Dark Matter Scaling Relations

Abstract

We establish the presence of a dark matter core radius, for the first time in a very large number of spiral galaxies of all luminosities. Contrary to common opinion we find that the sizes of these cores and the " DM core problem" are bigger for more massive spirals. As a result the Burkert profile provides an excellent mass model for dark halos around disk galaxies. Moreover, we find that the spiral dark matter core densities ${\rho }_0$ and core radii $r_0$ lie in the same scaling relation ${\rho }_0=4.5\times 10^{-}2(r_0/kpc{)}^{-2/3}{M}_{\odot }p{c}^{-3}$ of dwarf galaxies with core radii upto ten times more smaller.

4 pages, 4 figures, Accepted for Publication in Apj Lett

References in corpus (1)

• The Extended Rotation Curve and the Dark Matter Halo of M33

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