Spin Flavor Spectral Splits of Supernova Neutrino Flavor Conversions
arXiv:2105.07928
Abstract
The supernova neutrino flavor evolution in the presence of the non-trivial neutrino magnetic moment and strong magnetic field is numerically derived using the two-flavor and single-angle approximation. The novel properties of collective neutrino oscillations are studied and distinct patterns of flavor and spin-flavor spectral splits are presented. Finally we also discuss how the neutrino magnetic moment affects the observable supernova neutrino energy spectra.
arXiv comment10 pages, 4 figures
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