GW and the Bethe–Salpeter equation

Theory track

In plain words

Two calculations that take over where , the standard one, stops. The first corrects the energy cost of adding or removing an electron; the second adds the attraction between an it leaves behind, which is what decides the colour of light a thin crystal absorbs.

Going deeper

Left: three energy-level diagrams for one monolayer. DFT gives a small gap; GW gives a larger quasiparticle gap; GW plus the Bethe–Salpeter equation places an exciton level below the quasiparticle conduction band, and the optical gap is the energy of that exciton, lower by the binding energy E_b, which is close to 1 eV in free-standing MoS₂. Right: quasiparticle gap against the vacuum between periodic copies of the sheet; with Coulomb truncation the gap is flat, without it the gap creeps up slowly, like 1/L. three levels of theory, one monolayer E_b DFT gap too small GW quasiparticle GW + BSE optical gap exciton E_b close to 1 eV: free-standing MoS₂ why 2D calculations converge slowly quasiparticle gap vacuum between periodic copies with Coulomb truncation without: creeps up slowly, like 1/L
Semi-local DFT underestimates the gap, GW corrects it to the energy of adding or removing an electron, and the Bethe–Salpeter equation adds the electron–hole attraction that sets the optical gap. For a 2D sheet, periodic copies screen each other unless the Coulomb interaction is truncated, and results then converge only slowly with vacuum size.

Why DFT gaps are too small, and what GW fixes

The band energies of density functional theory are not, strictly, the energies needed to add or remove an electron, and the common semi-local functionals underestimate substantially, often by a third or more. Hybrid functionals help, but include screening only in an averaged way.

GW, introduced by Hedin in 1965, calculates energies directly. The self-energy – the correction an electron feels from the response of all the others – is approximated as the product of the one-particle Green’s function G and the interaction W. Usually GW is applied once on top of a DFT calculation, called G0W0, or iterated partly to self-consistency. The result is the , the quantity measured by and .

Adding the exciton

Light does not measure the quasiparticle gap. It creates an electron and a hole that attract each other, and the Bethe–Salpeter equation, solved with GW energies and the screened interaction, finds those correlated pairs: energies, binding energies and a full absorption spectrum.

In this step is not a small correction. Free-standing MoS2 is calculated to have excitons bound by close to 1 eV; a or screens the attraction and reduces it. A historical warning follows: semi-local DFT gaps of monolayers often land near the measured optical gap, but only because two large errors, the missing self-energy and the missing exciton binding, roughly cancel.

Why 2D calculations are expensive

Plane-wave codes treat a sheet as a stack of periodic copies separated by vacuum. The long-range Coulomb interaction couples those copies, so each layer is screened by its images, and gaps and binding energies creep towards their true values only slowly as the vacuum grows. Truncating the Coulomb interaction between copies removes the problem and should be standard.

Screening in 2D also changes rapidly at small wavevectors, so the Brillouin zone has to be sampled densely near its centre, and convergence with the number of empty bands and the cutoff is slow. GW and BSE cost far more than DFT, and is essential for TMDCs. Results only mean something with the starting functional, the level of self-consistency, the truncation, the k-point grid and the treatment of the substrate stated.

For specialists

GW replaces Kohn–Sham eigenvalues with quasiparticle energies from a screened-exchange self-energy, opening the gaps that semi-local DFT underestimates; solving the Bethe–Salpeter equation on top adds the electron–hole interaction and produces optical spectra with bound excitons. In 2D both converge painfully slowly with vacuum size and k-point sampling, because screening is non-analytic near q = 0 – a Coulomb cutoff and dense sampling around the band edge are not optional.

Where this comes from

  1. New method for calculating the one-particle Green’s function with application to the electron-gas problem Hedin · Physical Review 139, A796 (1965) cited by 5,512
  2. Electron-hole excitations and optical spectra from first principles Rohlfing and Louie · Physical Review B 62, 4927 (2000) cited by 1,955
  3. Optical spectrum of MoS2: many-body effects and diversity of exciton states Qiu et al. · Physical Review Letters 111, 216805 (2013) cited by 1,616