Supernova neutrino oscillations: what do we understand?

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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6 pages, 1 eps figure, jpconf.cls used. Talk given at TAUP 2009, Rome, July 2009

Scientific paper

10.1088/1742-6596/203/1/012015

We summarize our current understanding of the neutrino flavor conversions inside a core collapse supernova, clarifying the important role played by the "collective effects" in determining flavor conversion probabilities. The potentially observable $\nu_e$ and $\bar{\nu}_e$ spectra may help us identify the neutrino mixing scenario, distinguish between primary flux models, and learn more about the supernova explosion.

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