Neutrino Nucleosynthesis
A. Heger, E. Kolbe, W. C. Haxton, K. Langanke, G. Martinez-Pinedo, S. E. Woosley
Abstract
We study neutrino process nucleosynthesis in massive stars using newly calculated cross sections, an expanded reaction network, and complete and self-consistent models of the progenitor star. We reevaluate the production of light isotopes from abundant progenitors as well as that of rare, heavy, proton-rich isotopes. In particular, new results are given for B11, F19, La138, and Ta180. The production of these isotopes places limits on neutrino spectrum and oscialltions.
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