概括
圣克拉拉铁石中含有萨马-152,这表明在太阳系早期存在超重元素. 这限制了它们相对于-238.8的丰度.
科学领域:
- 宇宙化学 宇宙化学
- 核天体物理学 核天体物理学
- 行星科学 行星科学
背景情况:
- 早期太阳系的核合成过程尚未完全理解.
- 超重元素 (SHEs) 假设通过快速中子捕获 (r-过程) 或其他奇特的途径形成.
- 石为研究早期太阳系条件提供了至关重要的样本.
研究的目的:
- 在圣克拉拉铁石中调查-152 (152Sm) 的起源.
- 为了限制太阳系早期假设的超重元素的丰富性.
主要方法:
- 在圣克拉拉铁石中对-152丰富性的定量分析.
- 建模超重元素裂变对152Sm产生的贡献.
- 基于观察到的152Sm水平计算超重元素丰度的上限.
主要成果:
- 萨马-152的丰富性被确定为每克108×107个原子.
- 如果归因于超重元素 (原子号107-109) 的裂变,它们的丰度相对于-238.8而言仅限于1.7×10−5.
- 对于元素110,相对于-238.8的丰度极限是3.4×10−5.
结论:
- 圣克拉拉石中152Sm的存在对早期太阳系中超重元素的丰富性产生了重大限制.
- 这些发现表明,超重元素,如果它们存在,不会在足够的数量中产生,成为某些同位素的主要来源.
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