Radial acceleration relation and dissipative dark matter
  Observations indicate that ordinary matter, the baryons, influence the
structural properties of dark matter on galactic scales. One such indication is
the radial acceleration relation, which is a tight correlation between the
measured gravitational acceleration and that expected from the baryons. We show
here that the dark matter density profile that has been motivated by
dissipative dark matter models, including mirror dark matter, can reproduce
this radial acceleration relation.
