Supernova Neutrinos, LSND and MiniBooNE

dc.creatorSorel, Michel
dc.date2002-05-19
dc.date.accessioned2026-07-07T03:47:05Z
dc.date.available2026-07-07T03:47:05Z
dc.descriptionThe unique constraints on neutrino oscillations which can be obtained by measuring the energy spectrum of supernova $\barν_e$'s are first discussed. The focus is on 4-neutrino mass and mixing models capable of explaining the LSND evidence of $\barν_μ\to \barν_e$ oscillations. The potential of the Fermilab neutrino detector MiniBooNE to observe supernova neutrinos is then addressed, and a general description of the detector is given. As of May, 2002, the MiniBooNE detector is fully operational.
dc.description6 pages, 6 figures. To appear in the proceedings of 37th Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, France, 9-16 Mar 2002
dc.identifierhttps://arxiv.org/abs/hep-ph/0205207
dc.identifierhttp://arxiv.org/abs/hep-ph/0205207
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41533
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSupernova Neutrinos, LSND and MiniBooNE
dc.typetext

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