一个ab initio糖尿病研究的CN的罗维慢性光谱的CN
Shuai Zhang1, Zhi Qin1, Linhua Liu1
1School of Energy and Power Engineering, Shandong University, Jinan, Shandong, 250061, China. liulinhua@sdu.edu.cn.
本研究提供了对基 (CN) 的罗维布朗基光谱的全面初始计算. 结果为行星探索应用提供了精确的吸收截面.
科学领域:
- 计算化学计算化学
- 分子光谱学 分子光谱学
- 量子化学 是一个量子化学.
背景情况:
- 基 (CN) 是天体化学和燃烧过程中至关重要的分子.
- 在解释实验观测和建模复杂化学系统方面,准确的理论数据对CN的罗维波朗谱是必不可少的.
研究的目的:
- 通过使用糖尿病表示方法,对蓝色基 (CN) 的罗维布朗基光谱进行初始研究.
- 为了在行星探索中的潜在应用,在广泛的波数范围内提供精确的吸收截面.
主要方法:
- 使用了内部合约的多引用配置交互方法,包括戴维森校正 (icMRCI + Q) 与 aug-cc-pwCV5Z-DK 基础集.
- 采用基于属性的diabatization方法来处理电子状态之间的避免交叉.
- 解决了合的核运动施罗丁格方程,以获得罗维布朗谱.
主要成果:
- 从0到80,000厘米-1的CN计算的罗维龙谱,考虑了17个电子状态.
- 与 30,000 cm-1以下的吸收截面的理论数据达成良好一致.
- 由于包含高层电子状态,观察到超过30,000厘米的更大的截面-1.
结论:
- 这项工作提供了对CN的罗维龙频谱的全面预测.
- 结果适用于低于8000K的温度,适用于行星探索研究.
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