Density Functional Theory (DFT) - Basics
The information of a quantum system can be obtained from the state function (or wave function), which is described by the Schrödinger equation as $\hat{H} \Psi=E \Psi$. In this equation, $\hat{H}$ is the Hamiltonian operator and $\Psi$ is a set of solutions of the Hamiltonian. Each of these solution $\psi_{n}$ has an associated eigenvalue $E_{n}$ that satisfies the eigenvalue equation. For a system consisting of N electrons, the time independent Schrödinger equation is a function of 3N coordinates. To obtain an approximation solution of Schrödinger equation, define the electron density as $n(\mathbf{r})=2\sum_{i}\psi_{i}^{*}(\mathbf{r})\psi_{i}(\mathbf{r})$, where $n(\mathbf{r})$ is a function of only 3 coordinates and contains a great amount of the information that is actually physical observable. The density functional theory (DFT) rests on the Hohenberg and Kohn theorem and Kohn-Sham equation.
The Hohenberg and Kohn theorem states:
- The ground-state energy from Schrödinger's equation is a unique functional of the electron density.
- The electron density that minimizes the energy of the overall functional is the true electron density corresponding to the full solution of the Schrödinger equation.
The approximation of exchange-correlation potential includes local density approximation (LDA), generalized gradient approximation (GGA), etc. Two of the most widely used GGA functionals are the Perdew-Wang functional (PW91) and the Perdew-Burke-Ernzerhof functional (PBE).