The Nucleosynthesis of the Light Elements C to Al by Core Collapse Supernovae

Publications of the Astronomical Society of Australia

Alessandro Chieffi¹ 

[1] Marco Limongi

关键词: nuclear reactions;    nucleosynthesis;    abundances;    stars: evolution;    stars: interiors;    supernovae: general;   

DOI  :  10.1071/AS03033

学科分类：天文学(综合)

来源: CSIRO

【 摘 要 】

We discuss the production sites of the nuclei from C to Al in solar metallicity stars in the range 13–35 M⊙. We will show how, contrary to current beliefs, the advanced burning phases and the passage of the blast wave play a pivotal role in determining the final yields of quite a few ‘light’ nuclei. We will also show how the relative contributions of the hydrostatic and explosive burning depend on the initial mass of the star: the smaller the mass the larger the importance of the explosive burning.

【 授权许可】

Unknown