Shell and explosive hydrogen burning Nuclear reaction rates for hydrogen burning in RGB, AGB and Novae
Shell and explosive hydrogen burning Nuclear reaction rates for hydrogen burning in RGB, AGB and Novae
复制标题
壳牌和爆炸性氢燃烧 RGB、AGB 和 Novae 中氢燃烧的核反应速率
DOI：
10.1140/epja/i2016-16075-4
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发表时间：
2016
期刊：
影响因子：
--
通讯作者：
Boeltzig A
中科院分区：
文献类型：
--
作者：
Boeltzig A
轻元素的核合成，从氦到硅，主要发生在红巨星和渐近巨星分支恒星和新星。合成核素的相对丰度主要取决于所涉及的核过程的速率，通常是通过不平凡的反应链，结合复杂的混合机制。在本文中，我们总结了LUNA实验在进一步了解AGB恒星和新星爆炸中核合成建模所需的核反应速率方面所做的贡献。
The nucleosynthesis of light elements, from helium up to silicon, mainly occurs in Red Giant and Asymptotic Giant Branch stars and Novae. The relative abundances of the synthesized nuclides critically depend on the rates of the nuclear processes involved, often through non-trivial reaction chains, combined with complex mixing mechanisms. In this paper, we summarize the contributions made by LUNA experiments in furthering our understanding of nuclear reaction rates necessary for modeling nucleosynthesis in AGB stars and Novae explosions.