石中的129I和247Cm限制了太阳r过程元素的最后一个天体物理来源
Benoit Côté1,2,3, Marius Eichler4, Andrés Yagüe López5
1Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network, Konkoly Observatory, 1121 Budapest, Hungary. benoit.cote@csfk.org.
概括
石揭示了太阳系早期的组成. -129与-247在石中的比例表明中子星的合并通过快速中子捕获过程 (r过程) 产生了重元素.
科学领域:
- 宇宙化学和核天体物理学
- 研究太阳系中重元素的起源
背景情况:
- 石为太阳系早期的化学组成提供了关键的见解.
- 快速中子捕获过程 (r过程) 负责合成比铁更重的元素,但其天体物理位置仍然不确定.
研究的目的:
- 限制太阳系形成之前的最后一个r过程事件的天体物理位置.
- 用-129 (129I) 和-247 (247Cm) 在石中的保存比作为标记物.
主要方法:
- 在石中测量了129I/247Cm的比率.
- 将石比例与中子星合并和磁旋超新星模拟的核合成计算进行了比较.
- 利用129I和247Cm几乎相同的半衰期来保持它们的产量比率.
主要成果:
- 测量的129I/247Cm的流星比为438±184.
- 核合成计算表明中等中子丰富的条件最符合观察到的比率.
- 这些条件经常在中子星合并盘的喷射中模拟.
结论:
- 中子星的合并是早期太阳系中r过程元素的可能来源.
- 这项研究突显出石中同位素比例对于理解核合成的重要性.
- 目前核物理数据的不确定性限制了对这些结论的信心.
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