Neutrino Mass Hierarchy and Stepwise Spectral Swapping of Supernova Neutrino Flavors
arXiv:0707.0290 · doi:10.1103/PhysRevLett.99.241802
Abstract
We examine a phenomenon recently predicted by numerical simulations of supernova neutrino flavor evolution: the swapping of supernova and energy spectra below (above) energy $\EC$ for the normal (inverted) neutrino mass hierarchy. We present the results of large-scale numerical calculations which show that in the normal neutrino mass hierarchy case, $\EC$ decreases as the assumed effective vacuum mixing angle () is decreased. However, these calculations also indicate that $\EC$ is essentially independent of the vacuum mixing angle in the inverted neutrino mass hierarchy case. With a good neutrino signal from a future Galactic supernova, the above results could be used to determine the neutrino mass hierarchy even if is too small to be detected in terrestrial neutrino oscillation experiments.
arXiv comment4 pages, 2 figures. Version accepted by PRL
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