Response to Comments on ” NEUTRINO FLAVOR EVOLUTION NEAR A SUPERNOVA ’ S CORE ”

@inproceedings{Pantaleone1994ResponseTC,
  title={Response to Comments on ” NEUTRINO FLAVOR EVOLUTION NEAR A SUPERNOVA ’ S CORE ”},
  author={Jim Pantaleone},
  year={1994}
}
In supernovae and in the early universe, neutrino flavor evolution is a many-body phenomena. Here the equations describing the evolution of the density matrices in phase space are derived. Then these equations are applied to neutrino emission from a supernova core. The effects of a 'small' background neutrino density on adiabatic and nonadiabatic flavor evolution 

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