The search for Milky Way halo substructure WIMP annihilations using the GLAST LAT

Details The search for Milky Way halo substructure WIMP annihilations using the GLAST LAT The search for Milky Way halo substructure WIMP annihilations using the GLAST LAT

2007-01-31

arxiv.org/abs/astro-ph/0701885v1

Nucl.Phys.Proc.Suppl.173:60-63,2007

Astronomy and Astrophysics

Astrophysics

DM06 Proceedings (contributed talk)

Scientific paper

10.1016/j.nuclphysbps.2007.08.02

The GLAST LAT Collaboration is one among several experimental groups, covering a wide range of approaches, pursuing the search for the nature of dark matter. The GLAST LAT has the unique ability to find new sources of high energy gamma radiation emanating directly from WIMP annihilations in situ in the universe. Using it's wide band spectral and full sky spatial capabilities, the GLAST LAT can form "images" in high energy gamma-rays of dark matter substructures in the gamma-ray sky. We describe a preliminary feasibility study for indirect detection of Milky Way dark matter satellites using the GLAST LAT.

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