Particle Dark Matter

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dc.creatorDrees, Manuel
dc.date1996-09-09
dc.date1996-09-13
dc.date.accessioned2026-07-07T09:03:20Z
dc.date.available2026-07-07T09:03:20Z
dc.descriptionThere is plenty of evidence that most matter in the Universe is dark (non-luminous). Particle physics offers several possible explanations. In this talk I focus on cold dark matter; the most promising candidates are then axions and the lightest supersymetric particle. I briefly summarize estimates of the present relic density of these particles, and describe efforts to detect them
dc.description14 pages, 4 enclosed figures. Replaced to (hopefully) solve problems with printing of first figure
dc.identifierhttps://arxiv.org/abs/hep-ph/9609300
dc.identifierhttp://arxiv.org/abs/hep-ph/9609300
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/148969
dc.subjectHigh Energy Physics - Phenomenology
dc.titleParticle Dark Matter
dc.typetext

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