恒星中的元素丰富性模式表明核的分裂比更重
Ian U Roederer1, Nicole Vassh2, Erika M Holmbeck3
1Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA.
概括
快速中子捕获过程 (r过程) 产生了重元素. 这项研究表明,跨原子核的裂变碎片有助于元素的丰富性,表明在r过程中产生了超过260质量的中子丰富的原子核.
科学领域:
- 核天体物理学
- 宇宙化学
背景情况:
- 最重的元素是通过快速的中子捕获过程 (r过程) 形成的,这种过程是在中子星的合并过程中发生的.
- 由于实验的局限性,了解重于的元素 (超核) 的 r-过程生产是具有挑战性的,需要依赖理论核合成模型.
研究的目的:
- 研究超核裂变碎片对恒星中观察到的r过程元素的贡献.
- 确定特定元素的丰度相关性,可以作为裂变碎片贡献的证据.
主要方法:
- 用r过程元素丰富的恒星中的元素丰度的分析.
- 对元素丰度的统计相关性分析,重点是特定的质量和原子数范围.
主要成果:
- 在,,和银 (Z=44-47) 和更重的元素 (Z=63-78) 之间发现了显著的相关性.
- 对邻近元素 (Z=34-42和Z=48-62) 没有观察到这种相关性.
- 这些相关性支持的假设是,跨原子核的裂变碎片在r过程核合成中起作用.
结论:
- 观察到的丰度模式提供了证据,证明跨原子核的裂变碎片对r过程元素库存的贡献.
- 这些发现表明,在r过程中合成的质量超过260的中子丰富的核.
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