Schedule Oct 02, 2008
The Gamma-ray Signal from Galactic Dark Matter Substructure
Mike Kuhlen (IAS)

The amount and spatial distribution of dark matter substructure in the Milky Way halo provide unique information and clues on the galaxy assembly process and the nature of the dark matter. I will present results from "Via Lactea II", a high resolution numerical simulation of Galactic CDM substructure, with a particular focus on the possibility of GLAST detecting gamma-rays from DM annihilations in the centers of subhalos.

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