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arxiv: astro-ph/0607527 · v2 · submitted 2006-07-23 · 🌌 astro-ph · hep-ph· nucl-th

Neutrino-Neutrino Interactions and Flavor Mixing in Dense Matter

classification 🌌 astro-ph hep-phnucl-th
keywords denseintegralmany-bodyneutrinopathalgebraicapproachappropriate
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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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    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 ...