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Symmetry and bipolar motion in collective neutrino flavor oscillations

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arxiv 2303.05906 v2 pith:MO54GV6K submitted 2023-03-10 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords flavorsymmetrybipolarcollectiveevolutionmotionneutrinooscillations
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We identify a geometric symmetry on the two-flavor Bloch sphere for collective flavor oscillations of a homogeneous dense neutrino gas. Based on this symmetry, analytical solutions to the periodic bipolar flavor evolution are derived. Using numerical calculations, we show that for configurations without this symmetry, the flavor evolution displays deviations from the bipolar flavor motion or even exhibits aperiodic patterns. We also discuss the implication of our finding for more general three-flavor and inhomogeneous cases.

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Cited by 3 Pith papers

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

  1. Advection Algorithms for Quantum Neutrino Moment Transport

    astro-ph.HE 2025-01 conditional novelty 7.0 of 10

    A modulus-phase Riemann solver for quantum neutrino moments gives fast-flavor instability growth rates and wavenumbers closer to multi-angle simulations than the prior real-imaginary implementation.

  2. 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.

  3. Flavor Equilibration of Supernova Neutrinos: Exploring the Dynamics of Slow Modes

    astro-ph.HE 2025-05 conditional novelty 6.0 of 10

    Slow flavor conversion drives supernova neutrinos to a coarse-grained flavor-equilibrated state within a few inverse vacuum frequencies, with survival probabilities set by the neutrino-antineutrino density ratio alone.

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