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arXiv · astro-ph/9209005

Neutrino Flavor Conversion in a Supernova Core

G. Raffelt·G. Sigl
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Abstract

If $ν_μ$ or $ν_τ$ mix with $ν_e$, neutrino oscillations and collisions in a supernova (SN) core allow these flavors effectively to participate in $β$ equilibrium and thus to obtain a large chemical potential. If a sterile species mixes with $ν_e$, these effects lead to an anomalous loss of energy and lepton number. We study flavor conversion in a SN core on the basis of a new kinetic equation which rigorously includes neutrino interference and degeneneracy effects. Our discussion serves as an example and illustration of the properties of this ``non-abelian Boltzmann equation''.

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G. Raffelt, G. Sigl. 1992-09-24. Neutrino Flavor Conversion in a Supernova Core. https://doi.org/10.1016/0927-6505(93)90020-e

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