SIESTA
Introduction
SIESTA is a density-functional theory code for very large systems based on atomic orbital (LCAO) basis sets.
Environment variables
The environment variable ASE_SIESTA_COMMAND
must hold the command
to invoke the siesta calculation. The variable must be a string
where PREFIX.fdf
/PREFIX.out
are the placeholders for the
input/output files. This variable allows you to specify serial or parallel
execution of SIESTA.
Examples: siesta < PREFIX.fdf > PREFIX.out
and
mpirun -np 4 /bin/siesta4.0 < PREFIX.fdf > PREFIX.out
.
A default directory holding pseudopotential files .vps/.psf
can be
defined to avoid defining this every time the calculator is used.
This directory can be set by the environment variable
SIESTA_PP_PATH
.
Set both environment variables in your shell configuration file:
$ export ASE_SIESTA_COMMAND="siesta < PREFIX.fdf > PREFIX.out"
$ export SIESTA_PP_PATH=$HOME/mypps
Alternatively, the path to the pseudopotentials can be given in the calculator initialization. Listed below all parameters related to pseudopotential control.
keyword |
type |
default value |
description |
---|---|---|---|
|
|
|
Directory for pseudopotentials to use None means using $SIESTA_PP_PATH |
|
|
|
String for picking out specific type
type of pseudopotentials. Giving
|
|
|
|
Whether psedos will be sym-linked into the execution directory. If False they will be copied in stead. Default is True on Unix and False on Windows. |
SIESTA Calculator
These parameters are set explicitly and overrides the native values if different.
keyword |
type |
default value |
description |
---|---|---|---|
|
|
|
Name of the output file |
|
|
|
Mesh cut-off energy in eV |
|
|
|
Exchange-correlation functional. Corresponds to either XC.functional or XC.authors keyword in SIESTA |
|
|
|
Energy shift for determining cutoff radii |
|
|
|
Monkhorst-Pack k-point sampling |
|
|
|
Type of basis set (‘SZ’, ‘DZ’, ‘SZP’, ‘DZP’) |
|
|
|
The spin approximation used, must be
either |
|
|
|
A method for specifying the basis set for some atoms. |
Most other parameters are set to the default values of the native interface.
Extra FDF parameters
The SIESTA code reads the input parameters for any calculation from a
.fdf
file. This means that you can set parameters by manually setting
entries in this input .fdf
file. This is done by the argument:
>>> Siesta(fdf_arguments={'variable_name': value, 'other_name': other_value})
For example, the DM.MixingWeight
can be set using
>>> Siesta(fdf_arguments={'DM.MixingWeight': 0.01})
The explicit fdf arguments will always override those given by other keywords, even if it breaks calculator functionality. The complete list of the FDF entries can be found in the official SIESTA manual.
Example
Here is an example of how to calculate the total energy for bulk Silicon, using a double-zeta basis generated by specifying a given energy-shift:
>>> from ase import Atoms
>>> from ase.calculators.siesta import Siesta
>>> from ase.units import Ry
>>>
>>> a0 = 5.43
>>> bulk = Atoms('Si2', [(0, 0, 0),
... (0.25, 0.25, 0.25)],
... pbc=True)
>>> b = a0 / 2
>>> bulk.set_cell([(0, b, b),
... (b, 0, b),
... (b, b, 0)], scale_atoms=True)
>>>
>>> calc = Siesta(label='Si',
... xc='PBE',
... mesh_cutoff=200 * Ry,
... energy_shift=0.01 * Ry,
... basis_set='DZ',
... kpts=[10, 10, 10],
... fdf_arguments={'DM.MixingWeight': 0.1,
... 'MaxSCFIterations': 100},
... )
>>> bulk.calc = calc
>>> e = bulk.get_potential_energy()
Here, the only input information on the basis set is, that it should
be double-zeta (basis='DZP'
) and that the confinement potential
should result in an energy shift of 0.01 Rydberg (the
energy_shift=0.01 * Ry
keyword). Sometimes it can be necessary to specify
more information on the basis set.
Defining Custom Species
Standard basis sets can be set by the keyword basis_set
directly, but for
anything more complex than one standard basis size for all elements,
a list of species
must be defined. Each specie is identified by atomic
element and the tag set on the atom.
For instance if we wish to investigate a H2 molecule and put a ghost atom (the basis set corresponding to an atom but without the actual atom) in the middle with a special type of basis set you would write:
>>> from ase.calculators.siesta.parameters import Specie, PAOBasisBlock
>>> from ase import Atoms
>>> from ase.calculators.siesta import Siesta
>>> atoms = Atoms(
... '3H',
... [(0.0, 0.0, 0.0),
... (0.0, 0.0, 0.5),
... (0.0, 0.0, 1.0)],
... cell=[10, 10, 10])
>>> atoms.set_tags([0, 1, 0])
>>>
>>> basis_set = PAOBasisBlock(
... """1
... 0 2 S 0.2
... 0.0 0.0""")
>>>
>>> siesta = Siesta(
... species=[
... Specie(symbol='H', tag=None, basis_set='SZ'),
... Specie(symbol='H', tag=1, basis_set=basis_set, ghost=True)])
>>>
>>> atoms.calc = siesta
When more species are defined, species defined with a tag has the highest priority.
General species with tag=None
has a lower priority.
Finally, if no species apply
to an atom, the general calculator keywords are used.
Pseudopotentials
Pseudopotential files in the .psf
or .vps
formats are needed.
Pseudopotentials generated from the ABINIT code and converted to
the SIESTA format are available in the SIESTA website.
A database of user contributed pseudopotentials is also available there.
Optimized GGA–PBE pseudos and DZP basis sets for some common elements are also available from the SIMUNE website.
You can also find an on-line pseudopotential generator from the OCTOPUS code.
Species can also be used to specify pseudopotentials:
>>> specie = Specie(symbol='H', tag=1, pseudopotential='H.example.psf')
When specifying the pseudopotential in this manner, both absolute and relative paths can be given. Relative paths are interpreted as relative to the set pseudopotential path.
Restarting from an old Calculation
If you want to rerun an old SIESTA calculation, whether made using the ASE
interface or not, you can set the keyword restart
to the siesta .XV
file. The keyword ignore_bad_restart
(True/False) will decide whether
a broken file will result in an error(False) or the whether the calculator
will simply continue without the restart file.
Choosing the coordinate format
If you are mainly using ASE to generate SIESTA files for relaxation with native SIESTA relaxation, you may want to write the coordinates in the Z-matrix format which will best allow you to use the advanced constraints present in SIESTA.
keyword |
type |
default value |
description |
---|---|---|---|
|
|
|
Choose between |
Siesta Calculator Class
- class ase.calculators.siesta.siesta.Siesta(command=None, profile=None, directory='.', **kwargs)[source]
Calculator interface to the SIESTA code.
ASE interface to the SIESTA code.
- Parameters:
label (-) – The basename of all files created during calculation.
mesh_cutoff (-) – Energy in eV. The mesh cutoff energy for determining number of grid points in the matrix-element calculation.
energy_shift (-) – Energy in eV The confining energy of the basis set generation.
kpts (-) – Tuple of 3 integers, the k-points in different directions.
xc (-) – The exchange-correlation potential. Can be set to any allowed value for either the Siesta XC.funtional or XC.authors keyword. Default “LDA”
basis_set (-) – “SZ”|”SZP”|”DZ”|”DZP”|”TZP”, strings which specify the type of functions basis set.
spin (-) – “non-polarized”|”collinear”| “non-collinear|spin-orbit”. The level of spin description to be used.
species (-) – None|list of Species objects. The species objects can be used to to specify the basis set, pseudopotential and whether the species is ghost. The tag on the atoms object and the element is used together to identify the species.
pseudo_path (-) – None|path. This path is where pseudopotentials are taken from. If None is given, then then the path given in $SIESTA_PP_PATH will be used.
pseudo_qualifier (-) – None|string. This string will be added to the pseudopotential path that will be retrieved. For hydrogen with qualifier “abc” the pseudopotential “H.abc.psf” will be retrieved.
symlink_pseudos (-) – None|bool If true, symlink pseudopotentials into the calculation directory, else copy them. Defaults to true on Unix and false on Windows.
atoms (-) – The Atoms object.
restart (-) – str. Prefix for restart file. May contain a directory. Default is None, don’t restart.
fdf_arguments (-) – Explicitly given fdf arguments. Dictonary using Siesta keywords as given in the manual. List values are written as fdf blocks with each element on a separate line, while tuples will write each element in a single line. ASE units are assumed in the input.
atomic_coord_format (-) – “xyz”|”zmatrix”, strings to switch between the default way of entering the system’s geometry (via the block AtomicCoordinatesAndAtomicSpecies) and a recent method via the block Zmatrix. The block Zmatrix allows to specify basic geometry constrains such as realized through the ASE classes FixAtom, FixedLine and FixedPlane.
Excited states calculations
The PyNAO code can be used to access excited state properties after having obtained the ground state properties with SIESTA. PyNAO allows to perform
Time Dependent Density Functional Theory (TDDFT) calculations
GW approximation calculations
Bethe-Salpeter equation (BSE) calculations.
Example of code to calculate polarizability of CH4 molecule:
from ase.calculators.siesta.siesta_lrtddft import SiestaLRTDDFT
from ase.build import molecule
import numpy as np
# Define the systems
ch4 = molecule('CH4')
lrtddft = SiestaLRTDDFT(label="siesta", xc_code='LDA,PZ')
# run DFT with siesta
lrtddft.get_ground_state(ch4)
# Run TDDFT with PyNAO
freq = np.arange(0.0, 25.0, 0.5)
pmat = lrtddft.get_polarizability(freq)
import matplotlib.pyplot as plt
plt.plot(freq, pmat[0, 0, :].imag)
plt.show()
Raman Calculations with SIESTA and PyNAO
It is possible to calculate the Raman spectra with SIESTA and PyNAO using the Raman function of the vibration module:
from ase.calculators.siesta.siesta_lrtddft import RamanCalculatorInterface
from ase.calculators.siesta import Siesta
from ase.vibrations.raman import StaticRamanCalculator
from ase.vibrations.placzek import PlaczekStatic
from ase.build import molecule
n2 = molecule('N2')
# enter siesta input
n2.calc = Siesta(
basis_set='DZP',
fdf_arguments={
'COOP.Write': True,
'WriteDenchar': True,
'XML.Write': True})
name = 'n2'
pynao_args = dict(label="siesta", jcutoff=7, iter_broadening=0.15,
xc_code='LDA,PZ', tol_loc=1e-6, tol_biloc=1e-7)
rm = StaticRamanCalculator(n2, RamanCalculatorInterface, name=name,
delta=0.011, exkwargs=pynao_args)
rm.run()
Pz = PlaczekStatic(n2, name=name)
e_vib = Pz.get_energies()
Pz.summary()
Further Examples
See also ase/test/calculators/siesta/lrtddft
for further examples
on how the calculator can be used.
Siesta lrtddft Class
- class ase.calculators.siesta.siesta_lrtddft.SiestaLRTDDFT(initialize=False, **kw)[source]
Interface for linear response TDDFT for Siesta via PyNAO
When using PyNAO please cite the papers indicated in the documentation
- Parameters:
initialize (bool) – To initialize the tddft calculations before calculating the polarizability Can be useful to calculate multiple frequency range without the need to recalculate the kernel
kw (dictionary) – keywords for the tddft_iter function from PyNAO
Siesta RamanCalculatorInterface Calculator Class
- class ase.calculators.siesta.siesta_lrtddft.RamanCalculatorInterface(omega=0.0, **kw)[source]
Raman interface for Siesta calculator. When using the Raman calculator, please cite
M. Walter and M. Moseler, Ab Initio Wavelength-Dependent Raman Spectra: Placzek Approximation and Beyond, J. Chem. Theory Comput. 2020, 16, 1, 576–586
- Parameters:
omega (float) – frequency at which the Raman intensity should be computed, in eV
kw (dictionary) – The parameter for the siesta_lrtddft object