具有天体物理意义的MgC4H激素的能量和光谱性质使用高水平Ab Initio计算
Tarun Roy1, Sayon Satpati1, Aland Sinjari2,3
1Department of Chemistry, National Institute of Technology Durgapur, M G Avenue, Durgapur, West Bengal 713209, India.
The journal of physical chemistry. A
|February 16, 2024
概括
含的碳化合物分子在富含碳的环境中至关重要. 计算方法确定MgC4H的线性同位素是最稳定的,与实验室和天文观测结果相匹配.
科学领域:
- 天体化学是天体化学.
- 计算化学计算化学
- 量子化学 是一个量子化学.
背景情况:
- 含的碳化合物分子 (MgCHn) 在富含碳的环恒星外中很重要,例如IRC+10216.
- 了解它们的结构和稳定性是理解星际化学的关键.
研究的目的:
- 理论上研究四碳水化合物 (MgC4H) 的组成异构体.
- 为了确定最稳定的同位素及其特性,以便进行潜在的天文检测.
主要方法:
- 用密度函数理论 (DFT) 和合集群方法进行理论计算.
- 使用 ROCCSD ((T) /cc-pCVTZ用于相对能量测定和CASPT2用于多参考系统.
主要成果:
- 确定了28种MgC4H的组成异构体,其中线性1-magnesapent-2,4-diyn-1-yl异构体是全球最小的.
- 全球最小值的计算光谱数据与实验观测结果非常接近 (误差≤0.78%).
- 第二个最稳定的异构体,1-乙烯基-1λ3-magnesacycloprop-2-ene-2,3-diyl,是能量可访问的.
结论:
- 理论方法通过全球最低值计算和实验数据之间的协议来验证.
- 线性MgC4H同位素被证实是星际环境中的关键分子.
- 第二个最稳定的同位素是未来实验室和星际介质检测的有希望的目标.
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