Earth matter effects on the supernova neutrino spectra
Abstract
We explore the earth matter effects on the energy spectra of neutrinos from a supernova. We show that the observations of the energy spectra of e and e from a galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of m232, and to probe the mixing matrix element |Ue3|2 to values as low as 10-3. We point out scenarios in which the matter effects can even be established through the observation of the spectrum at a single detector.
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