http://arxiv.org/abs/1506.06222
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.
C. Volpe
Tue, 23 Jun 15
17/67
Comments: 19 pages, 1 figure, review for the special issue “Collective motion in nuclei, neutrinos, and neutron stars”
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