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Neutrino Quantum Kinetic Equations

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arxiv 1506.06222 v1 pith:2ZEGJ5F5 submitted 2015-06-20 astro-ph.SR hep-phnucl-th

Neutrino Quantum Kinetic Equations

classification astro-ph.SR hep-phnucl-th
keywords equationsmean-fieldneutrinoapplicationsastrophysicalboltzmanncosmologicalderive
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Neutrinos propagate in astrophysical and cosmological environments modifying their flavor in intriguing ways. The study of neutrino propagation in media is based on the mean-field, extended mean-field and Boltzmann equations. We summarise salient features of these evolution equations and the methods employed so far to derive them. We emphasize applications to situations of observational interest.

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Cited by 1 Pith paper

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  1. 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 ...