Speaker
Carlos Frenk
Description
I will present results from the "Phoenix" programme of very
high resolution N-body simulations of cluster-size cold dark
matter halos. I will discuss the mass distribution and
internal structure of the halos and their subhalos. If the
dark matter is made of supersymmetric particles,
particle/anti-particle annihilation is likely to result in
the emission of detectable gamma-ray radiation. I will
discuss predictions from these simulations for the
properties of this emission.
