Antimatter and Gamma-rays from Dark Matter Annihilation

Details Antimatter and Gamma-rays from Dark Matter Annihilation Antimatter and Gamma-rays from Dark Matter Annihilation

2007-12-06

arxiv.org/abs/0712.0984v1

J.Phys.Conf.Ser.120:042005,2008

Astronomy and Astrophysics

Astrophysics

7p, one fig., invited talk at TAUP 2007, Sendai, Japan, to appear in the Proceedings

Scientific paper

10.1088/1742-6596/120/4/042005

A brief review of the indirect detection signatures of dark matter is given. In particular, detection methods of dark matter particle annihilation to antimatter and gamma-rays are reviewed. With the GLAST satellite soon to be launched, a crucial window in the energy range of a few GeV up to 300 GeV will open. The good angular and energy resolution of the instrument means that structures predicted by cold dark matter models can be searched for. Large, currently planned ground-based imaging Cherenkov telescope arrays, may further improve the limits, or discover a signal, if the current understanding of halo dark matter structure is correct.

Affiliated with

Also associated with

No associations

Rating

Antimatter and Gamma-rays from Dark Matter Annihilation 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 Antimatter and Gamma-rays from Dark Matter Annihilation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Antimatter and Gamma-rays from Dark Matter Annihilation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-92200