Indirect Detection of WIMPs
Abstract
I review several proposed techniques for indirect detection of weakly interacting massive particles (WIMPs) in the halo. I focus on distinctive signatures from cosmic-ray positrons, antiprotons, and gamma rays produced by annihilation of WIMPs in the galactic halo. (To appear in Particle Astrophysics, Atomic Physics, and Gravitation, proceedings of the the XIVth Moriond Workshop, Villars sur Ollon, Switzerland, Jan. 22-29, 1994.)
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