Evert Jan Baerends
Theoretical Chemistry,Vrije Universiteit, Amsterdam, The Netherlands
Video Recording
Abstract
We will first review many wrong statements in the literature on the nature and the (lack of) physical meaning of Kohn-Sham orbitals.
Next the nature of the occupied KS orbitals, and their advantages over Hartree-Fock orbitals are highlighted.
Then we address orbital energies. Exact KS orbitals have many virtues:
- the orbital energies of the occupied orbitals are close to ionization potentials (an order of magnitude better agreement than the Koopmans’ type agreement in Hartee-Fock) [1];
- virtual orbital energies are realistic: occupied-unoccupied orbital energy differencies are very close to excitation energies. There is no “gap problem” in DFT! [2,3]
- the KS virtual orbitals are typically bound states and have good (valence type) shapes (not unphysically diffuse like the Hartree-Fock virtuals); excitations can be described in most cases as simple single orbital-to-orbital transitions [2,3].
Unfortunately, orbital energies in the common LDA and GGA calculations are very wrong: they are typically 5 eV (more than 100 kcal/mol) higher than the exact Kohn-Sham orbital energies, an error that would be completely unacceptable in total energies. We will first analyze where this error comes from - it is not due to wrong asymptotic behavior of LDA/GGA potentials, or to a “self-interaction error” but it is caused by erroneous density dependence of the standard Exc[ρ] functionals, hence a wrong derivative (= potential). We will demonstrate that approximate potentials can be formulated that have similar good properties for ionization and excitation energies as the exact KS potential [4].
[1] D. P. Chong, O. Gritsenko, E. J. Baerends, J. Chem. Phys. 116 (2002) 1760; O. Gritsenko, B. Braïda, E. J. Baerends, J. Chem. Phys. 119 (2003) 1937
[2] E. J. Baerends, O. Gritsenko, R. van Meer, PCCP 15 (2013) 16408
[3] R. van Meer, O. Gritsenko, E. J. Baerends, J. Chem. Theor. Comp. 10 (2014) 4432.
[4] O. Gritsenko, L. Mentel, E. J. Baerends, J. Chem. Phys. 144 (2016) 204114