Neutrino oscillations and dark matter

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dc.creatorZuber, K.
dc.date1996-12-17
dc.date.accessioned2026-07-07T04:00:59Z
dc.date.available2026-07-07T04:00:59Z
dc.descriptionThe significance of light massive neutrinos as hot dark matter is outlined. The power of neutrino oscillation experiments with respect to detect such neutrinos in the eV-region is discussed. Present hints for neutrino oscillations in solar, atmospheric and LSND data are reviewed as well as future experiments and their potential.
dc.description9 pages, including 3 eps-figures. Talk presented at Workshop Dark96 (Aspects of Dark Matter in Astro- and Particle Physics), Sep. 96 Heidelberg, Germany
dc.identifierhttps://arxiv.org/abs/hep-ph/9612379
dc.identifierhttp://arxiv.org/abs/hep-ph/9612379
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46743
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleNeutrino oscillations and dark matter
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