Speaker
Raul Angulo
(DIPC)
Description
In this talk I will describe novel techniques to simulate the nonlinear collapse of dark matter in the cosmos. I will then present simulations of the abundance of dark matter halos and subhalos as a function of the properties of dark matter. In addition, I will discuss simulations that focus on the first collapse of dark matter haloes and the emergence of single power law density profiles. Finally, I will mention various implications for the detection of dark matter and it's potential self-annihilation signature.
Primary author
Raul Angulo
(DIPC)
