中文

稠密介质中的中微子-中微子相互作用与味道混合

天体物理学 2008-11-26 v2 高能物理 - 唯象学 核理论

摘要

presented an algebraic approach to the neutrino propagation in dense media. 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.

引用

@article{arxiv.astro-ph/0607527,
  title  = {Neutrino-Neutrino Interactions and Flavor Mixing in Dense Matter},
  author = {A. B. Balantekin and Y. Pehlivan},
  journal= {arXiv preprint arXiv:astro-ph/0607527},
  year   = {2008}
}

备注

16 pages of REVTEX