Searching for TeV dark matter by atmospheric Cerenkov techniques

Details Searching for TeV dark matter by atmospheric Cerenkov techniques Searching for TeV dark matter by atmospheric Cerenkov techniques

1992-08-27

arxiv.org/abs/hep-ph/9208255v1

Phys.Lett. B293 (1992) 149-156

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pp, LaTex (3 figures available by e-mail) PAR-LPTHE 92XX

Scientific paper

10.1016/0370-2693(92)91494-T

There is a growing interest in the possibility that dark matter could be
formed of weakly interacting particles with a mass in the 100 GeV - 2 TeV
range, and supersymmetric particles are favorite candidates. If they constitute
the dark halo of our Galaxy, their mutual annihilations produce energetic gamma
rays that could be detected using existing atmospheric \u{C}erenkov techniques.

Affiliated with

Also associated with

No associations

Rating

Searching for TeV dark matter by atmospheric Cerenkov techniques 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 Searching for TeV dark matter by atmospheric Cerenkov techniques, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Searching for TeV dark matter by atmospheric Cerenkov techniques will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-701982