Supernova Neutrino Oscillations

Details Supernova Neutrino Oscillations Supernova Neutrino Oscillations

2005-01-07

arxiv.org/abs/hep-ph/0501049v1

Phys.Scripta T121 (2005) 102-105

Physics

High Energy Physics

High Energy Physics - Phenomenology

Proc. 129 Nobel Symposium "Neutrino Physics", 19-24 Aug 2004, Sweden

Scientific paper

10.1088/0031-8949/2005/T121/014

Observing a high-statistics neutrino signal from a galactic supernova (SN) would allow one to test the standard delayed explosion scenario and may allow one to distinguish between the normal and inverted neutrino mass ordering due to the effects of flavor oscillations in the SN envelope. One may even observe a signature of SN shock-wave propagation in the detailed time-evolution of the neutrino spectra. A clear identification of flavor oscillation effects in a water Cherenkov detector probably requires a megatonne-class experiment.

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