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Single-wave solutions of the neutrino fast flavor system. Part I. Mechanical properties

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

A dense neutrino plasma can exhibit collective flavor evolution caused by neutrino--neutrino refraction. Recently, a new class of exact nonlinear inhomogeneous solutions was discovered: single-wave (SW) solutions of the fast flavor system. The key property is that the flavor occupation numbers remain homogeneous, whereas the field of flavor coherence varies spatially with a single wave vector. The equations of motion for this structure resemble those of a collection of classical spins, in analogy with the homogeneous slow and fast flavor cases. In contrast, the SW system is not integrable (it does not possess Gaudin invariants) so that, while two-beam pendulum solutions are inevitable, they do not extend to a multi-angle system. We develop a taxonomy of all known nonlinear collective flavor solutions, explaining the overlap between categories and their differences.

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fields

hep-ph 2

years

2026 2

verdicts

UNVERDICTED 2

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background 1

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background 1

representative citing papers

Neutrino-antineutrino superfluidity

hep-ph · 2026-05-26 · unverdicted · novelty 7.0

Pairing instabilities in neutrino plasmas arise only with occupation number discontinuities and are spurious artifacts of energy discretization that disappear in the continuum.

Collective neutrino-antineutrino pair oscillations

hep-ph · 2026-04-28 · unverdicted · novelty 7.0

In anisotropic neutrino gases, νν-bar pairing instabilities emerge when the excessive pair-occupation number distribution changes sign, producing pair conversions at growth rates comparable to fast flavor instabilities.

citing papers explorer

Showing 2 of 2 citing papers.

  • Neutrino-antineutrino superfluidity hep-ph · 2026-05-26 · unverdicted · none · ref 48 · internal anchor

    Pairing instabilities in neutrino plasmas arise only with occupation number discontinuities and are spurious artifacts of energy discretization that disappear in the continuum.

  • Collective neutrino-antineutrino pair oscillations hep-ph · 2026-04-28 · unverdicted · none · ref 100 · internal anchor

    In anisotropic neutrino gases, νν-bar pairing instabilities emerge when the excessive pair-occupation number distribution changes sign, producing pair conversions at growth rates comparable to fast flavor instabilities.