Recent Developments in Dark Matter Physics

dc.creatorDrees, Manuel
dc.date1997-03-07
dc.date.accessioned2026-07-07T04:01:22Z
dc.date.available2026-07-07T04:01:22Z
dc.descriptionAfter a short review of the arguments for the existence of Particle Dark Matter in the Universe, I list the most plausible candidates provided by particle physics, i.e. neutrinos, axions, and WIMPs. In each case I briefly describe how to estimate the relic density, and discuss attempts at detecting these particles. At the end I discuss my personal favorite, the lightest supersymmetric particle, in a little more detail.
dc.description13 pages, LaTeX with equation.sty, no figures; invited talk given at the 12th DAE Symposium, Guwahati, Assam, India, Dec. 1996
dc.identifierhttps://arxiv.org/abs/hep-ph/9703260
dc.identifierhttp://arxiv.org/abs/hep-ph/9703260
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46870
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRecent Developments in Dark Matter Physics
dc.typetext

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