R-Process Nucleosynthesis in Core-Collapse Supernova Explosion

T. Kajino; S. Wanajo; G. J. Mathews

doi:10.1016/s0375-9474(02)00777-7

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arXiv · astro-ph/0111403

R-Process Nucleosynthesis in Core-Collapse Supernova Explosion

T. Kajino·S. Wanajo·G. J. Mathews

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Abstract

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.

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T. Kajino, S. Wanajo, G. J. Mathews. 2001-11-21. R-Process Nucleosynthesis in Core-Collapse Supernova Explosion. https://doi.org/10.1016/s0375-9474(02)00777-7

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