锡团Sn22的延迟光解离
Alexander Jankowski1, Paul Fischer1, Klavs Hansen2
1Institute for Physics, University of Greifswald, Felix-Hausdorff-Straße 6, 17498 Greifswald, Germany. alexander.jankowski@uni-greifswald.de.
Physical chemistry chemical physics : PCCP
|December 15, 2023
概括
调查锡团光解离的结果显示,Sn15-是主要的碎片. 这表明中性Sn7的损失,其确定的解离能量为2.1 eV,挑战了先前的计算.
科学领域:
- 物理化学 物理化学
- 材料科学 材料科学 材料科学
- 原子和分子物理 原子和分子物理
背景情况:
- 气相锡集群 (Snn-) 在材料科学中至关重要.
- 了解它们的稳定性和碎片化是预测材料性质的关键.
研究的目的:
- 为了研究Sn22星团的毫秒延迟光解离动态.
- 确定从Sn22-中中性Sn7的损失的离散能量.
主要方法:
- 在Penning陷中存储气相Sn22-集群.
- 在不同激发能量下进行毫秒延迟的光解离实验.
- 分析带电碎片的分布和衰变动力学.
主要成果:
- 确定Sn15-是唯一重要的带电碎片,表明中性Sn7部分的损失.
- 时间解析的碎片分析需要由于初始内部能量变化而需要分解常数的分布.
- 对Sn22- → Sn15- + Sn7的离散能量的下限被确定为2.1(1) eV.
结论:
- 确定的分离能量大约是现有量子化学计算预测的两倍.
- 这一发现凸显了对锡集群稳定性的精细理论模型的需求.
- 该研究提供了关键的实验数据,以了解锡集群碎片化途径.
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