TL;DR
This paper reviews the theoretical frameworks used to describe neutrino flavor evolution in astrophysical and cosmological environments, highlighting their derivation methods and observational relevance.
Contribution
It provides a comprehensive summary of the mean-field, extended mean-field, and Boltzmann equations used for neutrino propagation modeling.
Findings
Summarizes key features of neutrino evolution equations.
Highlights methods for deriving these equations.
Discusses applications to observational scenarios.
Abstract
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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