Kramers unrestricted Coupled-Cluster methods

See [Visscher1996] for the initial CCSD(T) implementation. The Fock-space CC implementation is described in [Visscher2001].

**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. Because the first sector of Fock space gives the same result as a regular CCSD calculation, the latter calculation is switched off. If you do wish to perform also a regular CC calculation (e.g. to get the CCSD(T) energy) you need to activate this explicitly via .ENERGY (see below).

.ENERGY

Activate the energy calculation. This is the preferred option for calculations on closed shell or simple open shell systems and need not be specified explictly in such cases. For Fock space calculations the keyword switches on a separate single reference calculation done prior to the FS calculation.

Default:

Perform energy calculation.

.GRADIENT

Calculate the effective 1-particle density matrix. This option can be used to calculate molecular properties. For closed-shell MP2 see [vanStralen2005]. For closed-shell CC see [Shee2016].

Default:

No gradient calculation.

.EOMCC

Activate the equation of motion (EOMCC) module. This option can be used to obtain excitation energies (EOM-EE), singly ionized (EOM-IP) and electron attached (EOM-EA) states starting from a closed shell reference and at the CCSD level, by solving for the right-hand eigenvalues and eigenvectors of the appropriate similarity-transformed Hamiltonian.

Unlike in Fock-space calculations, where the full model Hamiltonian for each sector is diagonalized, in EOMCC the user must specify the desired number of roots per symmetry, (see *EOMCC for further details) and these are determined via matrix-free diagonalization procedures such as the Davidson method (see *CCDIAG for the options available).

Default:

No EOM-CC calculation.

.EOMPROP

Warning

Development version only.

Activate the calculation of excited-state first-order properties for the EOMCC module for CCSD wavefunctions, by solving for the left-hand eigenvectors of the corresponding similarity-transformed Hamiltonian. It should be specified along with .EOMCC as it requires the right-hand eigenvectors and, as such, the same type of calculation (EOM-EE/IP/EA) will be performed. See *EOMPROP for further details.

Default:

No EOM-CC excited-state expectation value calculation.

.NELEC

Number of correlated electrons. This variable determines the reference determinant to be used in the exponential expansion of the wave function. Since the default values correspond to the information passed on by the MOLTRA code on basis of the Hartree-Fock occupations and chosen range of active orbitals in MOLTRA, for CLOSED SHELL systems there is usually no need to specify this variable manually. If you do chose to specify this manually, you should make sure to count electrons carefully as the numbers relate to the number of correlated electrons rather than the total number. This number may therefore change if you change tresholds in the integral transformation.

For OPEN SHELL systems it is usually better to employ the multireference Fock space approach, except for simple cases such as a high-spin open shell state. In this case the single reference CCSD(T) ansatz works rater well. For such cases it is easier to use the .NELEC_OPEN keyword that allows to just specify the distribution of open shell electrons over the irreps, but for backwards compatibility we retain the older NELEC option as well.

Arguments:

Integer (NELEC(I),I=1,NFSYM*2).

Default:

Number of correlated electrons in closed shells in these irreps (written by **MOLTRA).

.NELEC_OPEN

Distribution of correlated open shell electrons over the irreps. This determines the reference determinant for open shell single reference calculations.

This input should always be given for average-of-configuration SCF calculations that are followed by a CC calculation. The total number of electrons that is given should correspond to the number of open shell electrons.

Arguments:

Integer (NELEC_OPEN(I),I=1,NFSYM*2).

Default:

Zero. (note that this default leads to wrong results because a closed shell ion will be calculated if no input is given).

.NEL_F1

Number of electrons in the gerade irreps of the Abelian symmetry group. This works like the NELEC keyword, but uses the supersymmetry possible for linear groups in which irreps are ordered as 1/2, -1/2, 3/2, -3/2, 5/2, ... (with the number being the m_j value).

.NEL_F2

Number of electrons in the ungerade irreps of the Abelian symmetry group.

.PRINT

Print level.

Default:

.PRINT
 0

.COUNTMEM

Stop CC module after counting the total memory demand. Needs only MRCONEE.

.TIMING

Print detailed timing information.

Default:

Only limited timing information is printed.

.DEBUG

Print debug information.

Default:

Debug information is not printed.

.RESTART

Reuses information from prior calculations to resume the calculation from the last sucessfully recorded checkpoint. In order for a restart to be possible, the appropriate files from both the 4-index transformation - e.g. MRCONEE, MDCINT (and MDCINX* for parallel runs) and, if the transformation of property operators was requested, MDPROP - and from the previous coupled cluster run (ft.* for the sorting of integrals, MCCRES* for the amplitudes) have to be present at the scratch directory. Given the size and number of these files, this means in practice one must request the the scratch directory is kept at the end of the runs (see the pam script options for details)

Default:

No restart is performed.

.NOSORT

Forces the code to skip the sorting of integrals coming from the 4-index transformation into six integral classes. Using this option without the integral sorting stap having been properly carried out may produce incorrect results.

Default:

Sorting of integrals into classes is performed.

*CCENER

Covers options related to energy.

.NOMP2

Deactivate MP2 calculation.

.NOSD

Deactivate CCSD calculation.

.NOSDT

Deactivate the calculation of perturbative triples. This is potentially useful when running into memory problems for very big calculations and will also save some CPU time.

.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). Deactivate contribution from doubles; corresponds to a CCS calculation.

*CCFOPR

Calculate first-order properties (expectation values) for the MP2 and CCSD wave function.

.MP2G

Use MP2 wave function.

.CCSDG

Use CCSD wave function.

.NATORB

Calculate natural orbitals (currently only for MP2 density matrix)

.RELAXED

Use orbital-relaxed density matrix (currently only for MP2). The current default for MP2 and CC wave functions is to use the unrelaxed density matrix. This is computationally less expensive, but also less accurate.

*EOMCC

This menu controls the parameters for the definition of the EOM model used and the number of roots per symmetry.

Currently the implementation supports the excitation energy (EE), single electron attachment (EA) and detachment (IP) models for CCSD wavefunctions only.

Note that there is no default, if no options are selected no calculations will be performed.

.EE

Selects excitation energy calculations.

Expects two integers, the first specifying the state symmetry and the second the number of states for this symmetry. The keyword should be repeated multiple times if different symmetries are desired. The implementation does not allow for mixing the different EOM models in the same run.

Example: requesting two excitation energies for symmetry 1, four for symmetry 3, and one for symmetry 8:

.EE
1 2
.EE
3 4
.EE
8 1

Default:

No excitation energies requested

.EA

Selects single electron attachment calculations.

Expects two integers, the first specifying the state symmetry and the second the number of states for this symmetry. The keyword should be repeated multiple times if different symmetries are desired. The implementation does not allow for mixing the different EOM models in the same run.

Example: requesting two electron attachment energies for symmetry 1, four for symmetry 3, and one for symmetry 8:

.EA
1 2
.EA
3 4
.EA
8 1

Default:

No excitation energies requested

.IP

Selects electron detachment calculations.

Expects two integers, the first specifying the state symmetry and the second the number of states for this symmetry. The keyword should be repeated multiple times if different symmetries are desired. The implementation does not allow for mixing the different EOM models in the same run.

Example: requesting two single electron detachment energies for symmetry 1, four for symmetry 3, and one for symmetry 8:

.IP
1 2
.IP
3 4
.IP
8 1

Default:

No excitation energies requested

*EOMPROP

.EXCPRP

Warning

Development version only.

number of excited states to calculate expectation values for, on a given symmetry.

Arguments: two integers, the first specifying the state symmetry and the second the number of states for this symmetry

*CCDIAG

This menu controls the parameters to the iterative Davidson diagonalization procedure.

Note that the implementation currently does not support the saving of eigenvectors, so no restarts are possible.

.CONVERG

Sets the convergence threshold on the norm of the residual vectors

Default:

.CONVERG
1.0E-8

.MAXSIZE

Sets the maximum size of the subspace

Default:

.MAXSIZE
128

.MAXITER

Sets the maximum number of iterations

Default:

.MAXITR
80

.TRV_I

` Creates trial vectors based on unit vectors sorted by lowest energy of the diagonal of the similarity-transoformed Hamitonian (pivoting).

Default:

Enabled

.TRV_FULLMATRIX

Creates unit trial vectors from a unit matrix. This roughly means that the first trial vectors will be those for high-lying states.

If combined with a number of EE/EA/IP roots set to -1 and a maximum number of iterations set to 1, the full similarity transformed Hamiltonian for a given symmetry will be diagonalized. This yields the full spectrum, but for anything other than CC singles will require significant amounts of memory, so in practice such a combination is useful for debug purposes only.

Default:

Disabled

.TRV_CCS

Creates trial vectors from the eigenvectors of the singles-singles EOM-EE/IP/EA blocks.

.TRV_R2L

.TRV_NOR2L

Control the use the right-hand side (R) vectors as guess for the left-hand side (L). If disabled, (.TRV_NOR2L) trial vector generation will be controlled by the options above.

Default:

.TRV_R2L

.OVERLAP

.NOOVERLAP

Controls the use of root following via overlap in sorting the left/right-hand side eigenvalues and eigenvectors.

Default:

.NOOVERLAP

.DEBUG

Enables debug printout. Massive output.

Default:

Does not print out debug information

*CCPROJ

This menu controls the use of projection operators in the CC calculations.

These projectors are used to remove terms from the ground state CC equations (frozen core), the EOM-CC similarity transformed Hamiltonian (CVS and restricted excitation window), or a combination of both.

.FCORE

Defines which active occupied spinors to consider as part of frozen core within the ground-state CC calculation.

Input is an threshold energy value in atomic units. T amplitudes contaning spinors with energies below such value are set to zero.

Note this value does not have to be the same as for the definition of the core spinors for core-valence separation. Assuring the consistency of these choices is up to the user.

Example: requests that all spinors with energies below -10.0 a.u. are frozen:

.FCORE
-10.0

Default:

No frozen core spinors

.CVS_CORE

Defines which active occupied spinors to consider as core spinors for EOM-CC calculations employing the core-valence separation (CVS) framework. To be used with EOM-IP or EOM-EE, in order to target high-lying excited/ionized states, namely for core spectra.

Input is an threshold energy value in atomic units.

Right/Left-hand side trial vector and similarity transformed Hamiltonian matrix elements representing excited determinants containing at least one occupied spinor with energies below such value are set to zero.

Note this value does not have to be the same as for the definition of the frozen core. Assuring the consistency of these choices is up to the user.

In addition to this, users should make sure to enable root following (see .OVERLAP) if they want to target states with dominant singly ionized or singly excited character.

Example: requests that all spinors with energies below -10.0 a.u. are considered to be core:

.CVS_CORE
-10.0

Default:

No core-valence separation is enforced

.NODOCC

Requests that, when using core-valence separation, Right/Left-hand side trial vector and similarity transformed Hamiltonian matrix elements representing excited determinants containing both core occupied spinors to be projected out.

Example: requests that double core excited determinants are projected out:

.NODOCC

Default:

Double core excited determinants are retained in the calculations

.REW_OCC

.REW_VIRT

Defines a set or active occupied and/or virtual spinors as part of restricted window for EOM-CC calculations. Can be used with any EOM variant.

If an occupied/virtual restricted window is defined, the Right/Left-hand side trial vector and similarity transformed Hamiltonian matrix elements representing excited determinants containing at least one occupied/virtual spinor within the window(s) are retained in the calculation, the rest being projected out.

Input for each keyword is a pair of values defining thethreshold energy value in atomic units, one per line. Note that the two keywords can be used independently.

Right/Left-hand side trial vector and similarity transformed Hamiltonian matrix elements representing excited determinants containing at least one occupied spinor with energies below such value are set to zero.

The option .REW_OCC is incompatible with .CVS_CORE. It can however be used with .FCORE, but assuring the consistency of these choices is up to the user.

In addition to this, users should make sure to enable root following (see under *EOMCC) if they want to target states with dominant singly ionized or singly excited character.

Example: requests two restricted windows, one for occupied spinors with energies between -200.0 a.u. and -150.0 a.u. and another for virtual spinors with energies between 0.001 a.u. and 35.0 a.u.:

.REW_OCC
 -200.0
 -150.0
.REW_VIRT
 0.001
 35.0

Default:

No restricted window is defined, all occupied and/or virtual spinors are active

*CCFSPC

Perform a Fock space MRCC calculation. Fock space allows variable particle number. Sectors \((m,n)\) in Fock space corresponds to \(N+n-m\) - electron states obtained by the generation of \(m\) holes (electron removal) and \(n\) particles (electron attachment) with respect to a closed-shell reference determinant, the \((0,0)\) sector. Within each specified sector (and the lower ones), an effective Hamiltonian is built and 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, corresponding to the \((0,1)\) sector).

.DOIE

Calculate ionization energies (remove one electron from the reference state, allowing depletion of the active occupied orbitals, corresponding to the \((1,0)\) sector).

.DOEA2

Calculate second electron affinities (add two electrons to the reference state, allowing occupation of the active virtual orbitals, corresponding to the \((0,2)\) sector).

.DOIE2

Calculate second ionization energies (remove two electrons from the reference state, allowing depletion of the active occupied orbitals, corresponding to the \((2,0)\) sector).

.DOEXC

Calculate excitation energies (allow excitation from the set of active occupied orbitals to the set of active virtual orbitals, corresponding to the \((1,1)\) sector).

.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.

.GESTAT

Specify the state number in the last active sector to pick the energy from (remember to account for degeneracies) for a state-specific FSCC geometry optimization based on a numerical gradient.

*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.

low limit of orbital energies of active occupied orbitals, which constitute the secondary Pi space. Could be used in (1,0), (2,0) and (1,1) sectors. Arguments: real.

.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.

This is upper limit of one-electronic energies of active occupied orbitals, which constitute the secondary Pi space. Could be used in (1,0), (2,0) and (1,1) sectors. Arguments: real.

.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.

This is the low limit of orbital energies of active virtual orbitals, which constitute the secondary Pi space. Could be used in (0,1), (0,2) and (1,1) sectors. Arguments: real.

.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.

This is the upper limit of one-electronic energies of active virtual orbitals, which constitute the secondary Pi space. Could be used in (0,1), (0,2) and (1,1) sectors. Arguments: real.

Other Intermediate Hamiltonian (IH) input parameters

For experts only.

Following keywords belong to the CCIH namelist section.

.IHSCHEME

Choose particular IH scheme. Arguments: Integer IHSCHEME = 1, or 2.

The IHSCHEME=1 corresponds to the extrapolated IH (XIH) approach, described in the paper [Eliav2005].

Main idea: proper modification of the energetic denominators, containing problematic Pi -> Q transition. The original denominator 1/(E_Pi - E_Q) , used during CC iterations, is substituted by the following expression (1)

\[\frac{(1-[\frac{AIH*SHIFT}{(E_{Pi} - E_{Q} + SHIFT)}]^{NIH})}{\frac{(1-AIH*SHIFT}{(E_{Pi} - E_{Q} + SHIFT))}},\]

here AIH, SHIFT,NIH are parameters, specially chosen for overcoming of the intruder states problem. These parameters could be used in the procedure of the extrapolation of the “exact” effective Hamiltonian solutions from corresponding IH CC energies and wave functions.

The IHSCHEME=2 corresponds to the simplified IH-2 approach, described in the paper [Landau2004].

Here the problematic denominators \(1/(E_{Pi} - E_{Q})\) are substituted simply by the factor 0.

Default: IHSCHEME = 2

Next key options are used only in case of XIH (IHSCHEME = 1).

.SHIFTH11

Energy shift for the one-electronic excitations in (1,0) sector. Arguments: real.

.SHIFTH12

Energy shift for the two-electronic excitations in (1,0) sector. Arguments: real.

.SHIFTH2

Energy shift for the two-electronic excitations in (2,0) sector. Arguments: real.

.SHIFTP11

Energy shift for the one-electronic excitations in (0,1) sector. Arguments: real.

.SHIFTP12

Energy shift for the two-electronic excitations in (0,1) sector. Arguments: real.

.SHIFTP2

Energy shift for the two-electronic excitations in (0,2) sector. Arguments: real. Usually we choose the approximate difference between the highest orbital energy belonging to Pi and the lowest orbital energy belonging to the Pm space. Works only with the old style of RELCC input.

.SHIFTHP

Energy shift for the two-electronic excitations in (1,1) sector. Arguments: real

.AIH

Compensation factor, used in expression (1). Arguments: real positive, not greater then 1.0.

.NIH

Compensation power, used in expression (1). Arguments: integer.

In the case of the limit: AIH=1.0 and NIH -> “infinity” ( NIH>100, in practice) we have so called “full compensation” method, corresponding to the extrapolation of the effective Hamiltonian from the intermediate one.

*CCSORT

Specialist options related to the sorting of two-electron integrals and the calculation of the reference Fock matrix.

.NORECMP

Do not recompute the Fock matrix, but assume a diagonal matrix with the orbital energies taken from the SCF program on the dioagonal. This is usually not recommended as the latter correspond to a restricted open shell expression and RELCCSD uses an unrestricted formalism. For closed shell systems the two expressions are identical and this option merely suppresses a build-in check on the accuracy of transformed integrals.

.USEOE

Ignore recomputed Fock matrix and use orbital energies supplied by the SCF program. This option is sometimes useful for degenerate open shell cases in which case the perturbation theory for the unrestricted formalism is not invariant for rotations among degenerate orbitals. It should only change the outcome of the [T], (T) and -T energy corrections.

*CCRESTART

Control parameters for the restart option. The default behavior of the restart option is to verify whether in the RELCCSD the successive checkpoints have been passed, and restart the calculation at the first one which is not flagged as “Completed, restartable”.

For example, one would have

Status of the calculations
Integral sort # 1 :                   Completed, restartable
Integral sort # 2 :                   Completed, restartable
Fock matrix build :                   Completed, restartable
MP2 energy calculation :              Completed, restartable
CCSD energy calculation :             Completed, restartable
CCSD(T) energy calculation :          Completed, restartable

if a calculations has successfully has passed through all checkpoints.

For the single-reference calculations the restart is straightforward and in general no additional keywords are necessary. Users must nevertheless be careful that the restart is performed for exactly the same calculation, as there are no interla consistency checks in place in the case of a restart: this means that, for example, if either the geometry or the number of corrlated electrons or virtual spinors has been changed after the initial calculations, if the RESTART option is on the code will proceed with the old checkpoint data (sorted integrals, etc) and any results will be erroneous.

Fock-space calculations can also be restarted, but for these additional care must be taken: (1) One must redo the integral sorting steps if the model (P) or correlation (Q) spaces change dimension. A change in the values that define the partition between main (Pm) and intermediate (Pi) model spaces, on the other hand, does not require the integral sorting to be redone. (2) One has to specifically indentify which which sectors of Fock space are to be (re)calculated and which should be skipped. Some examples of such a procedure can be found in the test set.

Important: for EOMCC calculations it is currently only possible to restart from ground-state calculations. In this case, the ”.REDOCSD” keyword must be used, otherwise the code will produce incorrect results.

.UNCONVERGED

Forces results from unconverged iterative procedures to be considered as converged.

Default:

False

.FORCER

Forces restart even if setup is potentially different (number of electrons, active/inactive spinors etc).

Default:

False

.REDOCCSD

Forces the iterative procedure to solve the CCSD (or CCD or CCS) equations to be performed, even if in a prior run it has been marked as completed.

Default:

False

.REDOSECT

In the case of fock-space calculations, indicate which sectors are to be relcalculated during the restart.

This keyword expects two lines as input; on the first line, an integer specifying how many sectors are recalculated and in the second line a list of the sectors in question in the RELCC notation.

.REDOSECT
 2
 00 01

will redo sectors 0h0p and 0h1p

Default:

All sectors are recalculated

.SKIPSECT

In the case of fock-space calculations, indicate which sectors are to be skipped during the restart

This keyword expects two lines as input; on the first line, an integer specifying how many sectors are recalculated and in the second line a list of the sectors in question in the RELCC notation.

.SKIPSECT
 2
 00 01

will bypass the calculation of sectors 0h0p and 0h1p.

Default:

No sectors are skipped

.REDOSORT

Forces the sorting into the six integral classes to be performed again, even if prior sorting was completed.

Default:

False. integrals are not resorted if the prior sorting was completed.