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Fast Neutrino Flavor Conversion: Collective Motion vs. Decoherence

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arxiv 1906.08794 v3 pith:IGROYJZB submitted 2019-06-20 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords collectiveflavormodesnon-collectivedecoherencefastmodeneutrino
verification ladder T0 review T1 audit T2 compute T3 formal
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In an interacting neutrino gas, flavor coherence becomes dynamical and can propagate as a collective mode. In particular, tachyonic instabilities can appear, leading to "fast flavor conversion" that is independent of neutrino masses and mixing angles. On the other hand, without neutrino-neutrino interaction, a prepared wave packet of flavor coherence simply dissipates by kinematical decoherence of infinitely many non-collective modes. We reexamine the dispersion relation for fast flavor modes and show that for any wavenumber,there exists a continuum of non-collective modes besides a few discrete collective ones. So for any initial wave packet, both decoherence and collective motion occurs, although the latter typically dominates for a sufficiently dense gas. We derive explicit eigenfunctions for both collective and non-collective modes. If the angular mode distribution of electron-lepton number crosses between positive and negative values, two non-collective modes can merge to become a tachyonic collective mode. We explicitly calculate the interaction strength for this critical point. As a corollary we find that a single crossing always leads to a tachyonic instability. For an even number of crossings, no instability needs to occur.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Neutrino quantum kinetics for fast flavor conversion in a time-dependent environment

    astro-ph.HE 2026-08 unverdicted novelty 6.0 of 10

    Fast flavor conversion in a time-varying supernova background proceeds through three episodes and broadly agrees with static two-step model results.

  2. Fast Flavor Pendulum: Instability Condition

    hep-ph 2024-12 conditional novelty 6.0 of 10

    The Nyquist criterion for homogeneous fast flavor instability is corrected to N = W - Ns/2, where W is the subluminal winding number and Ns counts real superluminal solutions.

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