Supernova Neutrinos, LSND and MiniBooNE

Details Supernova Neutrinos, LSND and MiniBooNE Supernova Neutrinos, LSND and MiniBooNE

2002-05-19

arxiv.org/abs/hep-ph/0205207v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 6 figures. To appear in the proceedings of 37th Rencontres de Moriond on Electroweak Interactions and Unified Theorie

Scientific paper

The unique constraints on neutrino oscillations which can be obtained by measuring the energy spectrum of supernova $\bar{\nu}_e$'s are first discussed. The focus is on 4-neutrino mass and mixing models capable of explaining the LSND evidence of $\bar{\nu}_{\mu}\to \bar{\nu}_e$ 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.

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