Manual:RELCCSD:New input
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DIRAC-styleinput
The old namelist style input used up to DIRAC10 is replaced by an input that is more consistent with the rest of the input. In DIRAC11 it is possible to use both styles of inputs but we have the intention to phase out the namelist input in upcoming releases.
**RELCC
Specification of reference determinant, type of calculation, and general settings.
.FOCKSP
Activate the Fock space module. This option should be used for multireference calculations. See further CCFSPC
.ENERGY
Activate the energy calculation. This is the preferred option for calculations on closed shell or simple open shell systems.
Default:
No energy calculation.
.GRADIENT
Calculate the effective 1-particle density matrix (currently only for a closed shell MP2 wave function). This option can be used to calculate molecular properties.
Default:
No gradient calculation.
.NELEC
Specify the occupation of the reference determinant (both for CC and FSCC calculations). More information can be found here: NELEC
.NEL_F1
Number of electrons in the gerade irreps of the Abelian symmetry group. See also NELEC_F1
.NEL_F2
Number of electrons in the ungerade irreps of the Abelian symmetry group. See also NELEC_F2
Print level.
Default:
.PRINT 0
.DEBUG
Print debug information.
Default:
Debug information is not printed.
*CCENER
Covers options related to energy.
.DOMP2
Calculate the MP2 energy.
.MAXIT
Set maximum number of iterations allowed to solve the CC equations.
.MAXDIM
Set maximum number of amplitude vectors used in the DIIS extrapolation.
.NTOL
Specify requested convergence (10^-NTOL) in the amplitudes.
.NOSING
Eliminate T1 amplitudes in the calculation (only interesting for test purposes, this gives no computational speed-up).
.NODOUB
Eliminate T2 amplitudes in the calculation (only interesting for test purposes, this gives no computational speed-up).
*CCFOPR
Calculate first-order properties (expectation values) for the MP2 wave function.
*CCFSPC
Perform a Fock space MRCC calculation in which a model space is correlated and then diagonalized to give CC energies for a set of states.
.DOIH
Use the Intermediate Hamiltonian formalism in which an auxiliary space is used to prevent the "intruder state" problem. Default: IH formalism not used.
.DOEA
Calculate electron affinities (add one electron to the reference state, allowing occupation of the active virtual orbitals)
.DOIE
Calculate ionization energies (remove one electron from the reference state, allowing depletion of the active occupied orbitals)
.DOEA2
Calculate second electron affinities (add two electrons to the reference state, allowing occupation of the active virtual orbitals)
.DOIE2
Calculate second ionization energies (remove two electrons from the reference state, allowing depletion of the active occupied orbitals)
.DOEXC
Calculate excitation energies (allow excitation from the set of active occupied orbitals to the set of active virtual orbitals)
.NACTH
Specification of the set of active hole orbitals (from which ionization/excitation takes place)
.NACTP
Specification of the set of active particle orbitals (to which electron attachment/excitation takes place)
.MAXIT
Maximum number of iterations allowed to solve the FSCC equations
.MAXDIM
Set maximum number of amplitude vectors used in the DIIS extrapolation.
.NTOL
Specify requested convergence (10^-NTOL) in the amplitudes.
*CCIH
Options for intermediate hamiltonian in FSCC.
.EHMIN
Minimum orbital energy of occupied orbitals forming the auxiliary (Pi) space. Orbitals with energies lower than this energy are taken in the secundary (Q) space and do not contribute to the model space.
.EHMAX
Maximum orbital energy of occupied orbitals forming the auxiliary (Pi) space. Orbitals with energies higher than this energy are taken in the primary (Pm) space.
.EPMIN
Minimum orbital energy of virtual orbitals forming the auxiliary (Pi) space. Orbitals with energies lower than this energy are taken in the primary (Pm) space.
.EPMAX
Maximum orbital energy of virtual orbitals forming the auxiliary (Pi) space. Orbitals with energies higher than this energy are taken in the secundary (Q) space and do not contribute to the model space.
