CCENERGY¶
Computes coupled cluster energies. Called as part of any coupled cluster computation.
General¶
ABCD¶
Type of ABCD algorithm will be used
Type: string
Possible Values: NEW, OLD
Default: NEW
ANALYZE¶
Do analyze T2 amplitudes
Type: boolean
Default: false
BCCD_MAXITER¶
Maximum number of iterations for Brueckner CCD.
Type: integer
Default: 50
BRUECKNER_ORBS_R_CONVERGENCE¶
Convergence criterion for Brueckner orbitals. The convergence is determined based on the largest \(T_1\) amplitude. Default adjusts depending on E_CONVERGENCE
Type: conv double
Default: 1e-5
CACHELEVEL¶
Caching level for libdpd governing the storage of amplitudes, integrals, and intermediates in the CC procedure. A value of 0 retains no quantities in cache, while a level of 6 attempts to store all quantities in cache. For particularly large calculations, a value of 0 may help with certain types of memory problems. The default is 2, which means that all four-index quantities with up to two virtual-orbital indices (e.g., \(\langle ij | ab \rangle\) integrals) may be held in the cache.
Type: integer
Default: 2
CACHETYPE¶
Selects the priority type for maintaining the automatic memory cache used by the libdpd codes. A value of
LOW
selects a “low priority” scheme in which the deletion of items from the cache is based on pre-programmed priorities. A value of LRU selects a “least recently used” scheme in which the oldest item in the cache will be the first one deleted.
Type: string
Possible Values: LOW, LRU
Default: LOW
CC_NUM_THREADS¶
Number of threads
Type: integer
Default: 1
CC_OS_SCALE¶
Coupled-cluster opposite-spin scaling value
Type: double
Default: 1.27
CC_SS_SCALE¶
Coupled-cluster same-spin scaling value
Type: double
Default: 1.13
DIIS¶
Do use DIIS extrapolation to accelerate convergence?
Type: boolean
Default: true
E_CONVERGENCE¶
Convergence criterion for energy. See Table Post-SCF Convergence for default convergence criteria for different calculation types.
Type: conv double
Default: 1e-6
LOCAL¶
Do simulate the effects of local correlation techniques?
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: 0.02
LOCAL_METHOD¶
Type of local-CCSD scheme to be simulated.
WERNER
selects the method developed by H.-J. Werner and co-workers, andAOBASIS
selects the method developed by G.E. Scuseria and co-workers (currently inoperative).
Type: string
Possible Values: WERNER, AOBASIS
Default: WERNER
LOCAL_PAIRDEF¶
Definition of local pair domains, default is BP, Boughton-Pulay.
Type: string
Possible Values: BP, RESPONSE
Default: BP
LOCAL_WEAKP¶
Desired treatment of “weak pairs” in the local-CCSD method. A value of
NEGLECT
ignores weak pairs entirely. A value ofNONE
treats weak pairs in the same manner as strong pairs. A value of MP2 uses second-order perturbation theory to correct the local-CCSD energy computed with weak pairs ignored.
Type: string
Possible Values: NONE, NEGLECT, MP2
Default: NONE
MAXITER¶
Maximum number of iterations to solve the CC equations
Type: integer
Default: 50
MP2_AMPS_PRINT¶
Do print the MP2 amplitudes which are the starting guesses for RHF and UHF reference functions?
Type: boolean
Default: false
MP2_OS_SCALE¶
MP2 opposite-spin scaling value
Type: double
Default: 1.20
MP2_SS_SCALE¶
MP2 same-spin scaling value
Type: double
Default: 1.0
NEW_TRIPLES¶
Do use new triples?
Type: boolean
Default: true
NUM_AMPS_PRINT¶
Number of important \(t_1\) and \(t_2\) amplitudes to print
Type: integer
Default: 10
PAIR_ENERGIES_PRINT¶
Do print MP2 and CCSD pair energies for RHF references?
Type: boolean
Default: false
PROPERTY¶
The response property desired. Acceptable values are
POLARIZABILITY
(default) for dipole-polarizabilities,ROTATION
for specific rotations,ROA
for Raman Optical Activity, andALL
for all of the above.
Type: string
Possible Values: POLARIZABILITY, ROTATION, MAGNETIZABILITY, ROA, ALL
Default: POLARIZABILITY
REFERENCE¶
Reference wavefunction type
Type: string
Possible Values: RHF, ROHF, UHF
Default: RHF
RESTART¶
Do restart the coupled-cluster iterations from old \(t_1\) and \(t_2\) amplitudes? For geometry optimizations, Brueckner calculations, etc. the iterative solution of the CC amplitude equations may benefit considerably by reusing old vectors as initial guesses. Assuming that the MO phases remain the same between updates, the CC codes will, by default, re-use old vectors, unless the user sets RESTART = false.
Type: boolean
Default: true
R_CONVERGENCE¶
Convergence criterion for wavefunction (change) in CC amplitude equations.
Type: conv double
Default: 1e-7
SCSN_MP2¶
Do SCS-MP2 with parameters optimized for nucleic acids?
Type: boolean
Default: false
SCS_CCSD¶
Do spin-component-scaled CCSD
Type: boolean
Default: false
SCS_MP2¶
Do spin-component-scaled MP2 (SCS-MP2)?
Type: boolean
Default: false
SEMICANONICAL¶
Convert ROHF MOs to semicanonical MOs
Type: boolean
Default: true
SPINADAPT_ENERGIES¶
Do print spin-adapted pair energies?
Type: boolean
Default: false
T2_COUPLED¶
Type: boolean
Default: false
T3_WS_INCORE¶
Do build W intermediates required for cc3 in core memory?
Type: boolean
Default: false
Expert¶
AO_BASIS¶
The algorithm to use for the \(\left\langle VV||VV\right\rangle\) terms If AO_BASIS is
NONE
, the MO-basis integrals will be used; if AO_BASIS isDISK
, the AO-basis integrals stored on disk will be used; if AO_BASIS isDIRECT
, the AO-basis integrals will be computed on the fly as necessary. NB: TheDIRECT
option is not fully implemented and should only be used by experts. Default is NONE. Note: The developers recommend use of this keyword only as a last resort because it significantly slows the calculation. The current algorithms for handling the MO-basis four-virtual-index integrals have been significantly improved and are preferable to the AO-based approach.
Type: string
Possible Values: NONE, DISK, DIRECT
Default: NONE
FORCE_RESTART¶
Do restart the coupled-cluster iterations even if MO phases are screwed up?
Type: boolean
Default: false
WFN¶
Wavefunction type
Type: string
Default: NONE