User input reference¶
Keywords without a default value are required.
Default values are either explicit or computed from the value of other keywords in the input.
Sections where all keywords have a default value can be omitted.
Predicates, if present, are the functions run to validate user input.
- Keywords
- world_prec
Overall relative precision in the calculation.
Type
float- Predicates
1.0e-10 < value < 1.0
- world_size
Total size of computational domain given as 2**(
world_size). Always cubic and symmetric around the origin. Negative value means it will be computed from the molecular geometry.Type
intDefault
-1- Predicates
value <= 10
- world_unit
Length unit for all coordinates given in user input. Everything will be converted to atomic units (bohr) before the main executable is launched, so the JSON input is always given in bohrs.
Type
strDefault
bohr- Predicates
value.lower() in ["bohr", "angstrom"]
- world_origin
Global gauge origin of the calculation.
Type
List[float]Default
[0.0, 0.0, 0.0]- Predicates
len(value) == 3
- Sections
- Precisions
Define specific precision parameters.
- Keywords
- exchange_prec
Precision parameter used in construction of Exchange operators. Negative value means it will follow the dynamic precision in SCF.
Type
floatDefault
-1.0- helmholtz_prec
Precision parameter used in construction of Helmholtz operators. Negative value means it will follow the dynamic precision in SCF.
Type
floatDefault
-1.0- poisson_prec
Precision parameter used in construction of Poisson operators.
Type
floatDefault
user['world_prec']- Predicates
1.0e-10 < value < 1.0
- nuclear_prec
Precision parameter used in smoothing and projection of nuclear potential.
Type
floatDefault
user['world_prec']- Predicates
1.0e-10 < value < 1.0
- Printer
Define variables for printed output.
- Keywords
- print_level
Level of detail in the written output. Level 0 for production calculations, negative level for complete silence.
Type
intDefault
0- print_mpi
Write separate output from each MPI to file called
<file_name>-<mpi-rank>.out.Type
boolDefault
False- print_prec
Number of digits in property output (energies will get twice this number of digits).
Type
intDefault
6- Predicates
0 < value < 10
- print_width
Line width of printed output (in number of characters).
Type
intDefault
75- Predicates
50 < value < 100
- print_constants
Print table of physical constants used by MRChem.
Type
boolDefault
False
- Plotter
Give details regarding the density and orbital plots. Three types of plots are available, line, surface and cube, and the plotting ranges are defined by three vectors (A, B and C) and an origin (O):
line: plots on line spanned by A, starting from O.surf: plots on surface spanned by A and B, starting from O.cube: plots on volume spanned by A, B and C, starting from O.- Keywords
- path
File path to plot directory.
Type
strDefault
plots- Predicates
value[-1] != '/'
- type
Type of plot: line (1D), surface (2D) or cube (3D).
Type
strDefault
cube- Predicates
value.lower() in ['line', 'surf', 'cube']
- points
Number of points in each direction on the cube grid.
Type
List[int]Default
[20, 20, 20]- Predicates
all(p > 0 for p in value)not (user['Plotter']['type'] == 'line' and len(value) < 1)not (user['Plotter']['type'] == 'surf' and len(value) < 2)not (user['Plotter']['type'] == 'cube' and len(value) < 3)
- O
Origin of plotting ranges.
Type
List[float]Default
[0.0, 0.0, 0.0]- Predicates
len(value) == 3
- A
First boundary vector for plot.
Type
List[float]Default
[1.0, 0.0, 0.0]- Predicates
len(value) == 3
- B
Second boundary vector for plot.
Type
List[float]Default
[0.0, 1.0, 0.0]- Predicates
len(value) == 3
- C
Third boundary vector for plot.
Type
List[float]Default
[0.0, 0.0, 1.0]- Predicates
len(value) == 3
- MPI
Define MPI related parameters.
- Keywords
- numerically_exact
This will use MPI algorithms that guarantees that the output is invariant wrt the number of MPI processes.
Type
boolDefault
False- shared_memory_size
Size (MB) of the MPI shared memory blocks of each shared function.
Type
intDefault
10000- share_nuclear_potential
This will use MPI shared memory for the nuclear potential.
Type
boolDefault
False- share_coulomb_potential
This will use MPI shared memory for the Coulomb potential.
Type
boolDefault
False- share_xc_potential
This will use MPI shared memory for the exchange-correlation potential.
Type
boolDefault
False- bank_size
Number of MPI processes exclusively dedicated to manage orbital bank.
Type
intDefault
-1
- Basis
Define polynomial basis.
- Keywords
- order
Polynomial order of multiwavelet basis. Negative value means it will be set automatically based on the world precision.
Type
intDefault
-1- type
Polynomial type of multiwavelet basis.
Type
strDefault
interpolating- Predicates
value.lower() in ['interpolating', 'legendre']
- Derivatives
Define various derivative operators used in the code.
- Keywords
- kinetic
Derivative used in kinetic operator.
Type
strDefault
abgv_55- h_b_dip
Derivative used in magnetic dipole operator.
Type
strDefault
abgv_00- h_m_pso
Derivative used in paramagnetic spin-orbit operator.
Type
strDefault
abgv_00- zora
Derivative used ZORA potential.
Type
strDefault
abgv_00
- Molecule
Define molecule.
- Keywords
- charge
Total charge of molecule.
Type
intDefault
0- multiplicity
Spin multiplicity of molecule.
Type
intDefault
1- Predicates
value > 0
- translate
Translate coordinates such that center of mass coincides with the global gauge origin.
Type
boolDefault
False- coords
Coordinates in xyz format. Atoms can be given either using atom symbol or atom number
Type
str
- WaveFunction
Define the wavefunction method.
- Keywords
- method
Wavefunction method. See predicates for valid methods.
hf,hartreefockandhartree-fockall mean the same thing, whileldais an alias forsvwn5. You can set a non-standard DFT functional (e.g. varying the amount of exact exchange) by choosingdftand specifing the functional(s) in theDFTsection below.Type
str- Predicates
value.lower() in ['core', 'hartree', 'hf', 'hartreefock', 'hartree-fock', 'dft', 'lda', 'svwn3', 'svwn5', 'pbe', 'pbe0', 'bpw91', 'bp86', 'b3p86', 'b3p86-g', 'blyp', 'b3lyp', 'b3lyp-g', 'olyp', 'kt1', 'kt2', 'kt3']
- restricted
Use spin restricted wavefunction.
Type
boolDefault
True- relativity
Set method for relativistic treatment.
ZORAfor fully self-consistent ZORA potential, by default including all potentials (V_nuc,J,V_xc) but this can be overwritten in theZORAsection.nZORAis shortcut for nuclear-ZORA, i.e. onlyV_nucis included (this keyword takes precedence over keywords in theZORAsection).Type
strDefault
none- Predicates
value.lower() in ['none', 'zora', 'nzora']
- environment
Set method for treatment of environment.
nonefor vacuum calculation.PCMfor Polarizable Continuum Model, which will activate thePCMinput section for further parametrization options.Type
strDefault
none- Predicates
value.lower() in ['none', 'pcm']
- nuclear_model
Type of nucleus model. Point-like (numerical smoothing): HFYGB (default), parabola or minimal. Finite models (physical smoothing): Gaussian or Homogeneous sphere Finite models are derived from nuclear RMS radius, Visscher (1997)
Type
strDefault
point_like- Predicates
value.lower() in ['point_like', 'point_parabola', 'point_minimal', 'finite_gaussian', 'finite_sphere']
- ZORA
Define required parameters for the ZORA Hamiltonian.
- Keywords
- include_nuclear
Include the nuclear potential
V_nucin the ZORA potential.Type
boolDefault
True- include_coulomb
Include the Coulomb potential
Jin the ZORA potential.Type
boolDefault
True- include_xc
Include the XC potential
V_xcin the ZORA potential.Type
boolDefault
True
- DFT
Define the exchange-correlation functional in case of DFT.
- Keywords
- density_cutoff
Hard cutoff for passing density values to XCFun.
Type
floatDefault
0.0- functionals
List of density functionals with numerical coefficient. E.g. for PBE0
EXX 0.25,PBEX 0.75,PBEC 1.0, see XCFun documentation <https://xcfun.readthedocs.io/>_.Type
strDefault `` ``
- spin
Use spin separated density functionals.
Type
boolDefault
not(user['WaveFunction']['restricted'])
- Properties
Provide a list of properties to compute (total SCF energy and orbital energies are always computed).
- Keywords
- dipole_moment
Compute dipole moment.
Type
boolDefault
True- quadrupole_moment
Compute quadrupole moment. Note: Gauge origin dependent, should be used with
translate = truein Molecule.Type
boolDefault
False- polarizability
Compute polarizability tensor.
Type
boolDefault
False- magnetizability
Compute magnetizability tensor.
Type
boolDefault
False- nmr_shielding
Compute NMR shielding tensor.
Type
boolDefault
False- geometric_derivative
Compute geometric derivative.
Type
boolDefault
False- plot_density
Plot converged electron density.
Type
boolDefault
False- plot_orbitals
Plot converged molecular orbitals from list of indices, negative index plots all orbitals.
Type
List[int]Default
[]
- ExternalFields
Define external electromagnetic fields.
- Keywords
- electric_field
Strength of external electric field.
Type
List[float]Default
[]- Predicates
len(value) == 0 or len(value) == 3
- Polarizability
Give details regarding the polarizability calculation.
- Keywords
- frequency
List of external field frequencies.
Type
List[float]Default
[0.0]
- NMRShielding
Give details regarding the NMR shileding calculation.
- Keywords
- nuclear_specific
Use nuclear specific perturbation operator (h_m_pso).
Type
boolDefault
False- nucleus_k
List of nuclei to compute. Negative value computes all nuclei.
Type
List[int]Default
[-1]
- Files
Defines file paths used for program input/output. Note: all paths must be given in quotes if they contain slashes “path/to/file”.
- Keywords
- guess_basis
File name for GTO basis set, used with
gtoguess.Type
strDefault
initial_guess/mrchem.bas- guess_gto_p
File name for paired orbitals, used with
gtoguess.Type
strDefault
initial_guess/mrchem.mop- guess_gto_a
File name for alpha orbitals, used with
gtoguess.Type
strDefault
initial_guess/mrchem.moa- guess_gto_b
File name for beta orbitals, used with
gtoguess.Type
strDefault
initial_guess/mrchem.mob- guess_phi_p
File name for paired orbitals, used with
mwguess. Expected path is ``<path_orbitals>/phi_p_scf_idx_<0…Np>_<re/im>.mwType
strDefault
initial_guess/phi_p- guess_phi_a
File name for alpha orbitals, used with
mwguess. Expected path is ``<path_orbitals>/phi_a_scf_idx_<0…Na>_<re/im>.mwType
strDefault
initial_guess/phi_a- guess_phi_b
File name for beta orbitals, used with
mwguess. Expected path is ``<path_orbitals>/phi_b_scf_idx_<0…Nb>_<re/im>.mwType
strDefault
initial_guess/phi_b- guess_x_p
File name for paired response orbitals, used with
mwguess. Expected path is ``<path_orbitals>/x_p_rsp_idx_<0…Np>_<re/im>.mwType
strDefault
initial_guess/X_p- guess_x_a
File name for alpha response orbitals, used with
mwguess. Expected path is ``<path_orbitals>/x_a_rsp_idx_<0…Na>_<re/im>.mwType
strDefault
initial_guess/X_a- guess_x_b
File name for beta response orbitals, used with
mwguess. Expected path is ``<path_orbitals>/x_b_rsp_idx_<0…Nb>_<re/im>.mwType
strDefault
initial_guess/X_b- guess_y_p
File name for paired response orbitals, used with
mwguess. Expected path is ``<path_orbitals>/y_p_rsp_idx_<0…Np>_<re/im>.mwType
strDefault
initial_guess/Y_p- guess_y_a
File name for alpha response orbitals, used with
mwguess. Expected path is ``<path_orbitals>/y_a_rsp_idx_<0…Na>_<re/im>.mwType
strDefault
initial_guess/Y_a- guess_y_b
File name for beta response orbitals, used with
mwguess. Expected path is ``<path_orbitals>/y_b_rsp_idx_<0…Nb>_<re/im>.mwType
strDefault
initial_guess/Y_b- guess_cube_p
File name for paired orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/phi_p_scf_idx_<0…Np>_<re/im>.cube where Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/phi_p- guess_cube_a
File name for alpha orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/phi_a_scf_idx_<0…Na>_<re/im>.cube where Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/phi_a- guess_cube_b
File name for beta orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/phi_b_scf_idx_<0…Nb>_<re/im>.cube where Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/phi_b- guess_cube_x_p
File name for paired response orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/x_p_rsp_<0,1,2>_<0…Np>_<re/im>.cube where 0,1,2 indicate the index of the components of the response vectors. Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/x_p- guess_cube_x_a
File name for alpha response orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/x_a_rsp_<0,1,2>_<0…Na>_<re/im>.cube where 0,1,2 indicate the index of the components of the response vectors. Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/x_a- guess_cube_x_b
File name for beta response orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/x_b_rsp_<0,1,2>_<0…Nb>_<re/im>.cube where 0,1,2 indicate the index of the components of the response vectors. Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/x_b- guess_cube_y_p
File name for paired response orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/y_p_rsp_<0,1,2>_<0…Np>_<re/im>.cube where 0,1,2 indicate the index of the components of the response vectors. Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/y_p- guess_cube_y_a
File name for alpha response orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/y_a_rsp_<0,1,2>_<0…Na>_<re/im>.cube where 0,1,2 indicate the index of the components of the response vectors. Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/y_a- guess_cube_y_b
File name for beta response orbitals, used with
cubeguess. Expected path is ``<path_orbitals>/y_b_rsp_<0,1,2>_<0…Nb>_<re/im>.cube where 0,1,2 indicate the index of the components of the response vectors. Np is the number of orbitals and re/im denote real or imaginary parts.Type
strDefault
initial_guess/y_b- cube_vectors
Directory where cube vectors are stored for mrchem calculation.
Type
strDefault
cube_vectors/
- SCF
Includes parameters related to the ground state SCF orbital optimization.
- Keywords
- run
Run SCF solver. Otherwise properties are computed on the initial orbitals.
Type
boolDefault
True- max_iter
Maximum number of SCF iterations.
Type
intDefault
100- kain
Length of KAIN iterative history.
Type
intDefault
5- rotation
Number of iterations between each diagonalization/localization.
Type
intDefault
0- localize
Use canonical or localized orbitals.
Type
boolDefault
False- energy_thrs
Convergence threshold for SCF energy.
Type
floatDefault
-1.0- guess_prec
Precision parameter used in construction of initial guess.
Type
floatDefault
0.001- Predicates
1.0e-10 < value < 1.0
- guess_screen
Screening parameter used in GTO evaluations, in number of standard deviations. Every coordinate beyond N StdDev from the Gaussian center is evaluated to zero. Note that too aggressive screening is counter productive, because it leads to a sharp cutoff in the resulting function which requires higher grid refinement. Negative value means no screening.
Type
floatDefault
12.0- start_prec
Incremental precision in SCF iterations, initial value.
Type
floatDefault
-1.0- final_prec
Incremental precision in SCF iterations, final value.
Type
floatDefault
-1.0- guess_type
Type of initial guess for ground state orbitals.
chkrestarts a previous calculation which was dumped using thewrite_checkpointkeyword. This will load MRA and electron spin configuration directly from the checkpoint files, which are thus required to be identical in the two calculations.mwwill start from final orbitals in a previous calculation written using thewrite_orbitalskeyword. The orbitals will be re-projected into the new computational setup, which means that the electron spin configuration and MRA can be different in the two calculations.gtoreads precomputed GTO orbitals (requires extra non-standard input files for basis set and MO coefficients).coreandsadwill diagonalize the Fock matrix in the given AO basis (SZ, DZ, TZ or QZ) using a Core or Superposition of Atomic Densities Hamiltonian, respectively.cubewill start from orbitals saved in cubefiles from external calculations.Type
strDefault
sad_gto- Predicates
value.lower() in ['mw', 'chk', 'gto', 'core_sz', 'core_dz', 'core_tz', 'core_qz', 'sad_sz', 'sad_dz', 'sad_tz', 'sad_qz', 'sad_gto', 'cube']
- write_checkpoint
Write orbitals to disk in each iteration, file name
<path_checkpoint>/phi_scf_idx_<0..N>. Can be used aschkinitial guess in subsequent calculations. Note: must be given in quotes if there are slashes in the path “path/to/checkpoint”.Type
boolDefault
False- path_checkpoint
Path to checkpoint files during SCF, used with
write_checkpointandchkguess.Type
strDefault
checkpoint- Predicates
value[-1] != '/'
- write_orbitals
Write final orbitals to disk, file name
<path_orbitals>/phi_<p/a/b>_scf_idx_<0..Np/Na/Nb>. Can be used asmwinitial guess in subsequent calculations.Type
boolDefault
False- path_orbitals
Path to where converged orbitals will be written in connection with the
write_orbitalskeyword. Note: must be given in quotes if there are slashes in the path “path/to/orbitals”.Type
strDefault
orbitals- Predicates
value[-1] != '/'
- orbital_thrs
Convergence threshold for orbital residuals.
Type
floatDefault
10 * user['world_prec']
- Response
Includes parameters related to the response SCF optimization.
- Keywords
- run
In which Cartesian directions to run response solver.
Type
List[bool]Default
[True, True, True]- max_iter
Maximum number of response iterations.
Type
intDefault
100- kain
Length of KAIN iterative history.
Type
intDefault
5- property_thrs
Convergence threshold for symmetric property. Symmetric meaning the property computed from the same operator as the response purturbation, e.g. for external magnetic field the symmetric property corresponds to the magnetizability (NMR shielding in non-symmetric, since one of the operators is external magnetic field, while the other is nuclear magnetic moment).
Type
floatDefault
-1.0- start_prec
Incremental precision in SCF iterations, initial value.
Type
floatDefault
-1.0- final_prec
Incremental precision in SCF iterations, final value.
Type
floatDefault
-1.0- guess_prec
Precision parameter used in construction of initial guess.
Type
floatDefault
0.001- Predicates
1.0e-10 < value < 1.0
- guess_type
Type of initial guess for response.
nonewill start from a zero guess for the response functions.chkrestarts a previous calculation which was dumped using thewrite_checkpointkeyword.mwwill start from final orbitals in a previous calculation written using thewrite_orbitalskeyword. The orbitals will be re-projected into the new computational setup.Type
strDefault
none- Predicates
value.lower() in ['none', 'chk', 'mw', 'cube']
- write_checkpoint
Write perturbed orbitals to disk in each iteration, file name
<path_checkpoint>/<X/Y>_rsp_<direction>_idx_<0..N>. Can be used aschkinitial guess in subsequent calculations.Type
boolDefault
False- path_checkpoint
Path to checkpoint files during SCF, used with
write_checkpointandchkguess.Type
strDefault
checkpoint- Predicates
value[-1] != '/'
- write_orbitals
Write final perturbed orbitals to disk, file name
<path_orbitals>/<X/Y>_<p/a/b>_rsp_<direction>_idx_<0..Np/Na/Nb>. Can be used asmwinitial guess in subsequent calculations.Type
boolDefault
False- path_orbitals
Path to where converged orbitals will be written in connection with the
write_orbitalskeyword.Type
strDefault
orbitals- Predicates
value[-1] != '/'
- orbital_thrs
Convergence threshold for orbital residuals.
Type
floatDefault
10 * user['world_prec']- localize
Use canonical or localized unperturbed orbitals.
Type
boolDefault
user['SCF']['localize']
- PCM
Includes parameters related to the computation of the reaction field energy of a system in an environment within the Polarizable Continuum Model.
- Sections
- SCRF
Parameters for the Self-Consistent Reaction Field optimization.
- Keywords
- max_iter
Max number of iterations allowed in the nested procedure.
Type
intDefault
100- dynamic_thrs
Set the convergence threshold for the nested procedure.
truewill dynamically tighten the convergence threshold based on the absolute value of the latest orbital update as. When the orbitals are close to convergence (mo_residual < world_prec*10) the convergence threshold will be set equal toworld_prec.falseusesworld_precas convergence threshold throughout.Type
boolDefault
True- optimizer
Choose which function to use in the KAIN solver, the surface charge
density(gamma) or the reactionpotential(V_R).Type
strDefault
potential- Predicates
value.lower() in ['density', 'potential']
- density_type
What part of the total molecular charge density to use in the algorithm.
totaluses the total charge density.nuclearuses only the nuclear part of the total charge density.electronicuses only the electronic part of the total charge density.Type
strDefault
total- Predicates
value.lower() in ['total', 'nuclear', 'electronic']
- kain
Number of previous reaction field iterates kept for convergence acceleration during the nested precedure.
Type
intDefault
user['SCF']['kain']
- Cavity
Define the interlocking spheres cavity.
- Keywords
- mode
Determines how to set up the interlocking spheres cavity.
atoms: centers are taken from the molecular geometry, radii taken from tabulated data (van der Waals radius), and rescaled using the parametersalpha,betaandsigma(R_i <- alpha*R_i + beta*sigma). Default spheres can be modified and/or extra spheres added, using the $spheres section, see documentation.explicit: centers and radii given explicitly in thespheresblock.Type
strDefault
atoms- Predicates
value.lower() in ['atoms', 'explicit']
- spheres
This input parameter affects the list of spheres used to generate the cavity. In all cases, values for the radius, the radius scaling factor (
alpha), the width (sigma), and the width scaling factor (beta) can be modified. If they are not specified their global default values are used. Inatomsmode, we modify the default list of spheres, built with centers from the molecular geometry and radii from internal tabulated van der Waals values. To substitute a sphere, include a line like: $spheres i R [alpha] [beta] [sigma] $end to specify that theiatom in the molecule (0-based indexing) should use radiusRinstead of the pre-tabulated vdW radius. To add a sphere, include a line like: $spheres x y z R [alpha] [beta] [sigma] $end to specify that a sphere of radiusRshould be added at position(x, y, z). Spheres added in this way are not aware of their parent atom, if any. They will not contribute to the molecular gradient. Inexplicitmode, we build the complete sphere list from scratch. You can add a line like: $spheres x y z R [alpha] [beta] [sigma] $end to specify that a sphere of radiusRshould be added at position(x, y, z). Spheres added in this way are not aware of their parent atom, if any. They will not contribute to the molecular gradient. Alternatively, you can specify a line like: $spheres i R [alpha] [beta] [sigma] $end to specify that theiatom in the molecule (0-based indexing) should use radiusR. Spheres added in this way are aware of their parent atom. They will contribute to the molecular gradient.Type
str- alpha
Scaling factor on the radius term for the cavity rescaling (R_i <- alpha*R_i + beta*sigma). Only used for the default vdW radii in atoms mode, not if explicit
$spheresare given.Type
floatDefault
1.1- beta
Scaling factor on the boundary width term for the cavity rescaling (R_i <- alpha*R_i + beta*sigma). Only used for the default vdW radii in atoms mode, not if explicit
$spheresare given.Type
floatDefault
0.5- sigma
Width of cavity boundary, smaller value means sharper transition.
Type
floatDefault
0.2
- Permittivity
Parameters for the permittivity function.
- Keywords
- epsilon_in
Permittivity inside the cavity. 1.0 is the permittivity of free space, anything other than this is undefined behaviour.
Type
floatDefault
1.0- epsilon_out
Permittivity outside the cavity. This is characteristic of the solvent used.
Type
floatDefault
1.0- formulation
Formulation of the Permittivity function. Currently only the exponential is used.
Type
strDefault
exponential- Predicates
value.lower() in ['exponential']
- Constants
Physical and mathematical constants used by MRChem
- Keywords
- hartree2simagnetizability
- Conversion factor for magnetizability from atomic units to SI units (unit: J T^-2). Affected code: Printed value of the magnetizability property.
Type
floatDefault
78.9451185 - light_speed
- Speed of light in atomic units (unit: au). Affected code: Relativistic Hamiltonians (ZORA, etc.)
Type
floatDefault
137.035999084 - angstrom2bohrs
- Conversion factor for Cartesian coordinates from Angstrom to Bohr (unit: Å^-1). Affected code: Parsing of input coordinates, printed coordinates
Type
floatDefault
1.8897261246257702 - hartree2kjmol
- Conversion factor from Hartree to kJ/mol (unit: kJ mol^-1). Affected code: Printed value of energies.
Type
floatDefault
2625.4996394798254 - hartree2kcalmol
- Conversion factor from Hartree to kcal/mol (unit: kcal mol^-1). Affected code: Printed value of energies.
Type
floatDefault
627.5094740630558 - hartree2ev
- Conversion factor from Hartree to eV (unit: ev). Affected code: Printed value of energies.
Type
floatDefault
27.211386245988 - hartree2wavenumbers
- Conversion factor from Hartree to wavenumbers (unit: cm^-1). Affected code: Printed value of frequencies.
Type
floatDefault
219474.6313632 - fine_structure_constant
- Fine-structure constant in atomic units (unit: au). Affected code: Certain magnetic interaction operators.
Type
floatDefault
0.0072973525693 - electron_g_factor
- Electron g factor in atomic units (unit: au). Affected code: Certain magnetic interaction operators.
Type
floatDefault
-2.00231930436256 - dipmom_au2debye
- Conversion factor for dipoles from atomic units to Debye (unit: ?). Affected code: Printed value of dipole moments.
Type
floatDefault
2.5417464739297717