This tutorial begins with an LDA calculation for Si, starting from an init file. Following this is a demonstration of a quasi-particle self-consistent GW (QSGW) calculation. An example of the 1-shot GW code is provided in a separate tutorial.
After the potential is obtained, the energy bands are drawn, and the macroscopic dielectric function is calculated in the RPA. This tutorial explains how to calculate with ladder diagrams.
Click on the Command Summary below for a summary of the commands explained in this tutorial. Theory for GW and QSGW, and its implementation in the Questaal suite, can be found in Phys. Rev. B76, 165106 (2007).
Each iteration of a QSGW calculation has two main parts: a section that uses effective one-body hamiltonians to make the density n (as in DFT), and the GW code that makes the self-energy of an interacting hamiltonian. For quasiparticle self-consistency, the GW code makes a “quasiparticlized” self-energy , which is used to construct the effective one-body hamiltonian for the next cycle. The process is iterated until the change in becomes small.
The one-body executable is lmf. The script lmfgwd is similar to lmf, but it is a driver whose purpose is to set up inputs for the GW code. is made by a shell script lmgw. The entire cycle is managed by a shell script lmgwsc, which runs the cycle shown in the figure above, and also does some bookkeeping, such as monitoring connvergence to self-consistency.
Before any self-energy exists, it is assumed to be zero. Thus the one-body hamiltonian is usually the LDA, though it can be something else, e.g. LDA+U.
Note: in some circumstances, e.g. to break time reversal symmetry inherent in the LDA, you need to start with LDA+U.
Thus, there are two self-energies and two corresponding Green’s functions: the interacting and non-interacting . At self-consistency the poles of and coincide: this is a unique and very advantageous feature of QSGW. It means that there is no “mass renormalization” of the bandwidth — at least at the GW level.
Usually the interacting isn’t made explicitly, but you can do so, as explained in this tutorial.
In short, a QSGW calculation consists of the following steps. The starting point is a self-consistent DFT calculation (usually LDA). The DFT eigenfunctions and eigenvalues are used by the GW code to construct a self-energy . This is called the “0th iteration.” If only the diagonal parts of are kept, the “0th” iteration corresponds to what is sometimes called 1-shot GW, or as GLDAWLDA.
In the next iteration, is added to the LDA hamiltonian. The density is made self-consistent, and control is handed over to the GW part. (Note that for a fixed density cancels the exchange-correlation potential from the LDA hamiltonian.) This process is repeated until the RMS change in falls below a certain tolerance value. The final self-energy (QSGW potential) can be thought of as an effective exchange-correlation functional that is tailored to the system. This is very convenient as it can now be used in an analogous way to standard DFT to calculate properties such as the band structure.
nano init.si #create init file using lines from box below blm init.si --express --gmax=5 --nk=4 --nit=20 --gw #use blm tool to create actrl and site files cp actrl.si ctrl.si && lmfa si && cp basp0.si basp.si #copy actrl to recognised ctrl prefix, run lmfa and copy basp lmf si > out.lmfsc #make self-consistent echo -1 | lmfgwd si #make GWinput file lmgwsc --wt --insul=4 --tol=2e-5 --maxit=5 si #self-consistent GW calculation vim ctrl.si #change number of iterations to 1 lmf si --rs=1,0 #lmf with QSGW potential to get QSGW band gap lmgwclear #clean up directory
Alternatively, you can run the following two one-liners to get the same result. This assumes you have already created the init file.
blm init.si --express=0 --gmax=5 --nk=4 --nit=20 --gw --nkgw=4 && cp actrl.si ctrl.si && lmfa si && cp basp0.si basp.si && lmf si > out.lmfsc echo -1 | lmfgwd si && lmgwsc --wt --insul=4 --tol=2e-5 --maxit=5 si > out.gwsc && lmgwclear && lmf si --rs=1,0 -vnit=1 > out.lmf_gwsc
The starting point is a self-consistent LDA density, you may want to review the DFT tutorial for silicon. Copy the following lines to a file called init.si:
LATTICE ALAT=10.26 PLAT= 0.00000000 0.50000000 0.50000000 0.50000000 0.00000000 0.50000000 0.50000000 0.50000000 0.00000000 # pos means cartesian coordinates, units of alat SITE ATOM=Si POS= 0.00000000 0.00000000 0.00000000 ATOM=Si POS= 0.25000000 0.25000000 0.25000000
Run the following commands to obtain a self-consistent density:
$ blm init.si --express --gmax=5 --nk=4 --nit=20 --gw $ cp actrl.si ctrl.si && lmfa si && cp basp0.si basp.si $ lmf si > out.lmfsc
Note that we have included an extra
--gw switch, which tailors the ctrl file for a GW calculation. To see how it affects the ctrl file, try running blm without
--gw. The switch modifies the basis set section (see the autobas line) to increase the size of the basis, which is necessary for GW calculations.
Two new blocks of text, the HAM and GW categories, are also added towards the end of the ctrl file. The extra parameters in the HAM category handle the inclusion of a self-energy, actually a GW potential (see theory notes above), in a DFT calculation. The GW category provides some default values for parameters that are required in the GW calculation. The GW code has its own input file and the DFT ctrl file influences what defaults are set in it, we will come back to this later.
Now check the output file out.lmfsc. It should converge in 10 iterations as can be seen from the end of the file. Note that ehf and ehk should be essentially the same (-1156.140684 Ry).
Search for the last occurence of the word ‘gap’. It should be around 0.58. Note that this result differs slightly from that from the LDA tutorial because the gw switch increases the size of the basis set.
Now that we have the input eigenfunctions and eigenvalues, the next step is to carry out a GW calculation. For this, we need an input file for the GW code.
The GW package (both one-shot and QSGW) uses one main user-supplied input file, GWinput. The structure of GWinput is documented here.
lmfgwd supplies the interface connecting the LDA code to the GW package. (The GW package only makes matrix elements of response functions or self-energies suitable for later analysis.)
It can also create a template GWinput file by running the following command:
$ echo -1 | lmfgwd si #make GWinput file
This is particularly convenient because GWinput is not easy to read, or to construct by hand.
Caution: the GWinput file made by lmfgwd should be regarded only as template. It is up to you to ensure that the contents are reasonable, even while for the most the template is reasonable.
lmfgwd has multiple options and is designed to run interactively. Using ‘echo -1’ automatically passes it the ‘-1’ option that specifies making a template input file. You can try running it interactively by just using the command ‘lmfgwd si’ and then entering ‘-1’. Some tags in GWinput read from the GW category. To see which ones, try
lmfgwd --input | grep GW_
Tags in the GW category of ctrl.si are used only to modify GWinput; the GW code does not read from the ctrl file. All of the tags in the You don’t need to supply any tags; lmfgwd will use reasonable defaults. Take a look at GWinput; it is a rather complicated input file but most of the time it the template lmfgwd uses reasonable defaults.
Two tags you particularly need to monitor are QpGcut_cou and n1n2n3. The former controls the plane wave cutoff. The computational cost is senstive to this value, so you want to make it as low as possible without messing up the results. It is a good idea to try a couple of values to satisfy your self that you have made a sensible choice: make it as small as you can while keeping the QP levels reasonable well converged.
n1n2n3 specifies the GW k-point mesh for now (further information can be found on the GWinput page). In GWinput look for the following line:
$ n1n2n3 4 4 4 ! for GW BZ mesh
This number was culled from ctrl.si. When reading this file, lmfgwd looks for tag GW_NKABC=4. In this case only one one number is supplied; that number is used for all three of the reciprocal lattice vectors, so 4 alone implies a 4 x 4 x 4 k mesh. If you want to run the calculation a bit quicker, change the k mesh to 3 x 3 x 3 by editing the GWinput file line:
$ n1n2n3 3 3 3 ! for GW BZ mesh
The k mesh of 3 x 3 x 3 divisions is rough, but it makes the calculation fast and for Si the results are reasonable. In this tutorial we will stick with 4 divisions. In any case, you need to monitor the k convergence. These can be time consuming and unfortunately there are no shortcuts. Note however, that the GW mesh is distinct from the k mesh lmf uses (read from BZ_NKABC). Typically a coarser mesh can often be used for the GW self-energy because generally varies much more smoothly with k than does the kinetic energy. This is fortunate because GW calculations are much more expensive, and in the existing implementation the computation time scales as n2.
Other convergence parameters to particularly watch out for are the product basis tolerance, the augmention lcutmx, and whether product basis functions are included for shallow core states.
We are now ready for a QSGW calculation, which you do with the shell script lmgwsc:
$ lmgwsc --wt --insul=4 --tol=2e-5 --maxit=0 si #zeroth iteration of QSGW calculation
Switch ‘–wt’ includes additional timing information in the printed output, insul refers to the number of occupied bands (normally spin degenerate so half the number of electrons), tol is the tolerance for the RMS change in the self-energy between iterations and maxit is the maximum number of QSGW iterations. Note that maxit is zero, this specifies that a single iteration is to be carried out starting from DFT with no self-energy (zeroth iteration).
Take a look at the line containing the file name llmf:
lmgw 15:26:47 : invoking mpix -np=8 /h/ms4/bin/lmf-MPIK --no-iactive cspi >llmf
Each QSGW iteration begins with a self-consistent DFT calculation by calling the program lmf and writing the output to the file llmf. We are starting from a self-consitent LDA density (we already ran lmf above) so this step is not actually necessary here. The next few lines are preparatory steps. The main GW calculation begins on the line containing the file name ‘lbasC’:
lmgw 16:27:55 : invoking /h/ms4/bin/code2/hbasfp0 --job=3 >lbasC lmgw 16:27:55 : invoking /h/ms4/bin/code2/hvccfp0 --job=0 >lvccC ... 0.0m (0.0h) lmgw 16:27:58 : invoking /h/ms4/bin/code2/hsfp0_sc --job=3 >lsxC ... 0.0m (0.0h) lmgw 16:27:59 : invoking /h/ms4/bin/code2/hbasfp0 --job=0 >lbas lmgw 16:27:59 : invoking /h/ms4/bin/code2/hvccfp0 --job=0 >lvcc ... 0.0m (0.0h) lmgw 16:28:02 : invoking /h/ms4/bin/code2/hsfp0_sc --job=1 >lsx ... 0.0m (0.0h) lmgw 16:28:02 : invoking /h/ms4/bin/code2/hx0fp0_sc --job=11 >lx0 ... 0.1m (0.0h) lmgw 16:28:07 : invoking /h/ms4/bin/code2/hsfp0_sc --job=2 >lsc ... 0.1m (0.0h) lmgw 16:28:13 : invoking /h/ms4/bin/code2/hqpe_sc 4 >lqpe
The three lines with lbasC, lvccC and lsxC are the steps that calculate the core contributions to the self-energy and the following lines up to the one with lsc are for the valence contribution to the self-energy. The lsc step, calculating the correlation part of the self-energy, is usually the most expensive step.
The last step (hpqe_sc) collects terms to make quasiparticlized self-energy and writes it to file sigm for every irreducible k point. Actually it writes . This makes running lmf very convenient, since lmf simply has to add this term to the LDA potential. Further information can be found in the annotated GW output page.
The self-energy produced so far is essentially the same as GLDAWLDA generated in the one-shot tutorial, only now there is no Z factor and the full is generated. This is distinct from computing the level shift in 1first order perturbation theory as lmgw1-shot did (and most GW codes do). This requires only the diagonal , which is fast and easier to make (and is why QSGW is more expensive to do).
It is interesting to compare one-shot results from the 0th iteration to the output of lmgw1-shot.
$ lmf si
The following line in the standard output specifies that the GW potential is being used:
RDSIGM: read file sigm and create COMPLEX sigma(R) by FT ...
The GW potential is contained in the file sigm, lmgwsc also makes a soft link sigm.si so lmf can read it. The GW potential is automatically used if present, this is specified by the HAM_RDSIG tag in the ctrl file.
After the first band pass, lmf yields a gap of 1.21 eV, essentially identical to what lmgw1-shot gives without a Z factor. In general this is not true; but Si is very simple and the and LDA eigenfunctions are very similar.
Nevertheless, note that as the density is updated (the off-diagonal elements of mean that the eigenfunctions change), the gap increases to 1.26 eV. This can be expressed as a change , where is implicitly given from DFT through self-consistency in lmf.
Run the command again but this time set the number of iterations (maxit) to something like 5:
$ lmgwsc --wt --insul=4 --tol=2e-5 --maxit=5 si #self-consistent GW calculation
The iteration count starts from 1 since we are now starting with a self-energy from the zeroth iteration. Again, the iteration starts with a self-consistent DFT-like calculation, but now from zeroth iteration is added. Take a look at the GW output again and you can see that the rest of the steps are the same as before. After 3 iterations the RMS change in the self-energy is below the tolerance - the calculation is converged.
mgwsc : iter 3 of 5 RMS change in sigma = 5.14E-06 Tolerance = 2e-5 more=F Mon 21 May 2018 19:08:21 BST elapsed wall time 5.0m (0.1h) mark
Now that we have a converged self-energy (sigm) we can go back to using lmf to calculate additional properties. We only want to run a single iteration so change the number of iterations (nit) to 1 in the ctrl file. Run the following command:
$ lmf si --rs=1,0 #lmf with QSGW potential to get QSGW band gap
--rs switch tells lmf to read from the restart file, which contains the LDA density, but not to write to it (once we have a converged density we want to keep this fixed). More information on command line switches can be found here.
Inspect the lmf output and you can find that the gap is now around 1.33 eV. It is larger because the one-body hamiltonian generating has a wider gap, which which increases $W$ and thus .
Check your directory and you will see that a large number of files were created. The following command removes many redundant files:
$ lmgwclear #clean up directory
Further details can be found in the Additional exercises below.
QSGW energy bands
lmf has a very powerful feature, that it can takes the inverse Bloch transform to put in real space, from the mesh of points it is calculated on From real space it can interpolate to any by performing a forward Bloch transform. The details are rather complicated, but they are explained in some detail in Section IIG of PRB76, 165106.
This feature enables us to compute the energy bands and any k, and allows us to draw the energy bands with minimal effort.
$ lmchk ctrl.si --syml~n=41~q=-.5,.5,.5,0,0,0,0,0,1 $ lmf ctrl.si --band~fn=syml $ echo -13,10,5,10 | plbnds -fplot -ef=0 -scl=13.6 -lbl=L,G,X bnds.si $ fplot -f plot.plbnds
lmchk makes a symmetry lines file, along the lines L-Γ and Γ-X. lmf generates the energy bands in symmetry-lines mode. Finally the last two commands convert bnds.si generated by lmf into a postscript figure.
QSGW RPA dielectric function
Here we show how to calculate the macroscopic dielectric function for Si in the RPA. Another tutorial shows how to calculate the macroscopic dielectric function with ladder diagrams.
The RPA dielectric function is computed from a starting hamiltonian . You can use any available , e.g. LDA, Here we use the QSGW generated in the previous section.
To make a good dielectric function it is necesssary to modify GWinput a little.
The 4×4×4 k mesh used for QSGW is reasonably sufficient for k integrated propertiees, but it is not not sufficient to pick up the detailed structure of the macroscopic dielectric function. Edit the n1n2n3 tag and increase the k mesh to 16×16×16 divisions:
n1n2n3 16 16 16 ! for GW BZ mesh
For a good frequency resolution, shrink the frequency mesh spacing to dw to 0.001 Hartree (or smaller, if desired)
dw 0.001 ! mesh spacing along Real axis (Hartree)
The macroscopic dielectric function is . Because it takes an average over the unit cell, the detailed shape of inside the unit cell is not so important. You can reduce the cutoffs significantly with minimal change in . Reducing it to 2 makes negligible difference in this case:
lcutmx(atom) = l-cutoff for the product basis 2 2
Supply GWinput with the q points for which you want to calculate . The code does not have the ability to take the limit analytically; you must choose a finite but small q. At the end of GWinput there are the following lines
QforEPSIBZ off <QforEPS> 0d0 0d0 0.015d0 </QforEPS>
It tells the GW code to make just a one point, close to the point. This corresponds approximately to . If you want to calculate also, add a line 0.015d0 0d0 0d0. Si is cubic and , so it is not necessary here.
You can either calculate the proper macroscopic dielectric function, , or one that neglects local fields, .
The latter is must faster, but it is approximate. Often the difference between the two is not large, however. Do one of:
lmgw --eps --ht si lmgw --epsNLF --ht si
The latter writes a file EPS0001.nlfc.dat, while the former writes both that file and EPS0001.dat.
Th first few lines should like the following
q(1:3) w(Ry) eps epsi --- LFC included. 0.00000000 0.00000000 0.01500000 0.0000D+00 0.928993543761226D+01 0.726517122804292D-15 0.107643374565477D+00 -0.841822371139706D-17 0.00000000 0.00000000 0.01500000 0.1005D-02 0.928999688792784D+01 0.721333610616975D-15 0.107642662539476D+00 -0.835805128491751D-17 0.00000000 0.00000000 0.01500000 0.3025D-02 0.929049220411353D+01 0.727839656503130D-15 0.107636923645147D+00 -0.843253724471668D-17 0.00000000 0.00000000 0.01500000 0.5065D-02 0.929149658090234D+01 0.730784249155761D-15 0.107625288487475D+00 -0.846482210402463D-17
Colums 1-4 are the q-point and frequency, resepectively. Columns 5-6 are the real and imaginary parts of ; columns 7-8 are the real and imaginary parts of .
Note that even while Si has a fundamental gap of approximately 1.2 eV, it is an indirect gap semiconductor. Since the electron-phonon interaction is missing absorption from indirect transitions is not included and is zero until the first direct gap transition at 0.2516D Ry, or 3.42 eV.
You can read the static dielectric constant, from EPS0001.dat. The calculated value is 9.3, which is 79% of the actual (11.7 at 0K). This error largely originates from the neglect of ladder diagrams.
1) Fundamental gap
The gap found in the tutorial is is actually the Γ-X gap; the true gap is a little smaller as can be seen by running lmf with a fine k mesh.
2) Changing k-point mesh
Test the convergence with respect to the GW k mesh by increasing to a 8 × 8 × 8 k mesh.
Try a QSGW calculation for GaAs. Note that the code automatically treats the Ga d state as valence (adds a local orbital). This requires a larger GMAX. You also need to run lmfa a second time to generate a starting density that includes this local orbital. The lmfa line for GaAs should be:
$ lmfa ctrl.gas; cp basp0.gas basp.gas; lmfa ctrl.gas
The init file is:
# init file for GaAs LATTICE # SPCGRP= ALAT=10.69 PLAT= 0.00000000 0.50000000 0.50000000 0.50000000 0.00000000 0.50000000 0.50000000 0.50000000 0.00000000 # 2 atoms, 1 species SITE ATOM=Ga POS= 0.00000000 0.00000000 0.00000000 ATOM=As POS= 0.25000000 0.25000000 0.25000000