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改进的状态特定多参考微扰理论中的虚拟轨道,用于拟简并电子结构的原型。

Improved virtual orbitals in state specific multireference perturbation theory for prototypes of quasidegenerate electronic structure.

机构信息

Department of Chemistry, Indian Institute of Engineering Science and Technology, Shibpur, Howrah 711103, India.

Department of Chemistry, Jhargram Raj College, Jhargram 721507, India.

出版信息

J Chem Phys. 2017 Feb 14;146(6):064111. doi: 10.1063/1.4975322.

Abstract

The state-specific multireference perturbation theory (SSMRPT) with an improved virtual orbital complete active space configuration interaction (IVO-CASCI) reference function [called as IVO-SSMRPT] is used to investigate the energy surface, geometrical parameters, molecular properties of spectroscopic interest for the systems/situations [such as BeH, BeCH, MgCH, SiH, unimolecular dissociation of HCO, and intramolecular reaction pathways of 1,3-butadiene] where the effect of quasidegeneracy cannot be neglected. The merit of using the IVO-CASCI rather than complete active space self-consistent field (CASSCF) is that it is free from iterations beyond those in the initial SCF calculation and the convergence difficulties that plague CASSCF calculations with increasing size of the CAS. While IVO-CASCI describes the non-dynamical correlation, the SSMRPT scheme is a good second-order perturbative approximation to account for the rest of the correlation energy. Our IVO-SSMRPT method is instrumental in avoiding intruder states in an size-extensive manner and allows the revision of the content of wave function in the model space. It can treat model as well as real systems with predictive accuracy, as is evident from the fairly nice accordance between our estimates, and high-level theoretical results. Our estimates also corroborate well with some experimental findings.

摘要

采用改进的虚拟轨道全活性空间组态相互作用(IVO-CASCI)参考函数(称为IVO-SSMRPT)的状态特定多参考微扰理论(SSMRPT),用于研究具有准简并效应的体系/情况(如 BeH、BeCH、MgCH、SiH、HCO 的单分子离解和 1,3-丁二烯的分子内反应途径)的能量表面、几何参数和分子性质。使用IVO-CASCI 而不是全活性空间自洽场(CASSCF)的优点是,它不受初始 SCF 计算之外的迭代和随着 CAS 大小增加而困扰 CASSCF 计算的收敛困难的影响。虽然 IVO-CASCI 描述了非动力学相关,但 SSMRPT 方案是一个很好的二阶微扰近似,可以计算其余的相关能量。我们的 IVO-SSMRPT 方法有助于以扩展性的方式避免侵入态,并允许在模型空间中修改波函数的内容。它可以以预测精度处理模型和真实系统,从我们的估计与高级理论结果之间相当好的一致性可以明显看出。我们的估计也与一些实验结果很好地吻合。

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