Indirect Detection of WIMPs

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dc.creatorKamionkowski, Marc
dc.date1994-03-24
dc.date.accessioned2026-07-07T03:56:45Z
dc.date.available2026-07-07T03:56:45Z
dc.descriptionI 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.)
dc.description(12 pages available as a uuencoded, tarred, compressed PostScript file), IASSNS-HEP-94/8
dc.identifierhttps://arxiv.org/abs/hep-ph/9403357
dc.identifierhttp://arxiv.org/abs/hep-ph/9403357
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/45116
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleIndirect Detection of WIMPs
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