中子星合并GW170817/SSS17a的光曲线:对r过程核合成的影响
M R Drout1, A L Piro2, B J Shappee2,3
1The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA. mdrout@carnegiescience.edu.
概括
像GW170817这样的双中子恒星的合并产生了重元素. 来自GW170817的观测光线表明,这些宇宙事件对于快速的中子捕获 (r过程) 核合成至关重要.
科学领域:
- 天文学与天体物理学
- 核天体物理学
背景情况:
- 2017年8月17日,从一个双中子星合并 (GW170817) 中发现了引力波.
- 一个短的马射线爆发 (GRB 170817A) 和一个光学瞬态 (SSS17a) 与GW事件相吻合.
研究的目的:
- 分析光学短变SSS17a的紫外线,光学和红外线光曲线.
- 了解核聚变中的富含中子的放射性物质.
- 确定中子星合并对重元素合成的贡献.
主要方法:
- 从合并后的10.9小时到18天内对SSS17a的光曲线进行观察和分析.
- 模拟射出物质的放射性衰变
- 限制了喷射物中的化物.
主要成果:
- 光线曲线呈现出快速的升降,衰落和快速的色彩演变,
- 根据光线曲线的特征推断出化物存在.
- 至少有0.05太阳质量的重元素是由SSS17a产生的.
结论:
- 中子星的合并是生产重元素的重要场所.
- 观察到的GW170817事件证实了中子星合并在快速中子捕获 (r过程) 核合成中的作用.
- 这项研究为这些宇宙事件中重元素的合成提供了观察证据.
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