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arXiv · 1609.08862

Astrophysical Neutrinos and Flavor Evolution With Self Interaction

T. Bulmus·Y. Pehlivan
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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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T. Bulmus, Y. Pehlivan. 2016-09-28. Astrophysical Neutrinos and Flavor Evolution With Self Interaction. https://doi.org/10.7566/jpscp.14.020709

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