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The effects of three-flavor neutrino oscillation on the supernova neutrinospectrum are studied. We calculate the expected event rate and energy spectra,and their time evolution at the Superkamiokande (SK) and the Sudbury NeutrinoObservatory (SNO), by using a realistic neutrino burst model based on numericalsimulations of supernova explosions. We also employ a realistic density profilebased on a presupernova model for the calculation of neutrino conversionprobability in supernova envelopes. These realistic models and numericalcalculations allow us to quantitatively estimate the effects of neutrinooscillation in a more realistic way than previous studies. We then found thatthe degeneracy of the solutions of the solar neutrino problem can be broken bythe combination of the SK and SNO detections of a future Galactic supernova.Comment: 10 pages, 14 figures, corrected versio

Effects of neutrino oscillation on the supernova neutrino spectrum