CCRESPONSE¶
Performs SCF linear response computations.
General¶
ABCD¶
Type of ABCD algorithm will be used
Type: string
Default: NEW
ANALYZE¶
Do analyze X2 amplitudes
Type: boolean
Default: false
CACHELEVEL¶
Caching level for libdpd
Type: integer
Default: 2
DIIS¶
Do use DIIS extrapolation to accelerate convergence?
Type: boolean
Default: true
GAUGE¶
Specifies the choice of representation of the electric dipole operator. For polarizability, this keyword is ignored and
LENGTH
gauge is computed. For optical rotation and raman optical activity, this keyword is active, and acceptable values areLENGTH
for the usual length-gauge representation,VELOCITY``(default) for the modified velocity-gauge representation in which the static-limit optical rotation tensor is subtracted from the frequency- dependent tensor, or ``BOTH
. Note that, for optical rotation and raman optical activity calculations, only the choices ofVELOCITY
orBOTH
will yield origin-independent results.
Type: string
Possible Values: LENGTH, VELOCITY, BOTH
Default: VELOCITY
LINEAR¶
Do Bartlett size-extensive linear model?
Type: boolean
Default: false
LOCAL¶
Do simulate local correlation?
Type: boolean
Default: false
LOCAL_CPHF_CUTOFF¶
Cutoff value for local-coupled-perturbed-Hartree-Fock
Type: double
Default: 0.10
LOCAL_CUTOFF¶
Value (always between one and zero) for the Broughton-Pulay completeness check used to contruct orbital domains for local-CC calculations. See J. Broughton and P. Pulay, J. Comp. Chem. 14, 736-740 (1993) and C. Hampel and H.-J. Werner, J. Chem. Phys. 104, 6286-6297 (1996).
Type: double
Default: 0.01
LOCAL_FILTER_SINGLES¶
Do apply local filtering to single excitation amplitudes?
Type: boolean
Default: false
LOCAL_METHOD¶
Type of local-CCSD scheme to be simulated.
WERNER
(unique available option) selects the method developed by H.-J. Werner and co-workers.
Type: string
Default: WERNER
LOCAL_PAIRDEF¶
Definition of local pair domains
Type: string
Default: NONE
LOCAL_WEAKP¶
Desired treatment of “weak pairs” in the local-CCSD method. The value of
NONE
(unique available option) treats weak pairs in the same manner as strong pairs.
Type: string
Default: NONE
MAXITER¶
Maximum number of iterations to converge perturbed amplitude equations
Type: integer
Default: 50
NUM_AMPS_PRINT¶
Number of important CC amplitudes per excitation level to print. CC analog to NUM_DETS_PRINT
Type: integer
Default: 5
OMEGA¶
Array that specifies the desired frequencies of the incident radiation field in CCLR calculations. If only one element is given, the units will be assumed to be atomic units. If more than one element is given, then the units must be specified as the final element of the array. Acceptable units are
HZ
,NM
,EV
, andAU
.
Type: array
Default: No Default
PROPERTY¶
The response property desired. Acceptable values are
POLARIZABILITY
(default) for dipole polarizabilities,ROTATION
for specific rotations,ROA
for Raman Optical Activity (ROA_TENSOR
for each displacement), andALL
for all of the above.
Type: string
Possible Values: POLARIZABILITY, ROTATION, ROA, ROA_TENSOR, ALL
Default: POLARIZABILITY
REFERENCE¶
Reference wavefunction type
Type: string
Default: RHF
RESTART¶
Do restart from on-disk amplitudes?
Type: boolean
Default: true
R_CONVERGENCE¶
Convergence criterion for wavefunction (change) in perturbed CC equations.
Type: conv double
Default: 1e-7
SEKINO¶
Do Sekino-Bartlett size-extensive model-III?
Type: boolean
Default: false
Expert¶
WFN¶
Wavefunction type
Type: string
Default: SCF