College of Physics and Electronic Engineering, Henan Normal University, Xinxiang 453007, China.
Spectrochim Acta A Mol Biomol Spectrosc. 2013 Nov;115:259-68. doi: 10.1016/j.saa.2013.06.038. Epub 2013 Jun 19.
The potential energy curves (PECs) of eleven Ω states generated from the seven Λ-S bound states of SiH radical are studied in detail using an ab initio quantum chemical method. The PECs are calculated for internuclear separations from about 0.10 to 1.00nm by the CASSCF method, which is followed by the internally contracted MRCI approach with the Davidson modification. The spin-orbit coupling is accounted for with the Breit-Pauli Hamiltonian. Core-valence correlation corrections are included with an aug-cc-pCVTZ basis set. Scalar relativistic correction calculations are made by the third-order Douglas-Kroll Hamiltonian approximation at the level of a cc-pV5Z basis set. To discuss the effect of core-electron correlations on the spectroscopic parameters, in particular on the Te, the all-electron basis set, aug-cc-pCVTZ with and without core-electron correlations, is employed to calculate the spin-orbit coupling splitting in the X(2)Π Λ-S state. The all-electron aug-cc-pCVTZ basis set with core-electron correlations is chosen for the present spin-orbit coupling studies. The convergent behavior of present calculations is discussed with respect to the basis set and level of theory. All the PECs are extrapolated to the complete basis set limit. The spectroscopic parameters of seven Λ-S and eleven Ω bound states are evaluated. The splitting energy of X(2)Π Λ-S state is determined as 141.12cm(-1), which agrees well with the recent measurements of 142.896cm(-1). Moreover, other spectroscopic parameters are also in excellent agreement with available measurements. It demonstrates that the spectroscopic parameters of eleven Ω bound states reported here can be expected to be reliable predicted ones.
使用从头算量子化学方法详细研究了 SiH 自由基的七个 Λ-S 束缚态生成的十一个 Ω 态的势能曲线(PECs)。通过 CASSCF 方法计算了核间距约为 0.10 到 1.00nm 的 PEC,随后采用 Davidson 修正的内收缩 MRCI 方法进行计算。自旋轨道耦合通过 Breit-Pauli 哈密顿量来描述。考虑了芯电子相关修正,采用 aug-cc-pCVTZ 基组。采用第三阶 Douglas-Kroll 哈密顿近似在 cc-pV5Z 基组的水平上进行标量相对论修正计算。为了讨论芯电子相关对光谱参数的影响,特别是对 Te 的影响,采用全电子基组 aug-cc-pCVTZ 及其不带芯电子相关的形式,计算了 X(2)Π Λ-S 态的自旋轨道耦合分裂。对于目前的自旋轨道耦合研究,选择了带有芯电子相关的全电子 aug-cc-pCVTZ 基组。讨论了不同基组和理论水平下的收敛行为。所有的 PEC 都被外推到完全基组极限。评估了七个 Λ-S 和十一个 Ω 束缚态的光谱参数。X(2)Π Λ-S 态的分裂能确定为 141.12cm(-1),与最近的测量值 142.896cm(-1)吻合较好。此外,其他光谱参数也与现有测量值非常吻合。这表明,本文报道的十一个 Ω 束缚态的光谱参数可以预期是可靠的预测值。