Astrophysical Neutrinos and Flavor Evolution With Self Interaction
arXiv:1609.08862 · doi:10.7566/JPSCP.14.020709
Abstract
In a core collapse supernova, collective oscillations of neutrinos emitted by the proto-neutron star significantly modifies the partition of energy between different flavors in a way which is potentially important for the nucleosynthesis of heavy elements at the outer layers. As the outcome of collective oscillations depends nonlinearly on the chosen initial conditions proto-neutron star, their systematical study across the proto-neutron star model space may provide answers to some key questions.
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