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CCRESPONSE

Performs SCF linear response computations.

General

ABCD

Type of ABCD algorithm will be used

  • Type: string
  • Default: NEW

ANALYZE

Do analyze X2 amplitudes

CACHELEVEL

Cacheing level for libdpd

  • Type: integer
  • Default: 2

DIIS

Do use DIIS extrapolation to accelerate convergence?

GAUGE

Specifies the choice of representation of the electric dipole operator. Acceptable values are LENGTH for the usual length-gauge representation, VELOCITY 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 calculations, only the choices of VELOCITY or BOTH will yield origin-independent results.

  • Type: string
  • Possible Values: LENGTH, VELOCITY, BOTH
  • Default: LENGTH

LINEAR

Do Bartlett size-extensive linear model?

LOCAL

Do simulate local correlation?

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?

LOCAL_METHOD

Type of local-CCSD scheme to be simulated. WERNER (unique avaliable 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 avaliable 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, and AU.

  • Type: array
  • Default: No Default

PROPERTY

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, and AU.

  • Type: string
  • Possible Values: POLARIZABILITY, ROTATION, ROA, ALL
  • Default: POLARIZABILITY

REFERENCE

Reference wavefunction type

  • Type: string
  • Default: RHF

RESTART

Do restart from on-disk amplitudes?

R_CONVERGENCE

Convergence criterion for wavefunction (change) in perturbed CC equations.

SEKINO

Do Sekino-Bartlett size-extensive model-III?

Expert

WFN

Wavefunction type

  • Type: string
  • Default: SCF