R-Process Nucleosynthesis in Core-Collapse Supernova Explosion
天体物理学
2015-06-24 v1
摘要
We study the r-process nucleosynthesis in neutrino-driven winds of gravitational core collapse SNeII. Appropriate physical conditions are found for successful r-process nucleosynthesis, which meet with several features of heavy elements discovered recently in metal-deficient halo stars. We find also several difficulties which are not explained in the present wind models. We discuss quests for new insights in nuclear physics, astrophysics, and astronomy.
引用
@article{arxiv.astro-ph/0111403,
title = {R-Process Nucleosynthesis in Core-Collapse Supernova Explosion},
author = {T. Kajino and S. Wanajo and G. J. Mathews},
journal= {arXiv preprint arXiv:astro-ph/0111403},
year = {2015}
}
备注
14 pages, 6 figures, Nuclear Physics A, in press