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Supernova Neutrinos, LSND and MiniBooNE

Michel Sorel
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Abstract

The 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.

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Michel Sorel. 2002-05-19. Supernova Neutrinos, LSND and MiniBooNE. https://arxiv.org/abs/hep-ph/0205207

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