Constraining Dark Matter hypothesis through Diffuse Source observations with the GLAST-LAT detector

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4 pages, 3 figures, presented at the ICRC 07

Scientific paper

The Gamma-Ray Large Area Space Telescope (GLAST), scheduled to be launched in Fall 2007, is a next generation high energy gamma-ray observatory. The Large Area Telescope (LAT) instrument on-board GLAST with a wide field of view ($>$ 2 sr), large effective area and 20 MeV to $>$300 GeV energy range, will provide excellent opportunity for future Dark Matter studies. We present an overview of the GLAST Dark Matter and New Physics Working Group efforts in the study of the LAT capability to detect a gamma-ray flux coming from WIMP pair annihilations in diffuse astrophysical sources. Particular attention will be given to extragalactic diffuse gamma-ray radiation and line searches from annihilation into gamma-gamma and/or gamma-Z final states.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Constraining Dark Matter hypothesis through Diffuse Source observations with the GLAST-LAT detector does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Constraining Dark Matter hypothesis through Diffuse Source observations with the GLAST-LAT detector, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraining Dark Matter hypothesis through Diffuse Source observations with the GLAST-LAT detector will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-467920

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.