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arXiv · astro-ph/0307546

Neutrino Nucleosynthesis

A. Heger·E. Kolbe·W. C. Haxton·K. Langanke·G. Martinez-Pinedo·S. E. Woosley
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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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A. Heger, E. Kolbe, W. C. Haxton, K. Langanke, G. Martinez-Pinedo, S. E. Woosley. 2003-07-31. Neutrino Nucleosynthesis. https://doi.org/10.1016/j.physletb.2004.12.017

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