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

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dc.creatorWai, Lawrence
dc.creatorCollaboration, GLAST LAT
dc.date2007-01-31
dc.date.accessioned2026-07-07T11:21:03Z
dc.date.available2026-07-07T11:21:03Z
dc.descriptionThe 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.
dc.descriptionDM06 Proceedings (contributed talk)
dc.identifierhttps://arxiv.org/abs/astro-ph/0701885
dc.identifierhttp://arxiv.org/abs/astro-ph/0701885
dc.identifierNucl.Phys.Proc.Suppl.173:60-63,2007
dc.identifierdoi:10.1016/j.nuclphysbps.2007.08.027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194149
dc.subjectAstrophysics
dc.titleThe search for Milky Way halo substructure WIMP annihilations using the GLAST LAT
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