%0 Journal Article
%T Dark Matter Searches with GLAST
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%A Nuss, E.
%Z Comment: 6 pages, 3 figures, 36th COSPAR proceeding accepted for publication in "Advances in Space Research"
%< avec comité de lecture
%Z LPTA/07-20
%@ 0273-1177
%J Advances in Space Research
%I Elsevier
%V 41/12
%P 2029-2031
%8 2007
%D 2007
%Z 0704.2738
%R 10.1016/j.asr.2007.03.045
%Z Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]Journal articles
%X The Gamma-Ray Large Area Space Telescope (GLAST), scheduled to be launched in fall 2007, is the next generation satellite for high-energy gamma-ray astronomy. The Large Area Telescope (LAT), GLAST main instrument, with a wide field of view (> 2 sr), a large effective area (> 8000 cm^2 at 1 GeV) and 20 MeV - 300 GeV energy range, will provide excellent high energy gamma-ray observations for Dark Matter searches. In this paper we examine the potential of the LAT to detect gamma-rays coming from WIMPS annihilation in the context of supersymmetry. As an example, two search regions are investigated: the galactic center and the galactic satellites.
%G English
%L in2p3-00148883
%U https://hal.in2p3.fr/in2p3-00148883
%~ IN2P3
%~ LPTA
%~ CNRS
%~ UNIV-MONTP2
%~ UNIV-MONTPELLIER
%~ UM1-UM2