Abstract

It has been realized that the shock wave propagation can produce interesting effects in the energy and time structure of the supernova (SN) neutrino signal. In the standard three-neutrino oscillation scenario, such effects crucially depend on the electron (anti)neutrino survival probability. The aim of this talk is to show that simple analytical approximations can replace numerical calculations of the survival probability for all practical purposes. Illustrative applications are also given, in terms of the positron spectra generated by SN electron antineutrinos through inverse beta decay.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call