Egorov Oleg, Rey Michaël, Nikitin Andrei V, Viglaska Dominika
Laboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics SB RAS 1, Akademician Zuev Sq., Tomsk 634055 Russia.
Groupe de Spectrométrie Moléculaire et Atmosphérique UMR CNRS 7331, UFR Sciences BP 1039, 51687 Reims Cedex 2, France.
J Phys Chem A. 2022 Sep 22;126(37):6429-6442. doi: 10.1021/acs.jpca.2c04822. Epub 2022 Sep 7.
In the present work, high-level ab initio calculations were carried out for the ground electronic state of the methyl radical (CH). Dunning's augmented correlation-consistent orbital basis sets were employed up to the quintuple-ζ valence quality with the core-valence electron correlation [aug-cc-pCV5Z] combined with the single- and double-excitation unrestricted coupled-cluster approach with a perturbative treatment of triple excitations [RHF-UCCSD(T)]. The explicitly correlated version of the coupled-cluster approach [RHF-UCCSD(T)-F12x{x = a, b}] was additionally applied with the core-valence cc-pCVQZ-F12 basis set in order to study convergence with respect to the basis set size. The contributions beyond the coupled-cluster level of the theory like Douglas-Kroll-Hess scalar relativistic Hamiltonian, diabatic Born-Oppenheimer corrections, and high-order electronic correlations have been included into the ab initio potential energy surfaces (PESs). It is shown that the theoretical band origins of CH converge gradually to the experimental values when applying the ab initio PESs using the aug-cc-pCVXZ [X = T, Q, and 5] basis sets. For the first time, all available experimental band origins of the gaseous CH are reproduced within an accuracy of 0.2 cm using a newly developed PES extrapolated to the complete basis set limit [CBS(TQ5Z)]. The reached accuracy is one order of magnitude better than that of the best available calculations. A new theoretical infrared line list was generated for astrophysical applications using an ab initio dipole moment surface computed at the RHF-UCCSD(T)/aug-cc-pCVQZ level of the theory. The manifestation of a large-amplitude motion in CH is also discussed.
在本工作中,对甲基自由基(CH)的基态电子态进行了高水平的从头算计算。采用了邓宁的增强相关一致轨道基组,直至具有芯价电子相关的五重ζ价质量[aug-cc-pCV5Z],并结合单双激发无限制耦合簇方法及三重激发的微扰处理[RHF-UCCSD(T)]。此外,还应用了耦合簇方法的显式相关版本[RHF-UCCSD(T)-F12x{x = a, b}],并使用芯价cc-pCVQZ-F12基组来研究基组大小的收敛性。理论中超出耦合簇水平的贡献,如道格拉斯-克罗尔-赫斯标量相对论哈密顿量、非绝热玻恩-奥本海默修正和高阶电子相关,都已包含在从头算势能面(PES)中。结果表明,当使用aug-cc-pCVXZ[X = T、Q和5]基组应用从头算PES时,CH的理论带起源逐渐收敛到实验值。首次使用外推到完全基组极限[CBS(TQ5Z)]的新开发的PES,在0.2 cm的精度内再现了气态CH的所有可用实验带起源。达到的精度比现有最佳计算结果好一个数量级。利用在RHF-UCCSD(T)/aug-cc-pCVQZ理论水平计算的从头算偶极矩面,生成了一个用于天体物理应用的新理论红外谱线列表。还讨论了CH中大振幅运动的表现。