Neutrino Conversion and Neutrino Astrophysics

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dc.creatorSmirnov, A. Yu.
dc.date1998-11-10
dc.date.accessioned2026-07-07T04:05:41Z
dc.date.available2026-07-07T04:05:41Z
dc.descriptionWe consider main ingredients which determine neutrino transformations in media. Strong transformations relevant for the astrophysics can be due to large depth oscillations, resonance conversion, parametric resonance effect, interplay of oscillations and inelastic collisions. Properties of transitions are discussed using the graphic representation. The applications of the transitions to supernova neutrinos are described. The supernova neutrinos can probe whole neutrino mass spectrum. Their studies will help to identify the pattern of neutrino mass and mixing.
dc.description33 pages, LaTeX, 16 figures, talk given at the Symposium ``New Era in Neutrino Physics", Tokyo Metropolitan University, Japan, 11-12 June, 1998
dc.identifierhttps://arxiv.org/abs/hep-ph/9811296
dc.identifierhttp://arxiv.org/abs/hep-ph/9811296
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48496
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleNeutrino Conversion and Neutrino Astrophysics
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