Effects of Neutrino Oscillation on the Supernova Neutrino Spectrum

Details Effects of Neutrino Oscillation on the Supernova Neutrino Spectrum Effects of Neutrino Oscillation on the Supernova Neutrino Spectrum

2001-05-21

arxiv.org/abs/hep-ph/0105204v2

Phys.Rev.D64:093004,2001

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, 14 figures, corrected version

Scientific paper

10.1103/PhysRevD.64.093004

The effects of three-flavor neutrino oscillation on the supernova neutrino spectrum are studied. We calculate the expected event rate and energy spectra, and their time evolution at the Superkamiokande (SK) and the Sudbury Neutrino Observatory (SNO), by using a realistic neutrino burst model based on numerical simulations of supernova explosions. We also employ a realistic density profile based on a presupernova model for the calculation of neutrino conversion probability in supernova envelopes. These realistic models and numerical calculations allow us to quantitatively estimate the effects of neutrino oscillation in a more realistic way than previous studies. We then found that the degeneracy of the solutions of the solar neutrino problem can be broken by the combination of the SK and SNO detections of a future Galactic supernova.

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