Implications of conservation laws and ergodicity for neutrino flavor instability

Collective neutrino flavor instabilities are believed to be prevalent in core-collapse supernovae and neutron star mergers. This work establishes two points related to instability, both in the spirit of developing a more fundamental understanding of collective flavor dynamics. First, a conservation law related to the lepton number implies that spectral crossings are necessary for instability. Second, the most permissive application of the ergodic hypothesis to neutrino flavor evolution implies that spectral crossings are in fact sufficient for instability. We also discuss flavor thermalization and energy conservation in relation to ergodicity.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-09-16
DOI
https://doi.org/10.1103/qd8x-29zm
Citations
3
Primary Topic
Neutrino Physics Research
Type
article
Field-Weighted Citation Impact
5.61
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article

Implications of conservation laws and ergodicity for neutrino flavor instability

Lucas Johns
3 citations
Physical review. D/Physical review. D.
Neutrino Physics Research
5.61
article

Implications of conservation laws and ergodicity for neutrino flavor instability

Lucas Johns
article en
3 citations

Abstract

Collective neutrino flavor instabilities are believed to be prevalent in core-collapse supernovae and neutron star mergers. This work establishes two points related to instability, both in the spirit of developing a more fundamental understanding of collective flavor dynamics. First, a conservation law related to the lepton number implies that spectral crossings are necessary for instability. Second, the most permissive application of the ergodic hypothesis to neutrino flavor evolution implies that spectral crossings are in fact sufficient for instability. We also discuss flavor thermalization and energy conservation in relation to ergodicity.

Physical review. D/Physical review. D.Vol. 112(6)
Los Alamos National Laboratory (US)
Openalex Percentile: Top 5%
Neutrino Physics Research
5.61
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