Harnessing the meta-generalized gradient approximation for time-dependent density functional theory

被引:108
|
作者
Bates, Jefferson E. [1 ]
Furche, Filipp [1 ]
机构
[1] Univ Calif Irvine, Dept Chem, Irvine, CA 92697 USA
来源
JOURNAL OF CHEMICAL PHYSICS | 2012年 / 137卷 / 16期
基金
美国国家科学基金会;
关键词
SHIELDING CONSTANTS; EXCITATION-ENERGIES; EXCITED-STATES; BASIS-SETS; EXCHANGE; ATOMS; THERMOCHEMISTRY; EQUATIONS; SYSTEMS; MODEL;
D O I
10.1063/1.4759080
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
Density functionals within the meta-generalized gradient approximation (MGGA) are widely used for ground-state electronic structure calculations. However, the gauge variance of the kinetic energy density tau confounds applications of MGGAs to time-dependent systems, excited states, magnetic properties, and states with strong spin-orbit coupling. Becke and Tao used the paramagnetic current density to construct a gauge invariant generalized kinetic energy density (tau) over cap. We show that tau(W) <= (tau) over cap where tau(W) is the von Weizsacker kinetic energy density of a one-electron system. Thus, replacing tau by (tau) over cap leads to current-dependent MGGAs (cMGGAs) that are not only gauge invariant but also restore the accuracy of MGGAs in iso-orbital regions for time-dependent and current-carrying states. The current dependence of cMGGAs produces a vector exchange-correlation (XC) potential in the time-dependent adiabatic Kohn-Sham (KS) equations. While MGGA response properties of current-free ground states become manifestly gauge-variant to second order, linear response properties are affected by a new XC kernel appearing in the cMGGA magnetic orbital rotation Hessian. This kernel reflects the first-order coupling of KS orbitals due to changes in the paramagnetic current density and has apparently been ignored in previous MGGA response implementations. Inclusion of the current dependence increases total computation times by less than 50%. Benchmark applications to 109 adiabatic excitation energies using the Tao-Perdew-Staroverov-Scuseria (TPSS) MGGA and its hybrid version TPSSh show that cMGGA excitation energies are slightly lower than the MGGA ones on average, but exhibit fewer outliers. Similarly, the optical rotations of 13 small organic molecules show a small but systematic improvement upon inclusion of the magnetic XC kernel. We conclude that cMGGAs should replace MGGAs in all applications involving time-dependent or current-carrying states. (C) 2012 American Institute of Physics. [http://dx.doi.org/10.1063/1.4759080]
引用
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页数:10
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