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creating_inputs [2016/12/29 15:49] krejcio |
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[[http://www.fireball-dft.org]] | [[http://www.fireball-dft.org]] | ||
- | Unfortunately official version cannot write out input files. | + | Official version of FireballTG can write out input files now. |
- | A working executable for creation of necessary input files is at: | + | A working executable for creation of necessary input files is also at: |
/storage/praha1/home/krejcio/bin_fireball_stable/fireball.x | /storage/praha1/home/krejcio/bin_fireball_stable/fireball.x | ||
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&END | &END | ||
- | In case of PBC calculations phik_0001_s.dat, phik_0001_py.dat, ... files are produced by the Fireball. In case of cluster calculations phik_s.dat, phik_py.dat, ... are outputs of the Fireball calculations. They serve as inputs for the PP-STM calculations. Inside they look like: | + | In case of PBC calculations __phik_0001_s.dat__, __phik_0001_py.dat__, ... files are produced by the Fireball. In case of cluster calculations __phik_s.dat__, __phik_py.dat__, ... are outputs of the Fireball calculations. They serve as inputs for the PP-STM calculations. Inside they look like: |
38 280 -5.37896401 Number of atoms Number of states (Molecular orbitals) The Fermi Level | 38 280 -5.37896401 Number of atoms Number of states (Molecular orbitals) The Fermi Level | ||
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[[http://wiki.fysik.dtu.dk/gpaw/]] | [[http://wiki.fysik.dtu.dk/gpaw/]] | ||
- | Even though the GPAW is mainly used for representing the wave-function on a grid it can work in LCAO mode as well. For the purpose of making inputs for the PP-STM calculations the LCAO mode is necessary. Both - default or double-zeta (basis='dzp'; for more information look at the GPAW web page) - basis sets can be used. The PP-STM code reads the stored *.gpw binary produced by the GPAW calculations. Here is an example of some GPAW script for the calculations of the input: | + | Even though the GPAW is mainly used for representing the wave-function on a grid it can work in LCAO mode as well. For the purpose of making inputs for the PP-STM calculations the LCAO mode is necessary. Both - default or double-zeta (basis='dzp'; for more information look at the GPAW web page http://wiki.fysik.dtu.dk/gpaw/) - basis sets can be used. The PP-STM code reads the stored *.gpw binary produced by the GPAW calculations. Here is an example of some GPAW script for the calculations of the input: |
from ase import * | from ase import * | ||
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calc.write('out_LCAO_'+xc+'.gpw',mode='all') # saves the calculation into binary 'out_LCAO_LDA.gpw' file | calc.write('out_LCAO_'+xc+'.gpw',mode='all') # saves the calculation into binary 'out_LCAO_LDA.gpw' file | ||
- | The results of the GPAW calculations is stored in binary file 'out_LCAO_LDA.gpw' | + | The results of the GPAW calculations is stored in binary file '__out_LCAO_LDA.gpw__' |
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into control.in | into control.in | ||
- | The calculations produces: KS_eigenvectors.band_1.kpt_1.out for spin-restricted calculations or KS_eigenvectors_dn.band_1.kpt_1.out & KS_eigenvectors_up.band_1.kpt_1.out in the case of spin-polarized calculations. | + | The calculations produces: __KS_eigenvectors.band_1.kpt_1.out__ for spin-restricted calculations or __KS_eigenvectors_dn.band_1.kpt_1.out__ & __KS_eigenvectors_up.band_1.kpt_1.out__ in the case of spin-polarized calculations. |
Note: For cluster calculations Mathematica scripts have to be used for creating PP-STM inputs. | Note: For cluster calculations Mathematica scripts have to be used for creating PP-STM inputs. | ||