Speaker
Dr
Andrea Maccio
(Max Planck Institute for Astronomy)
Description
I will summarize current results based on cosmological simulations about the
distribution of Dark Matter on both large and small scales. I will show how the
distribution of DM can be influence by the nature of the dark matter candidate (Warm
vs Cold), by the modeling of Dark Energy and by the presence of baryons.
Primary author
Dr
Andrea Maccio
(Max Planck Institute for Astronomy)
