Neutrino Mixing and Nucleosynthesis in Core-Collapse Supernovae

Astronomy and Astrophysics – Astrophysics

Scientific paper

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17 pages, 4 figures

Scientific paper

10.1088/1367-2630/7/1/051

A simple description of core-collapse supernovae is given. Properties of the neutrino-driven wind, neutrino fluxes and luminosities, reaction rates, and the equilibrium electron fraction in supernova environments are discussed. Neutrino mixing and neutrino interactions that are relevant to core-collapse supernovae are briefly reviewed. The values of electron fraction under several evolution scenarios that may impact rapid neutron capture process (r-process) nucleosynthesis are calculated.

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