通过气相SiCH的单光子电离对SiCH+进行实验性表征
N L Chen1, B Gans1, S Boyé-Péronne1
1Université Paris-Saclay, CNRS, Institut des Sciences Moléculaires d'Orsay, F-91405 Orsay, France.
The Journal of chemical physics
|March 19, 2024
概括
研究人员通过实验测量了碳化离子 (SiCH+),这是一种在星际空间中预测但从未观察到的分子. 这项研究提供了使用先进的电离技术对SiCH+的第一个光谱见解.
科学领域:
- 天体化学是天体化学.
- 物理化学 物理化学
- 频谱学是一种光谱学.
背景情况:
- 碳化离子 (SiCH+) 是星际介质模型中预测的一种物种.
- 由于其内在的不稳定性,SiCH+仍然没有被观察到,这阻碍了光谱研究.
研究的目的:
- 提供第一个实验性光谱洞察 SiCH + 阴离子.
- 为了确定SiCH基的离子电离能.
主要方法:
- 在微波放电流管反应器中产生的SiCH基的单光子电离谱.
- 在SOLEIL同步仪上使用了一种双成像光电子/光离子巧合光谱仪.
- 在初始计算和弗兰克-康登模拟的支持下.
主要成果:
- 从SiCH+的基电子状态X2Π向SiCH+的X+3Σ-和A+3Π状态导出离子电离能.
- 报告的电离能为8.935(6) eV和10.664(6) eV (没有自旋轨道校正).
- 排除了HSiC同位素的贡献.
结论:
- 这项研究提出了SiCH+的第一个实验性表征.
- 导出的电离能对于在天文观测中识别SiCH+至关重要.
- 实验数据为未来星际化学模型提供了基础.
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