arXiv · astro-ph/0607527
Neutrino-Neutrino Interactions and Flavor Mixing in Dense Matter
Abstract
An algebraic approach to the neutrino propagation in dense media is presented. The Hamiltonian describing a gas of neutrinos interacting with each other and with background fermions is written in terms of the appropriate SU(N) operators, where N is the number of neutrino flavors. The evolution of the resulting many-body problem is formulated as a coherent-state path integral. Some commonly used approximations are shown to represent the saddle-point solution of the path integral for the full many-body system.
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A. B. Balantekin, Y. Pehlivan. 2006-10-19. Neutrino-Neutrino Interactions and Flavor Mixing in Dense Matter. https://doi.org/10.1088/0954-3899%2F34%2F1%2F004
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