Neutrino transport in supernova shock fronts.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Supernovae: Neutrinos, Supernovae: Shock Waves

Scientific paper

The author has developed a numerical code for treating the transport of neutrinos in the shock wave of a supernova explosion propagating through the stellar matter. The Boltzmann transport equation and its first two angular moments are solved iteratively in order to give the exact solution of the transport problem including the angular distribution of the intensity. Some results of calculations using a background model with a moving shock front are presented.

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