Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos

Details Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos

1999-12-18

arxiv.org/abs/hep-ph/9912414v1

Nucl.Phys.Proc.Suppl. 87 (2000) 327-329

Physics

High Energy Physics

High Energy Physics - Phenomenology

3 pages, 1 eps figure. Talk given at TAUP-99. To be published in Nucl. Phys. B, Proc. Suppl

Scientific paper

10.1016/S0920-5632(00)00694-0

We analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. We find that the observations of the energy spectra of neutrinos from a future galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $\Delta m^2_{32}$, and to probe the mixing matrix element |U_{e3}|^2 to values as low as 10^{-4}-10^{-3}.

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