反应的实验速率常数S+D) +H2反应的实验速率常数
Alexandre Zanchet1, Jia Lei Chen-Qiu2,1, Pascal Larregaray3
1Instituto de Física Fundamental, CSIC, Serrano 123, Madrid 28006, Spain.
概括
硫酸 (S+) 的电子激发可以显著增强星际环境中SH+的产生. 这项研究通过实验测量反应截面以确定速率常数,揭示了星际化学的新途径.
科学领域:
- 天体化学是天体化学.
- 化学物理 化学物理
- 星际介质 星际介质
背景情况:
- 在星际介质 (ISM) 中,内热反应通常是微不足道的.
- 光子主导区域 (PDR) 的紫外线辐射可以克服内热性,提高反应速率.
- 以前的研究表明,对H2的振动激发增强了C+和S+与H2的反应性.
研究的目的:
- 研究硫酸盐 (S+) 的电子激发如何增强SH+的产生.
- 在各种碰撞能量下实验测量S++H2的反应截面.
- 将实验结果与理论预测进行比较,并得出温度依赖的速率常数.
主要方法:
- 实验测量S++H2的反应截面,从50 meV到几 eV.
- 实验数据与理论预测在0.0013 eV范围内进行比较.
- 从测量过的横截面推导速率常数,用于广泛的温度谱.
主要成果:
- 对S+的电子激发显著增强了SH+的产生.
- 获得实验横截面,并与理论模型进行比较.
- 导出了速率常数,适用于ISM相关的广泛温度范围.
结论:
- 硫酸的电子激发是PDR中SH+形成的关键因素.
- 这些发现为了解星际硫化学提供了关键数据.
- 这项研究扩大了对星际介质中紫外线驱动反应的知识.
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