baryons approximately a power-law only down to 0.1% virial radius while it has non-power law behavior below quoted scale, with inner profiles changing mass. Halos just matter, as one in simulations, are characterized by an behavior. results argue against universality when effect included, consequence constituted also discussed [1].