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IDM2008 - Identification of Dark Matter 2008
IDM2008 - Identification of Dark Matter 2008
18-22 August 2008 AlbaNova
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Indirect search for DarkMatter from the Galactic Center (15'+5')
High energy gamma ray observations can be used for the indirect search for
annihilating Dark Matter.
One of the possible observation strategy is the targeting of regions where high 
Matter density
is foreseen, such as the Galactic Center.
This observation poses a challenge: to disentangle the possible Dark Matter 
from the bright
gamma radiation of astrophysical sources.
The Large Area Telescope on board of the GLAST satellite provides the best
opportunity to date for such a study,
because of its excellent sensitivity and angular resolution, as compared to the 
satellite-borne detectors.
A report of the  GLAST LAT Dark Matter Group activities on this topic will be 
Id: 428
Place: AlbaNova
Room: FB42
Starting date:
20-Aug-2008   09:30
Duration: 20'
Contribution type: Talk
Primary Authors: Dr. VITALE, Vincenzo (dip. Fisica & INFN Roma Tor Vergata)
Presenters: Dr. VITALE, Vincenzo
Material: slide Slides
Included in session: Indirect searches - gammas, neutrinos, etc
Included in track: Indirect searches - gammas

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