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Second tutorial on GW

Treatment of metals.

This tutorial aims at showing how to obtain self-energy corrections to the DFT Kohn-Sham eigenvalues within the GW approximation, in the metallic case, without the use of a plasmon-pole model. The band width and Fermi energy of Aluminum will be computed.

The user may read the papers

  • F. Bruneval, N. Vast, and L. Reining, Phys. Rev. B 74 , 045102 (2006) [Bruneval2006], for some information and results about the GW treatment of Aluminum. He will also find there an analysis of the effect of self-consistency on quasiparticles in solids (not present in this tutorial, however available in Abinit). The description of the contour deformation technique that bypasses the use of a plasmon-pole model to calculate the frequency convolution of G and W can be found in

  • S. Lebegue, S. Arnaud, M. Alouani, P. Bloechl, Phys. Rev. B 67, 155208 (2003) [Lebegue2003],

with the relevant formulas.

A brief description of the equations implemented in the code can be found in the GW notes Also, it is suggested to acknowledge the efforts of developers of the GW part of ABINIT, by citing the 2005 ABINIT publication.

The user should be familiarized with the four basic tutorials of ABINIT, see the tutorial index as well as the first GW tutorial.


All the necessary input files to run the examples can be found in the ~abinit/tests/ directory where ~abinit is the absolute path of the abinit top-level directory.

To execute the tutorials, you are supposed to create a working directory (Work*) and copy there the input files and the files file of the lesson.

The files file ending with _x (e.g. tbase1_x.files) must be edited every time you start to use a new input file. You will discover more about the files file in section 1.1 of the help file.

To make things easier, we suggest to define some handy environment variables by executing the following lines in the terminal:

export ABI_HOME=Replace_with_the_absolute_path_to_the_abinit_top_level_dir

export ABI_TESTS=$ABI_HOME/tests/

export ABI_TUTORIAL=$ABI_TESTS/tutorial/           # Files for base1-2-3-4, GW ...
export ABI_TUTORESPFN=$ABI_TESTS/tutorespfn/       # Files specific to DFPT tutorials.
export ABI_TUTOPARAL=$ABI_TESTS/tutoparal/         # Tutorials about parallel version
export ABI_TUTOPLUGS=$ABI_TESTS/tutoplugs/         # Examples using external libraries.
export ABI_PSPDIR=$ABI_TESTS/Psps_for_tests/       # Pseudos used in examples.

export PATH=$ABI_HOME/src/98_main/:$PATH

The examples in this tutorial will use these shell variables so that one can easily copy and paste the code snippets into the terminal (remember to set ABI_HOME first!)

The last line adds the directory containing the executables to your PATH so that one can invoke the code by simply typing abinit in the terminal instead of providing the absolute path.

Finally, to run the examples in parallel with e.g. 2 MPI processes, use mpirun (mpiexec) and the syntax:

mpirun -n 2 abinit < files_file > log 2> err

The standard output of the application is redirected to log while err collects the standard error (runtime error messages, if any, are written here).

This tutorial should take about one hour to be completed (also including the reading of [Bruneval2006] and [Lebegue2003].

Visualisation tools are NOT covered in this tutorial. Powerful visualisation procedures have been developed in the Abipy context, relying on matplotlib. See the README of Abipy and the Abipy tutorials.

The preliminary Kohn-Sham band structure calculation

Before beginning, you might consider to work in a different subdirectory as for the other tutorials. Why not Work_gw2?

In tutorial 4, we have computed different properties of Aluminum within the LDA. Unlike for silicon, in this approximation, there is no outstanding problem in the computed band structure. Nevertheless, as you will see, the agreement of the band structure with experiment can be improved significantly if one relies on the GW approximation.

In the directory Work_gw2, copy the files tgw2_x.files and located in $ABI_TUTORIAL/Input, and modify the tgw2_x.files file as usual (see the first tutorial).

mkdir Work_gw2
cd Work_gw2
cp ../tgw2_x.files .  # modify this file as usual (see tutorial 1)
cp ../ .

Then issue:

abinit < tgw2_x.files > tgw2_1.log 2> err &

This run generates the WFK file for the subsequent GW computation and also provides the band width of Aluminum. Note that the simple Fermi-Dirac smearing functional is used (occopt = 3), with a large smearing (tsmear = 0.05 Ha). The k-point grid is quite rough, an unshifted 4x4x4 Monkhorst-Pack grid (64 k-points in the full Brillouin Zone, folding to 8 k-points in the Irreducible wedge, ngkpt = 4 4 4). Converged results would need a 4x4x4 grid with 4 shifts (256 k-points in the full Brillouin zone). This grid contains the \Gamma point, at which the valence band structure reaches its minimum.

The output file presents the Fermi energy

 Fermi (or HOMO) energy (eV) =   7.14774   Average Vxc (eV)=  -9.35982

as well as the lowest energy, at the \Gamma point

 Eigenvalues (   eV  ) for nkpt=   8  k points:
 kpt#   1, nband=  6, wtk=  0.01563, kpt=  0.0000  0.0000  0.0000 (reduced coord)
  -3.76175  19.92114  19.92114  19.92114  21.00078  21.00078

So, the occupied band width is 10.90 eV. More converged calculations would give 11.06 eV (see [Bruneval2006]).
This is to be compared to the experimental value of 10.6 eV (see references in [Bruneval2006]).

Calculation of the screening file

In order not to lose time, let us start the calculation of the screening file before the examination of the corresponding input file. So, copy the file, and modify the tgw2_x.files file as usual (replace occurrences of twg2_x by tgw2_2). Also, copy the WFK file (tgw2_1o_WFK) to tgw2_2i_WFK. Then run the calculation (it should take about 30 seconds).

We now have to consider starting a GW calculation. However, unlike in the case of Silicon in the previous GW tutorial, where we were focussing on quantities close to the Fermi energy (spanning a range of a few eV), here we need to consider a much wider range of energy: the bottom of the valence band lies around -11 eV below the Fermi level. Unfortunately, this energy is of the same order of magnitude as the plasmon excitations. With a rough evaluation, the classical plasma frequency for a homogeneous electron gas with a density equal to the average valence density of Aluminum is 15.77 eV. Hence, using plasmon-pole models may be not really appropriate.

In what follows, one will compute the GW band structure without a plasmon-pole model, by performing explicitly the numerical frequency convolution. In practice, it is convenient to extend all the functions of frequency to the full complex plane. And then, making use of the residue theorem, the integration path can be deformed: one transforms an integral along the real axis into an integral along the imaginary axis plus residues enclosed in the new contour of integration. The method is extensively described in [Lebegue2003].

Examine the input file

The ten first lines contain the important information. There, you find some input variables that you are already familiarized with, like optdriver, ecuteps, but also new input variables: gwcalctyp, nfreqim, nfreqre, and freqremax. The purpose of this run is simply to generate the screening matrices. Unlike for the plasmon-pole models, one needs to compute these at many different frequencies. This is the purpose of the new input variables. The main variable gwcalctyp is set to 2 in order to specify a non plasmon-pole model calculation. Note that the number of frequencies along the imaginary axis governed by nfreqim can be chosen quite small, since all functions are smooth in this direction. In contrast, the number of frequencies needed along the real axis set with the variable nfreqre is usually larger.

Finding the Fermi energy and the bottom of the valence band

In order not to lose time, let us start the calculation of the band width before the study of the input file. So, copy the file, and modify the tgw3_x.files file as usual (replace occurrences of twg2_x by tgw2_3). Also, copy the WFK file (tgw2_1o_WFK) to tgw2_3i_WFK, and the screening file (tgw2_2o_SCR) to tgw2_3i_SCR. Then run the calculation (it should take about 2 minutes on a 3 GHz PC).

The computation of the GW quasiparticle energy at the \Gamma point of Aluminum does not differ from the one of quasiparticle in Silicon. However, the determination of the Fermi energy raises a completely new problem: one should sample the Brillouin Zone, to get new energies (quasiparticle energies) and then determine the Fermi energy. This is actually the first step towards a self-consistency!

Examine the input file

The first thirty lines contain the important information. There, you find some input variables with values that you are already familiarized with, like optdriver, ecutsigx, ecutwfn. Then, comes the input variable gwcalctyp = 12. The value x2 corresponds to a contour integration. The value 1x corresponds to a self-consistent calculation with update of the energies only. Then, one finds the list of k points and bands for which a quasiparticle correction will be computed: nkptgw, kptgw, and bdgw. The number and list of k-points is simply the same as nkpt and kpt. One might have specified less k-points, though (only those needing an update). The list of band ranges bdgw has been generated on the basis of the LDA eigenenergies. We considered only the bands in the vicinity of the Fermi level: bands much below or much above are likely to remain much or much above the Fermi region. In the present run, we are just interested in the states that may cross the Fermi level, when going from LDA to GW. Of course, it would have been easier to select an homogeneous range for the whole Brillouin zone, e.g. from 1 to 5, but this would have been more time-consuming.

In the output file, one finds the quasiparticle energy at \Gamma, for the lowest band:

k =    0.000   0.000   0.000
 Band     E_lda   <Vxclda>   E(N-1)  <Hhartree>   SigX  SigC[E(N-1)]    Z     dSigC/dE  Sig[E(N)]  DeltaE  E(N)_pert E(N)_diago
    1    -3.762    -9.451    -3.762     5.689   -15.049     5.676     0.777    -0.287    -9.390     0.060    -3.701    -3.684

(the last column is the relevant quantity). The updated Fermi energy is also mentioned:

 New Fermi energy:     2.469501E-01 Ha ,    6.719854E+00 eV

The last information is not printed in case of gwcalctyp lower than 10.

Combining the quasiparticle energy at \Gamma and the Fermi energy, gives the band width, 10.404 eV. Using converged parameters, the band width will be 10.54 eV (see [Bruneval2006]). This is in excellent agreement with the experimental value of 10.6 eV.

Computing a GW spectral function, and the plasmon satellite of Aluminum

The access to the non-plasmon-pole-model self-energy (real and imaginary part) has additional benefit, e.g. an accurate spectral function can be computed, see [Lebegue2003]. You may be interested to see the plasmon satellite of Aluminum, which can be accounted for within the GW approximation.

Remember that the spectral function is proportional to (with some multiplicative matrix elements) the spectrum which is measured in photoemission spectroscopy (PES). In PES, a photon impinges the sample and extracts an electron from the material. The difference of energy between the incoming photon and the obtained electron gives the binding energy of the electron in the solid, or in other words the quasiparticle energy or the band structure. In simple metals, an additional process can take place easily: the impinging photon can extract an electron together with a global charge oscillation in the sample. The extracted electron will have a kinetic energy lower than in the direct process, because a part of the energy has gone to the plasmon. The electron will appear to have a larger binding energy… You will see that the spectral function of Aluminum consists of a main peak which corresponds to the quasiparticle excitation and some additional peaks which correspond to quasiparticle and plasmon excitations together.

In order not to lose time, this calculation can be started before the examination of the input file. So, copy the file, and modify the tgw4_x.files file as usual (replace occurrences of twg2_x by tgw2_4). Also, copy the WFK file (tgw2_1o_WFK) to tgw2_4i_WFK, and the screening file (tgw2_2o_SCR) to tgw2_4i_SCR. Then run the calculation (it should take about 2 minutes on a 3 GHz PC).

Compared to the previous file (, the input file contains two additional keywords: nfreqsp, and freqspmax. Also, the computation of the GW self-energy is done only at the \Gamma point.

The spectral function is written in the file tgw2_4o_SIG. It is a simple text file. It contains, as a function of the frequency (eV), the real part of the self-energy, the imaginary part of the self-energy, and the spectral function. You can visualize it using your preferred software. For instance, start gnuplot and issue

p 'tgw2_4o_SIG' u 1:4 w l

You should be able to distinguish the main quasiparticle peak located at the GW energy (-3.7 eV) and some additional features in the vicinity of the GW eigenvalue minus a plasmon energy (-3.7 eV - 15.8 eV = -19.5 eV).


If AbiPy is installed on your machine, you can use the abiopen script with the --expose option to visualize the results: -e -sns

Another file, tgw2_4o_GW, is worth to mention: it contains information to be used for the subsequent calculation of excitonic effects within the Bethe-Salpeter Equation with ABINIT or with other codes from the ETSF software page.