Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-11-06
New J.Phys. 7 (2005) 51
Astronomy and Astrophysics
Astrophysics
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.
Baha Balantekin A.
Yuksel Hasan
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