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Neutrino Quantum Kinetic Equations: The Collision Term

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arxiv 1605.09383 v2 pith:PHQZ47TE submitted 2016-05-30 hep-ph astro-ph.COastro-ph.HE

Neutrino Quantum Kinetic Equations: The Collision Term

classification hep-ph astro-ph.COastro-ph.HE
keywords collisiontermslimitneutrinoscatteringstructuretermearly
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We derive the collision term relevant for neutrino quantum kinetic equations in the early universe and compact astrophysical objects, displaying its full matrix structure in both flavor and spin degrees of freedom. We include in our analysis neutrino-neutrino processes, scattering and annihilation with electrons and positrons, and neutrino scattering off nucleons (the latter in the low-density limit). After presenting the general structure of the collision terms, we take two instructive limiting cases. The one-flavor limit highlights the structure in helicity space and allows for a straightforward interpretation of the off-diagonal entries in terms of the product of scattering amplitudes of the two helicity states. The isotropic limit is relevant for studies of the early universe: in this case the terms involving spin coherence vanish and the collision term can be expressed in terms of two-dimensional integrals, suitable for computational implementation.

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Cited by 4 Pith papers

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

  1. Collective neutrino-antineutrino pair oscillations

    hep-ph 2026-04 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.

  2. Majoron Dark Energy via Freezing Induced by Quantum Coherence

    hep-ph 2026-07 conditional novelty 6.5

    Quantum coherence lag in a hidden pseudo-Dirac sterile reservoir can freeze a physical Majoron into a metastable w≈−1 phase even when m_φ ≫ H_0.

  3. Collective neutrino oscillations: Many-body non-forward effects and non-classicality

    hep-ph 2026-06 unverdicted novelty 5.0

    In a neutrino-gas model, the many-body Hamiltonian yields different evolution timescales and asymptotics than the quantum kinetic approach with collisions, while quantum resources for the full case sit at the low end ...

  4. Neutrino helicity oscillations in astrophysical environments: a many-body approach

    hep-ph 2026-05 unverdicted novelty 5.0

    Many-body neutrino calculations in simple momentum-state configurations yield helicity conversion probabilities orders of magnitude above mean-field results due to momentum exchange.