WIMP and Axion Dark Matter

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dc.creatorKamionkowski, Marc
dc.date1997-10-24
dc.date.accessioned2026-07-07T04:02:42Z
dc.date.available2026-07-07T04:02:42Z
dc.descriptionThere is almost universal agreement among cosmologists that most of the matter in the Universe is dark, and there are very good reasons to believe that most of this dark matter must be nonbaryonic. The two leading candidates for this dark matter are axions and weakly-interacting massive particles (WIMPs), such as the neutralino in supersymmetric extensions of the standard model. I discuss the arguments for these two dark-matter candidates and review techniques for discovery of these dark-matter particles.
dc.description18 pages, LaTeX, introductory lectures given at the 1997 ICTP Summer School on High Energy Physics and Cosmology, Trieste, Italy, June 2--July 4, 1997
dc.identifierhttps://arxiv.org/abs/hep-ph/9710467
dc.identifierhttp://arxiv.org/abs/hep-ph/9710467
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/47339
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleWIMP and Axion Dark Matter
dc.typetext

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