Direct Detection of Nonbaryonic Dark Matter

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dc.creatorBaudis, Laura
dc.creatorKlapdor-Kleingrothaus, H. V.
dc.date2000-03-29
dc.date.accessioned2026-07-07T01:52:56Z
dc.date.available2026-07-07T01:52:56Z
dc.descriptionWeakly Interacting Massive Particles (WIMPs) are leading candidates for the dominant part of the mass density of the Universe. Here we will review direct WIMP detection techniques by giving examples of currently running experiments, and present the status of the most promising future projects.
dc.description18 pages, latex, 8 eps figures, requires iopconf1.sty. To appear in Proceedings of Beyond the Desert '99, Second International Conference on Physics beyond the Standard Model, Castle Ringberg, Tegernsee, Germany, 6-12 June 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/0003434
dc.identifierhttp://arxiv.org/abs/astro-ph/0003434
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/793
dc.subjectAstrophysics
dc.titleDirect Detection of Nonbaryonic Dark Matter
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