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Neutrino oscillations in a variable-density medium and $\nu-$ bursts due to the gravitational collapse of stars
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Under certain conditions, the propagation of a beam of oscillating neutrinos in a variable-density medium takes the form of an almost complete transformation of the initial type of neutrino into another type. The depth of oscillations is then negligible. The transformation can occur in the cores and envelopes of collapsing stars.
Forward citations
Cited by 2 Pith papers
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Theory of neutrino slow flavor evolution. Part I. Homogeneous medium
Slow neutrino flavor instabilities split into a new resonant small-scale branch with growth rate ~omega_E/epsilon and the familiar non-resonant branch with the traditional scale 1/sqrt(omega_E mu).
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Pauli blocking: probing beyond-mean-field effects in neutrino flavor evolution
Adding heuristic Pauli-blocking factors to neutrino self-interactions shifts fast flavor stability regions: two instabilities weaken, and one stable case becomes unstable.
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