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arXiv · 1209.5894

Flavor Oscillations in Core-Collapse Supernovae

A. B. Balantekin
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Abstract

Core collapse supernovae are unique laboratories to study many aspects of neutrino physics. The vicinity of the proto-neutron star in a core-collapse supernova is characterized by large matter and neutrino densities. A salient feature of this region is the impact of neutrino-neutrino interactions. Properties of the ensuing non-linear many-neutrino system are examined with a particular emphasis on its collective behavior and its symmetries. The impact of neutrino properties and interactions on the r-process nucleosynthesis that may take place in the supernova environment is discussed.

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A. B. Balantekin. 2012-09-26. Flavor Oscillations in Core-Collapse Supernovae. https://doi.org/10.1016/j.nuclphysbps.2013.04.037

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