Wang Fan, Ziegler Tom
Department of Chemistry, University of Calgary, Calgary, Alberta T2N 1N4, Canada.
J Chem Phys. 2005 Oct 15;123(15):154102. doi: 10.1063/1.2061187.
In the present work we have proposed an approximate time-dependent density-functional theory (TDDFT) formalism to deal with the influence of spin-orbit coupling effect on the excitation energies for closed-shell systems. In this formalism scalar relativistic TDDFT calculations are first performed to determine the lowest single-group excited states and the spin-orbit coupling operator is applied to these single-group excited states to obtain the excitation energies with spin-orbit coupling effects included. The computational effort of the present method is much smaller than that of the two-component TDDFT formalism and this method can be applied to medium-size systems containing heavy elements. The compositions of the double-group excited states in terms of single-group singlet and triplet excited states are obtained automatically from the calculations. The calculated excitation energies based on the present formalism show that this formalism affords reasonable excitation energies for transitions not involving 5p and 6p orbitals. For transitions involving 5p orbitals, one can still obtain acceptable results for excitations with a small truncation error, while the formalism will fail for transitions involving 6p orbitals, especially 6p1/2 spinors.
在本工作中,我们提出了一种近似的含时密度泛函理论(TDDFT)形式体系,以处理自旋轨道耦合效应对闭壳层体系激发能的影响。在这种形式体系中,首先进行标量相对论TDDFT计算以确定最低的单重态激发态,然后将自旋轨道耦合算符应用于这些单重态激发态,以获得包含自旋轨道耦合效应的激发能。本方法的计算量比二分量TDDFT形式体系小得多,并且该方法可应用于包含重元素的中等规模体系。双重态激发态在单重态和三重态激发态方面的组成可从计算中自动获得。基于本形式体系计算得到的激发能表明,对于不涉及5p和6p轨道的跃迁,该形式体系能给出合理的激发能。对于涉及5p轨道的跃迁,在截断误差较小的情况下,仍能得到可接受的激发结果,而对于涉及6p轨道,特别是6p1/2旋量的跃迁,该形式体系将失效。