Ordinary Kohn–Sham DFT:
where:
- : the external potential from the atomic nuclei acting on the electrons;
- : the classical electrostatic Coulomb potential generated by the electron density;
- : the exchange–correlation potential, which accounts for the quantum many-body effects not included in the Hartree potential.
The KS equations mainly help us obtain an accurate ground-state electron density, but their eigenvalues are not guaranteed to be true electron excitation energies.
For example, the exchange–correlation potential used in PBE approximates the complex electron interactions mainly from the electron density and its gradient near a given position. However, after adding an electron to the material, the other electrons in the system redistribute, and the resulting many-body response is clearly nonlocal and dynamic; has only a limited ability to describe these effects.
The GW approximation:
Suppose we add an electron to a material. It repels the surrounding electrons, causing them to redistribute and forming a polarization cloud.
Therefore, what actually propagates is no longer a completely independent bare electron; it can be understood as:
The quasiparticle equation derived from the Dyson equation: describes the energy and wavefunction of a quasiparticle
Here , i.e., the self-energy.
Comparing the quasiparticle equation with the Kohn–Sham DFT equation, the self-energy can be understood as an upgrade of the exchange–correlation potential :
Here is usually a local or semilocal, static potential, whereas is generally a nonlocal, energy-dependent operator.
The central formula of the GW approximation is:
that is:
where:
- : the single-particle Green's function;
- : the screened Coulomb interaction.
In , the noninteracting Green's function is usually constructed from the wavefunctions and eigenvalues obtained from DFT:
The screened Coulomb interaction is:
where:
is the bare Coulomb interaction;
is the dielectric function;
is the transferred momentum, corresponding to:
and:
.
Origin of :
After the system is subjected to the total potential , the electron density changes. Within the linear response regime:
where is the polarizability, which describes the response of the electron density to an external potential perturbation.
After the electron density changes, it in turn produces an induced potential through the Coulomb interaction:
where is the bare Coulomb interaction.
The total potential consists of the external potential and the induced potential:
Rearranging gives:
Define the dielectric function:
Thus:
Therefore:
So describes how electronic screening in the material converts the original external potential into the total potential actually felt inside the system.
can also be understood through the multiple responses of the electrons:
- First electron response:
- The newly generated charge density produces a new Coulomb potential:
- The new Coulomb potential acts on the electrons again, causing a second response:
............
Continuing indefinitely:
Define :
Therefore:
Polarization function P
In :
and:
Substituting the two 's gives the independent-particle polarizability:
Fourier transforming it and projecting it onto a plane-wave basis:
we obtain:
Because the crystal has translational symmetry, momentum conservation requires:
Therefore define the transition matrix element:
that is:
Finally we get:
where:
is the crystal volume, and is the occupation number.
Here it can be intuitively understood as:
Next:
- Construct the dielectric matrix from .
Formula:
In a plane-wave basis:
Since the bare Coulomb interaction is diagonal in a plane-wave basis:
Therefore:
Inverting the dielectric matrix gives:
Then construct the screened Coulomb interaction :
Thus the whole process is:
Substituting this back into:
gives the self-energy .
Finally, the quasiparticle energy is obtained from:
where is the quasiparticle renormalization factor, which accounts for the energy dependence of the self-energy :
Therefore the entire computational workflow can be summarized as: