nu-Process Nucleosynthesis in Population III Core-Collapse Supernovae
Abstract
We investigate the effects of neutrino-nucleus interactions (the nu-process) on the production of iron-peak elements in Population III core-collapse supernovae. The nu-process and the following proton and neutron capture reactions produce odd-Z iron-peak elements in complete and incomplete Si burning region. This reaction sequence enhances the abundances of Sc, Mn, and Co in the supernova ejecta. The supernova explosion models of 15 M_sol and 25 M_sol stars with the nu-process well reproduce the averaged Mn/Fe ratio observed in extremely metal-poor halo stars. In order to reproduce the observed Mn/Fe ratio, the total neutrino energy in the supernovae should be 3 - 9 x 10^{53} ergs. Stronger neutrino irradiation and other production sites are necessary to reproduce the observed Sc/Fe and Co/Fe ratios, although these ratios increase by the nu-process.
Cite
@article{arxiv.0710.0251,
title = {nu-Process Nucleosynthesis in Population III Core-Collapse Supernovae},
author = {Takashi Yoshida and Hideyuki Umeda and Ken'ichi Nomoto},
journal= {arXiv preprint arXiv:0710.0251},
year = {2009}
}
Comments
10 pages, 12 figures, Accepted for publication in The Astrophysical Journal