From the theory point of view, the quasiparticle energy of an excitation corresponds
to the energy required to remove/add an electron from/to a many-particle system.
It is the solution of a non-linear and energy-dependent equation, the quasiparticle equation, in which all
the many-body interaction effects among the electrons of the system, are accounted by
the self-energy.
The GW approximation
is the first-order perturbative expansion of the electronic self-energy
in terms of the screened interaction $W$.
In the GW approximation vertex corrections are neglected and
the self-energy reduces to a simple direct product (in real space)
of the Green function or dressed electron propagator $G$ and the
dynamically screened interaction $W$, $\Sigma^{GW} = i G(x_1,x_2) W(x_1^+,x_2)$,
or diagrammatically:
The first GW calculation on the jellium model is due to Hedin 1965. First ab initio calculations in real systems are due to Strinati, Mattausch and Hanke 1980 and 1982 ( $G_0W_0$ on top of Hartree-Fock, HF) and then to Hybertsen and Louie 1985, and Godby, Schlüter and Sham 1987 ( $G_0W_0$ on top of density-functional theory in the local-density approximation, DFT-LDA). They all showed that already a non-self-consistent G0 W0 self-energy always improves the band gap toward the experiment, reducing the HF and increasing the DFT-LDA band-gaps, achieving an error of around 1% with respect to angle-resolved photoemission (ARPES) experiments. Since then, the validity of the GW approximation has been confirmed by many other calculations. Here a figure reporting a statistics over several G0 W0 calculations of the band gap in literature, starting with the statistics reported in the 1999 Hedin review.