1996/12/17 by K. Zuber, Zuber, K.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9612379
9 pages, including 3 eps-figures. Talk presented at Workshop Dark96 (Aspects of Dark Matter in Astro- and Particle Physics), Sep. 96 Heidelberg, Germany
arxiv created 1996/12/17 · arxiv updated 2009/11/30
The 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.