Supernova neutrinos: Flavor-dependent fluxes and spectra

Details Supernova neutrinos: Flavor-dependent fluxes and spectra Supernova neutrinos: Flavor-dependent fluxes and spectra

2003-03-11

arxiv.org/abs/astro-ph/0303226v1

Astronomy and Astrophysics

Astrophysics

Proceedings NOON 03, Kanazawa, 10-14 Feb 2003

Scientific paper

Transporting nu_mu and nu_tau in a supernova (SN) core involves several processes that have been neglected in traditional simulations. Based on a Monte Carlo study we find that the flavor-dependent spectral differences are much smaller than is often stated in the literature. A full-scale SN simulation using a Boltzmann solver and including all relevant neutrino reactions confirms these results. The flavor-dependent flux differences are largest during the initial accretion phase.

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