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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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arxiv 0706.0454 v1 pith:TWECCAPW submitted 2007-06-04 hep-ph

S. P. Mikheev , A. Yu. Smirnov This is my paper · ORCID
classification hep-ph
keywords mediumneutrinooscillationsstarstransformationtypevariable-densityalmost
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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.

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Cited by 1 Pith paper

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  1. Pauli blocking: probing beyond-mean-field effects in neutrino flavor evolution

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    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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