VIA lecture by Dr. Federico Lelli "The radial acceleration relation: linking baryons and dark matter in galaxies" was given on 02.12.2016. It's pdf is attached.
The following comments were made in the discussion:
Houri Ziaeepour: A comment: Assuming no initial bias between DM and baryons, one expects that even after collapse of baryons in the center of potentials, a correlation between the 2 persists, specially at large radii.
Houri Ziaeepour: Sure. But similations are still far from being complete.
Houri Ziaeepour: Therefore the deviation between observations and simulations cannot be automatically related to new physics.
You are welcome to continue discussion in replies to this post!