Simulations of galactic cold dark matter halos
Jürg Diemand (Lick observatory, Santa Cruz)
Mercredi 07/01/2009, 11:00
Bat 141, salle André Berthelot Masque obligatoire , CEA Paris-Saclay
Large cosmological simulations are now able to follow the formation and evolution of cold dark matter structures reliably and with considerable detail. I will present results about the structure and formation of galactic cold dark matter halos and discuss some of the implications for direct and indirect dark matter detection experiments.