Simulations of galactic cold dark matter halos
Jürg Diemand (Lick observatory, Santa Cruz)
Mercredi 07/01/2009, 11:00
Bat 141, salle André Berthelot (143) Masque recommandé, 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.


Retour en haut