Bulk material: h-BN: Difference between revisions

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[[Category:Modules]]
[[Category:Modules]]
[[Category:Tutorials]]
[[Category:Tutorials]]
In this module you will learn how to generate the Yambo ''SAVE'' folder for bulk hBN starting from a [https://www.quantum-espresso.org/ QuantumEspresso] calculation.<br>
Notice that beyond QuantumEspresso other DFT codes can be used to generate wave-functions for Yambo: [https://www.abinit.org/ Abinit] and [https://www.pwmat.com/ PWMat].


In this module you will learn how to generate the Yambo ''SAVE'' folder for bulk hBN starting from a PWscf calculation.
== Prerequisites ==
== Prerequisites ==
'''You will need''':
'''You will need''':
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* <code>pw.x</code> executable, version 5.0 or later
* <code>pw.x</code> executable, version 5.0 or later
* <code>p2y</code> and <code>yambo</code> executables
* <code>p2y</code> and <code>yambo</code> executables
* Follow the instructions in the [[Tutorials#Files|File page]] and download and unpack the hBN.tar.gz.


== System characteristics ==
== System characteristics ==
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* SCF run: shifted ''6x6x2'' grid (12 k-points) with 8 bands  
* SCF run: shifted ''6x6x2'' grid (12 k-points) with 8 bands  
* Non-SCF run: gamma-centred ''6x6x2'' (14 k-points) grid with 100 bands
* Non-SCF run: gamma-centred ''6x6x2'' (14 k-points) grid with 100 bands


== DFT calculations ==
== DFT calculations ==
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Next run a non-SCF calculation to generate a set of Kohn-Sham eigenvalues and eigenvectors for both occupied and unoccupied states (100 bands):  
Next run a non-SCF calculation to generate a set of Kohn-Sham eigenvalues and eigenvectors for both occupied and unoccupied states (100 bands):  
  $ pw.x < hBN_nscf.in > hBN_nscf.out
  $ pw.x < hBN_nscf.in > hBN_nscf.out                 ''(serial run, ~1 min) OR''
$ mpirun -np 2 pw.x < hBN_nscf.in > hBN_nscf.out      ''(parallel run, 40s)''
Here we use a ''6x6x2'' grid giving 14 k-points, but denser grids should be used for checking convergence of Yambo runs.
Here we use a ''6x6x2'' grid giving 14 k-points, but denser grids should be used for checking convergence of Yambo runs.


Line 40: Line 43:
  diago_thr_init=5.0e-6,
  diago_thr_init=5.0e-6,
  diago_full_acc=.true.
  diago_full_acc=.true.
which are needed for generating the Yambo databases accurately. Full explanations of these variables are given on the [http://www.quantum-espresso.org/wp-content/uploads/Doc/INPUT_PW.html quantum-ESPRESSO input variables page].  
which are needed for generating the Yambo databases accurately. Full explanations of these variables are given on the
[https://www.quantum-espresso.org/Doc/INPUT_PW.html quantum-ESPRESSO input variables page].


After these two runs, you should have a ''hBN.save'' directory:
After these two runs, you should have a ''hBN.save'' directory:
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* How to check the contents of the netCDF databases
* How to check the contents of the netCDF databases


== Links ==
<br>
* Next module: [[2D_material:_h-BN_sheet|Generate databases for 2D hBN]]
{| style="width:100%" border="1"
* Back to [[First steps: a walk through from DFT to optical properties|First steps with yambo]] tutorial
|style="width:15%; text-align:left"|Prev: [[First_steps:_a_walk_through_from_DFT_to_optical_properties|First steps]]  
* [[Tutorials|Back to tutorials menu]]
|style="width:70%; text-align:center"|Now: [[Tutorials|Tutorials Home]] --> [[First_steps:_a_walk_through_from_DFT_to_optical_properties|First steps]] --> [[Bulk_material:_h-BN|bulk hBN]]
 
|style="width:15%; text-align:right"|Next: [[Initialization|Initialization]]
<hr>
|-
Navigation: [[Main_Page|Home]] -> [[Tutorials]] --> [[Bulk material: h-BN|hBN bulk]]
|}

Latest revision as of 15:06, 16 June 2023

In this module you will learn how to generate the Yambo SAVE folder for bulk hBN starting from a QuantumEspresso calculation.
Notice that beyond QuantumEspresso other DFT codes can be used to generate wave-functions for Yambo: Abinit and PWMat.

Prerequisites

You will need:

  • PWSCF input files and pseudopotentials for hBN bulk
  • pw.x executable, version 5.0 or later
  • p2y and yambo executables
  • Follow the instructions in the File page and download and unpack the hBN.tar.gz.


System characteristics

Atomic structure of bulk hBN

Hexagonal boron nitride - hBN:

  • HCP lattice, ABAB stacking
  • Four atoms per cell, B and N (16 electrons)
  • Lattice constants: a = 4.716 [a.u.], c/a = 2.582
  • Plane wave cutoff 40 Ry (~1500 RL vectors in wavefunctions)
  • SCF run: shifted 6x6x2 grid (12 k-points) with 8 bands
  • Non-SCF run: gamma-centred 6x6x2 (14 k-points) grid with 100 bands


DFT calculations

$ cd YAMBO_TUTORIALS/hBN/PWSCF
$ ls
Inputs		Pseudos		PostProcessing		References
hBN_scf.in	hBN_nscf.in     hBN_scf_plot_bands.in  hBN_nscf_plot_bands.in 

First run the SCF calculation to generate the ground-state charge density, occupations, Fermi level, and so on:

$ pw.x < hBN_scf.in > hBN_scf.out

Inspection of the output shows that the valence band maximum lies at 5.06eV.

Next run a non-SCF calculation to generate a set of Kohn-Sham eigenvalues and eigenvectors for both occupied and unoccupied states (100 bands):

$ pw.x < hBN_nscf.in > hBN_nscf.out                  (serial run, ~1 min) OR
$ mpirun -np 2 pw.x < hBN_nscf.in > hBN_nscf.out       (parallel run, 40s)

Here we use a 6x6x2 grid giving 14 k-points, but denser grids should be used for checking convergence of Yambo runs.

Note the presence of the following flags in the input file:

wf_collect=.true.
force_symmorphic=.true.
diago_thr_init=5.0e-6,
diago_full_acc=.true.

which are needed for generating the Yambo databases accurately. Full explanations of these variables are given on the quantum-ESPRESSO input variables page.

After these two runs, you should have a hBN.save directory:

$ ls hBN.save
data-file.xml charge-density.dat gvectors.dat B.pz-vbc.UPF N.pz-vbc.UPF
K00001	K00002 .... 	K00035	K00036

Conversion to Yambo format

The PWscf bBN.save output is converted to the Yambo format using the p2y executable (pwscf to yambo), found in the yambo bin directory. Enter hBN.save and launch p2y:

$ cd hBN.save
$ p2y
...
<---> DBs path set to .
<---> Index file set to data-file.xml
<---> Header/K-points/Energies... done
...
<---> == DB1 (Gvecs and more) ...
<---> ... Database done
<---> == DB2 (wavefunctions)  ... done ==
<---> == DB3 (PseudoPotential) ... done ==
<--->  == P2Y completed ==

This output repeats some information about the system and generates a SAVE directory:

$ ls SAVE
ns.db1  ns.wf  ns.kb_pp_pwscf
ns.wf_fragments_1_1 ...
ns.kb_pp_pwscf_fragment_1 ...

These files, with an n prefix, indicate that they are in netCDF format, and thus not human readable. However, they are perfectly transferable across different architectures. You can check that the databases contain the information you expect by launching Yambo using the -D option:

$ yambo -D
[RD./SAVE//ns.db1]------------------------------------------
Bands                           : 100
K-points                        : 14
G-vectors             [RL space]:  8029
Components       [wavefunctions]: 1016
...
[RD./SAVE//ns.wf]-------------------------------------------
Fragmentation                    :yes
...
[RD./SAVE//ns.kb_pp_pwscf]----------------------------------
Fragmentation                    :yes
- S/N 006626 -------------------------- v.04.01.02 r.00000 -

In practice we suggest to move the SAVE folder into a new clean folder.

In this tutorial however, we ask instead that you continue using a SAVE folder that we prepared previously:

$ cd ../../YAMBO
$ ls
SAVE

Summary

From this tutorial you've learned:

  • How to run a DFT calculation with PWscf in preparation for Yambo
  • Convert the DFT output into the Yambo format
  • How to check the contents of the netCDF databases


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