The Kohn-Sham equations are a set of mathematical equations used in quantum mechanics to simplify the complex problem of understanding how electrons behave in atoms and molecules. They introduce fictitious non-interacting electrons and use them to find the most stable arrangement of electrons, which helps scientists understand and predict the properties of matter at the atomic and molecular scale.
In physics and quantum chemistry, specifically density functional theory, the KohnâÂÂSham equation is the non-interacting Schrödinger equation (more clearly, Schrödinger-like equation) of a fictitious system (the "KohnâÂÂSham system") of non-interacting particles (typically electrons) that generate the same density as any given system of interacting particles.
In the KohnâÂÂSham theory the introduction of the noninteracting kinetic energy functional T<sub>s</sub> into the energy expression leads, upon functional differentiation, to a collection of one-particle equations whose solutions are the KohnâÂÂSham orbitals.
The KohnâÂÂSham equation is defined by a local effective (fictitious) external potential in which the non-interacting particles move, typically denoted as v<sub>s</sub>(r) or v<sub>eff</sub>(r), called the KohnâÂÂSham potential. If the particles in the KohnâÂÂSham system are non-interacting fermions (non-fermion density functional theory has been studied), the KohnâÂÂSham wavefunction is a single Slater determinant constructed from a set of orbitals that are the lowest-energy solutions to
This eigenvalue equation is the typical representation of the KohnâÂÂSham equations. Here õ<sub>i</sub> is the orbital energy of the corresponding KohnâÂÂSham orbital , and the density for an N-particle system is
The KohnâÂÂSham equations are named after Walter Kohn and Lu Jeu Sham, who introduced the concept at the University of California, San Diego, in 1965.
Kohn received a Nobel Prize in Chemistry in 1998 for the KohnâÂÂSham equations and other work related to density functional theory (DFT).
In KohnâÂÂSham density functional theory, the total energy of a system is expressed as a functional of the charge density as
where T<sub>s</sub> is the KohnâÂÂSham kinetic energy, which is expressed in terms of the KohnâÂÂSham orbitals as
v<sub>ext</sub> is the external potential acting on the interacting system (at minimum, for a molecular system, the electronâÂÂnuclei interaction), E<sub>H</sub> is the Hartree (or Coulomb) energy
and E<sub>xc</sub> is the exchangeâÂÂcorrelation energy. The KohnâÂÂSham equations are found by varying the total energy expression with respect to a set of Kohn-Sham orbitals subject to the constraint that they are orthogonal, this yields a time-independent Schrödinger equation with a scalar potential equal to the KohnâÂÂSham potential
where the last term
is the exchangeâÂÂcorrelation potential. This term, and the corresponding energy expression, are the only unknowns in the KohnâÂÂSham approach to density functional theory. An approximation that does not vary the orbitals is Harris functional theory.
The KohnâÂÂSham orbital energies õ<sub>i</sub>, in general, have little physical meaning (see Koopmans' theorem). The sum of the orbital energies is related to the total energy as
Because the orbital energies are non-unique in the more general restricted open-shell case, this equation only holds true for specific choices of orbital energies (see Koopmans' theorem).