In this section the keywords of the Mrcc input file are listed in alphabetical order.
The active orbitals for multi-reference (active-space) CI/CC calculations can be specified using this keyword. Note that this keyword overwrites the effect of keywords nacto and nactv.
All orbitals are inactive (i.e., single-reference calculation).
Using this option one can select the active orbitals specifying their serial numbers. The latter should be given in the subsequent line as $<n_{1}>$,$<n_{2}>$,…,$<n_{k}>$-$<n_{l}>$,…, where $n_{i}$’s are the serial numbers of the correlated orbitals. Serial numbers separated by dash mean that $<n_{k}>$ through $<n_{l}>$ are active. Note that the numbering of the orbitals is relative to the first correlated orbital, that is, frozen orbitals are excluded.
Using this option one can set the active/inactive feature for each correlated orbital. In the subsequent line an integer vector should be supplied with as many elements as the number of correlated orbitals. The integers must be separated by spaces. Type 1 for active orbitals and 0 for inactive ones.
active=none
We have 20 correlated orbitals. Orbitals 1, 4, 5, 6, 9,
10, 11, 12, and 14 are active. Using the serialno option the input
should include the following two lines:
active=serialno
1,4-6,9-12,14
The same using the vector option:
active=vector
1 0 0 1 1 1 0 0 1 1 1 1 0 1 0 0 0 0 0 0
Specifies the angular integration grid for DFT calculations. The grid construction follows the design principles of Becke [7], the smoothing function for the Voronoi polyhedra are adopted from Ref. 103 with $m_{\mu}$ = 10. Angular grids are taken from the Grid file which is located in the BASIS directory created at the installation. By default, the 6-, 14-, 26-, 38-, 50-, 74-, 86-, 110-, 146-, 170-, 194-, 230-, 266-, 302-, 350-, 434-, 590-, 770-, 974-, 1202-, 1454-, and 1730-point Lebedev quadratures [7] are included in the file, which are labeled, respectively, by LD0006, LD0014, etc. In addition to the above grids, any angular integration grid can be used by adding it to the BASIS/Grid file or alternatively to the GENBAS file to be placed in the directory where Mrcc is executed. The format is as follows. On the first line give the label of the grid as XXNNNN, where XX is any character and NNNN is the number of the grid points (see the above examples). The subsequent NNNN lines must contain the Cartesian coordinates and the weights for the grid points.
For the selection of the angular grids, by default, an adaptive scheme motivated by Ref. 72 is used. The angular grids are selected for each radial point so that the error in the angular integrals will not be larger than $10^{-{\tt grtol}}$. The important difference is that the grids are optimized for each atom separately to avoid discontinuous potential energy surfaces. For the construction of the radial integration grid see the description of keyword rgrid. See also the description of keyword grtol.
the name of the quadrature as it is specified in the BASIS/Grid (or GENBAS) file. This angular quadrature will be used in each radial point.
An adaptive integration grid will be used. For each radial point, depending on its distance from the nucleus, a different Lebedev grid will be selected. The minimal and maximal number of points is MMMM and NNNN, respectively.
agrid=LD0006-LD0590
for a 974-point Lebedev grid set agrid=LD0974
to use an adaptive grid with at least 110 and at most 974 angular points set agrid=LD0110-LD0974
for a very fine grid use
agrid=LD0110-LD0974
grtol=12
Specifies the basis set used in all calculations. By default the basis sets are taken from the files named by the chemical symbol of the elements, which can be found in the BASIS directory created at the installation. The basis sets are stored in the format used by the Cfour package (see Sect. 6.9). In addition to the basis sets provided by default, any basis set can be used by adding it to the corresponding files in the BASIS directory. Alternatively, you can also specify your own basis sets in the file GENBAS which must be copied to the directory where Mrcc is executed.
If the same basis set is used for all atoms, the label of the basis set must be given.
If different basis set are used, but the basis sets are identical for atoms of the same type, basis=atomtype should be given, and the user must specify the basis sets for each atomtype in the subsequent lines as $<$atomic symbol$>$:$<$basis set$>$ .
Mixed basis sets will be used, that is, different basis sets will be
used for different groups of atoms specified by their serial number.
The number of groups, the basis sets, and corresponding atoms must be
specified in the subsequent lines as
$<$number of groups$>$
$<$basis set label 1$>$
$<n_{1}>$,$<n_{2}>$,…,$<n_{k}>$-$<n_{l}>$,…
$<$basis set label 2$>$
$<m_{1}>$,$<m_{2}>$,…,$<m_{k}>$-$<m_{l}>$,…
…
where $n_{i}$’s, $m_{i}$’s, …are the serial numbers of the atoms.
Serial numbers
separated by dash mean that atoms $<n_{k}>$ through $<n_{l}>$ are included.
A mixed basis set composed of two AO bases will be used in the case of an embedding calculation. It only works if keyword embed is also specified. The two basis sets must be given in the following two lines. The first basis will be used for the environment, while the second one is the AO basis for the embedded subsystem (see also the description of keyword embed).
It is the same as embed, but the partitioning defined by keyword corembed will be used.
In the general case, if different basis set are used for each atom, then one should give basis=special and specify the basis sets for each atom in the subsequent lines by giving the label of the corresponding basis sets in the order the atoms appear at the specification of the geometry.
By default the following basis sets are available for elements H to Kr in Mrcc:
the def2 Gaussian basis sets of Weigend and Ahlrichs [156]: def2-SV(P), def2-SVP, def2-TZVP, def2-TZVPP, def2-QZVP, def2-QZVPP
the augmented def2 Gaussian basis sets of Rappoport and Furche [132]: def2-SVPD, def2-TZVPD, def2-TZVPPD, def2-QZVPD, def2-QZVPPD
F12 basis sets for explicitly correlated wave functions developed by Peterson et al. [123]: cc-pV$X$Z-F12 ($X$ = D, T, Q)
the Gaussian basis sets of Dunning and Hay (LANL2DZ) [28]
the auxiliary basis sets of Hellweg and Rappoport for the augmented def2 Gaussian basis sets [56]: def2-SVPD-RI, def2-TZVPD-RI, def2-TZVPPD-RI, def2-QZVPD-RI, def2-QZVPPD-RI
Weigend’s Coulomb/exchange auxiliary basis sets for density fitting/resolution of the identity SCF calculations [159]: cc-pV$X$Z-RI-JK, aug-cc-pV$X$Z-RI-JK ($X$ = D, T, Q, 5), def2-QZVPP-RI-JK
From Na to La and from Hf to Rn the following basis sets are available, which must be used together with the corresponding ECP (see also the description of keyword ECP):
the def2 Gaussian basis sets of Weigend and Ahlrichs [156]: def2-SV(P), def2-SVP, def2-TZVP, def2-TZVPP, def2-QZVP, def2-QZVPP
the augmented def2 Gaussian basis sets of Rappoport and Furche [132]: def2-SVPD, def2-TZVPD, def2-TZVPPD, def2-QZVPD, def2-QZVPPD
the auxiliary basis sets of Hellweg and Rappoport for the augmented def2 Gaussian basis sets [56]: def2-SVPD-RI, def2-TZVPD-RI, def2-TZVPPD-RI, def2-QZVPD-RI, def2-QZVPPD-RI
the auxiliary basis sets of Hättig for correlation calculations with the PP basis sets: cc-pV$X$Z-PP-RI and aug-cc-pV$X$Z-PP-RI ($X$ = D, T, Q, 5)
Please note that some of the above basis sets are not available for all elements.
If you use your own basis sets, these must be copied to the end of the corresponding file in the BASIS directory. Alternatively, you can also create a file called GENBAS in the directory where Mrcc is executed, and then you should copy your basis sets to that file.
The labels of the basis sets must be identical to those used in the BASIS/* files (or the GENBAS file). For the default basis sets just type the usual name of the basis set as given above, e.g., cc-pVDZ, 6-311++G**, etc. If you employ non-default basis sets, you can use any label.
For Dunnings’s aug-cc-p(C)V$X$Z basis sets one, two, or three additional diffuse function sets can be automatically added by attaching the prefix d-, t-, or q-, respectively, to the name of the basis set. To generate a d-aug basis set one even tempered diffuse function is added to each primitive set. Its exponent is calculated by multiplying the exponent of the most diffuse function by the ratio of the exponents of the most diffuse and the second most diffuse functions in the primitive set. If there is only one function in the set, the exponent of the most diffuse function is divided by 2.5. To generate t-aug and q-aug sets this procedure is repeated.
For Dunnings’s basis sets, to use the aug-cc-p(C)V$X$Z set for the non-hydrogen atoms and the corresponding cc-p(C)V$X$Z set for the hydrogens give aug'-cc-p(C)V$X$Z. Then the diffuse functions will be automatically removed from the hydrogen atoms.
Only the conventional AO basis set can be specified with this keyword. For the fitting basis sets used in density fitting approximations see the description of keywords dfbasis_*.
The cc-pVDZ-RI-JK basis set has been generated from cc-pVTZ-RI-JK by dropping the functions of highest angular momentum. The aug-cc-pV$X$Z-RI-JK (def2-QZVPPD-RI-JK) basis sets are constructed automatically from the corresponding cc-pV$X$Z-RI-JK (def2-QZVPP-RI-JK) sets by adding diffuse functions as described above for the d-aug-cc-p(C)V$X$Z basis sets.
For Dunnings’s and Pople’s basis sets add the -min postfix to the basis set name to generate a minimal basis set dropping all the polarization (correlation) functions.
If the (aug-)cc-pV$X$Z-PP basis set does not exist for an element with $Z\leq 28$, the program will automatically attempt to use the corresponding aug-cc-pV$X$Z basis instead.
none, that is, the basis set must be specified (excepting the case when Mrcc is used together with another code, that is, iface $\neq$ none).
Consider any molecule and suppose that the cc-pVDZ basis
set is used for all atoms. The input must include the following line:
basis=cc-pVDZ
To use Dunning’s doubly augmented cc-pVDZ basis set
(d-aug-cc-pVDZ) for all atoms the input must include the following
line:
basis=d-aug-cc-pVDZ
Consider the water molecule and use the cc-pVDZ basis set
for the hydrogens and cc-pVTZ for the oxygen. The input must include
the following lines:
basis=atomtype
O:cc-pVTZ
H:cc-pVDZ
Consider water again and use the cc-pVQZ, cc-pVTZ, and
cc-pVDZ basis sets for the oxygen atom, for the first hydrogen, and for
the second hydrogen, respectively. Note that the order of the basis set
labels after the basis=special statement must be identical to the
order of the corresponding atoms in the Z-matrix/Cartesian coordinates:
geom
O
H 1 R
H 1 R 2 A
R=0.9575
A=104.51
basis=special
cc-pVQZ
cc-pVTZ
cc-pVDZ
Consider the water molecule and use the cc-pVTZ basis set
for the hydrogens and aug-cc-pVTZ for the oxygen. The following two
inputs are identical:
basis=atomtype
O:aug-cc-pVTZ
H:cc-pVTZ
or
basis=aug'-cc-pVTZ
Consider the water molecule. If you specify
basis=cc-pVTZ-min
minimal basis sets generated from cc-pVTZ will be used for the atoms,
that is, only one $s$
function (two $s$ and one $p$ shells) will be retained from the $s$–$p$
kernel of the H (O) cc-pVTZ basis set.
Consider the PbO molecule. If you want to use the
cc-pVDZ basis set for O and the cc-pVDZ-PP basis with the corresponding
ECP for Pb, you only need to set
basis=cc-pVDZ-PP
in the MINP file.
Mixed basis approach with two basis sets, the cc-pVTZ
basis is used for atoms 1, 2, 3, and 5, while cc-pVDZ is employed for
atoms 4, 6, 7, 8:
basis=mixed
2
cc-pVTZ 1-3,5
cc-pVDZ 4,6-8
Specifies the small basis set used in dual basis-set calculations as well as for generating SCF initial guess (scfiguess=small).
the options are the same as for keyword basis, but there is an additional one, none, which means that no small basis is defined.
basis_sm=none
To restart an SCF calculation with the cc-pVQZ basis set
from the densities obtained with the cc-pVDZ basis give
basis=cc-pVQZ
basis_sm=cc-pVDZ
scfiguess=small
To perform a dual basis set DF-HF calculation with the 6-311G** and
6-31G** basis sets you need:
basis=6-311G**
basis_sm=6-31G**
dual=on
calc=DF-HF
Use this keyword to turn on/off basis set optimization. Besides setting this keyword a user supplied GENBAS file is also required for basis set optimization jobs. It is also possible to set the value of basopt to be equal to an appropriate energy. In this case the basis set parameters are optimized so that the absolute value of the difference between this value and the actual energy is minimized. This option comes handy when optimizing a density fitting basis set. In this case the difference between the actual and non-density-fitting energy (obtained from a previous calculation) will be minimized. See also Sect. 6.9.
on, off, or $<$any real number$>$
basopt=off
To optimize a basis set variationally set basopt=on
To optimize a basis set minimizing the difference of the calculated energy and -76.287041 E${}_{h}$ set basopt=-76.287041
Specifies the bond function (BF) basis (see Ref. 95 for details).
No BFs are used.
name of the BF basis to be used.
The format of the name of the BF basis, $<$BF basis name$>$, is $<$AO basis name$>$-$<$BF type$>$. E.g., 6-31G-1s1p is a BF basis optimized for the 6-31G AO basis and one s and one p function set are placed on the corresponding bonds.
The BF basis sets are stored in the BASIS/Bond file but the BF basis can also be specified in the GENBAS file similar to the AO basis sets (see the description of keyword basis). The format of the label of the BF basis in the file is B$<$bond name$>$:$<$BF basis name$>$. E.g., BCH:6-31G-1s1p is 6-31G-1s1p BF basis optimized for the C–H bond.
If BF bases are used, the geometry must be given in mol format (see the description of keyword geom)
bfbasis=none
hydrogen-fluoride molecule, the 6-31G basis and the 6-31G-1s1p bond
function basis are used:
basis=6-31G
bfbasis=6-31G-1s1p
geom=mol
2 1
0.00000000 0.00000000 0.00000000 F
0.00000000 0.00000000 0.91690000 H
1 2 1
Boughton–Pulay completeness criterion [16] for occupied orbitals. In various local correlation approaches the Boughton–Pulay procedure is used to identify the atoms on which an LMO is localized. The least-squares residual of the parent LMO and the LMO truncated to the selected atoms is required to be less than one minus this criterion.
This number will be used as the completeness criterion.
bpcompo=0.985
Atom domains determined by bpcompo are also utilized to construct local fitting domains in the case of localcc=2016 or 2018 according to Ref. 105.
to set a threshold of 0.99 type bpcompo=0.99
Boughton–Pulay completeness criterion [16] for virtual orbitals (projected atomic orbitals). See also keyword bpcompo.
This number will be used as the completeness criterion.
bpcompv=0.98
to set a threshold of 0.95 type bpcompv=0.95
Boughton–Pulay completeness criterion [16] for the occupied orbitals of an extended domain. See also keyword bpcompo.
This number will be used as the completeness criterion.
bpedo=bpcompo is set if bpedo is not specified and not employed in the local correlation calculation
to set a threshold of 0.9998 type bpedo=0.9998
Boughton–Pulay completeness criterion [16] for the virtual orbitals (projected atomic orbitals) of an extended domain. See also keyword bpcompo.
This number will be used as the completeness criterion.
bpedv=0.995 is set as default in the case of localcc=2016 or 2018 according to Ref. 105.
bpedv=bpcompv is set if bpedv is not specified and not employed in the local correlation calculation
to set a threshold of 0.99 type bpedv=0.99
Boughton–Pulay completeness criterion [16] for the occupied orbital of a primary domain. See also keyword bpcompo.
This number will be used as the completeness criterion.
bppdo=0.999 is set as default in the case of localcc=2016 or 2018 according to Ref. 105.
bppdo=bpcompo is set if bppdo is not specified and not employed in the local correlation calculation
to set a threshold of 0.99 type bppdo=0.99
Boughton–Pulay completeness criterion [16] for virtual orbitals (projected atomic orbitals) of a primary domain. See also keywords bppdo and bpcompo.
This number will be used as the completeness criterion.
bppdv=bpcompv
to set a threshold of 0.99 type bppdv=0.99
Specifies the type of the calculation.
Hartree–Fock SCF calculation, the type of the Hartree–Fock wave function can be controlled by keyword scftype (see also keyword scftype).
Restricted, unrestricted, or restricted open-shell Hartree–Fock SCF calculation, respectively. The type of the Hartree–Fock wave function is also defined at the same time if these options are chosen, and it is not necessary to set scftype. That is, calc=RHF is equivalent to calc=SCF plus scftype=RHF, etc.
Kohn–Sham SCF calculation with the specified density functional. The type of the Kohn–Sham procedure (i.e., RKS of UKS) can be controlled by keyword scftype (see also keyword scftype). The options are identical to those of keyword dft (except for off, user, and userd), see the description of keyword dft. Note that for a correlated calculation with KS orbitals you can only select the functional with keyword dft, the value of keyword calc must be set to the desired correlation method. Note also that for DFT calculations the density fitting approximation is used by default, i.e., dfbasis_scf is set to auto. To run a conventional KS calculation set dfbasis_scf=none.
Time-dependent HF (TD-HF, also known as random-phase approximation). If calc=SCF and number of the states is greater than one (set by keywords nsing, ntrip, or nstate), also TD-HF calculations are performed for the excited states. It is only available with density fitting.
Full time-dependent DFT (TD-DFT). The density functional must be set using keyword dft. Alternatively, if calc is set to the name of the functional, and the number of the states is greater than one (set by keywords nsing, ntrip, or nstate), also TD-DFT calculations are performed for the excited states using the given functional. For HF reference it is equivalent to TD-HF. It is only available with density fitting.
TD-DFT in the Tamm–Dancoff approximation (TDA). For HF reference it is equivalent to CIS. It is only available with density fitting.
Second-order Møller–Plesset (MP2) calculation, the spin-component scaled MP2 (SCS-MP2) [46] and the scaled opposite-spin MP2 (SOS-MP2) [63] energy will also be computed (see also keywords scsps and scspt). Note that efficient MP2 calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-MP2 ($\equiv$ RI-MP2) calculation is performed (that is, options MP2, DF-MP2, and RI-MP2 are synonyms). If you are still interested in the MP2 energy without DF, you can, e.g., run a CCSD calculation (without DF), where the MP2 energy is also calculated.
Scaled opposite-spin second-order Møller–Plesset (SOS-MP2) calculation [63] using an $N^{4}$-scaling algorithm based on the Cholesky decomposition/Laplace transform of energy denominators (in practice one dRPA iteration is performed, see below). Note that it is only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-SOS-MP2 ($\equiv$ RI-SOS-MP2) calculation is performed (that is, options SOS-MP2, DF-SOS-MP2, and RI-SOS-MP2 are synonyms).
For canonical calculations it is equivalent to option MP2. If a local correlation calculation is executed, only the spin-component scaled MP2 (SCS-MP2) energy will be computed.
Direct random-phase approximation (dRPA) calculation (see Eqs. 7 and 8 in Ref. 152). Note that dRPA calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-dRPA ($\equiv$ RI-dRPA) calculation is performed (that is, options dRPA, DF-dRPA, and RI-dRPA are synonyms).
Random-phase approximation (RPA) calculation (see Eqs. 10 and 13 in Ref. 152, where it is referred to as RPAx-SO2). Note that RPA calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-RPA ($\equiv$ RI-RPA) calculation is performed (that is, options RPA, DF-RPA, and RI-RPA are synonyms).
Second-order screened exchange (SOSEX) [48] calculation (see Eqs. 7 and 9 in Ref. 152), the dRPA energy is also computed. Note that SOSEX calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-SOSEX ($\equiv$ RI-SOSEX) calculation is performed (that is, options SOSEX, DF-SOSEX, and RI-SOSEX are synonyms).
RPAX2 calculation (see Eqs. 17 to 19 in Ref. 58). Note that RPAX2 calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-RPAX2 ($\equiv$ RI-RPAX2) calculation is performed (that is, options RPAX2, DF-RPAX2, and RI-RPAX2 are synonyms).
Configuration interaction singles (CIS) calculation [96]. Efficient CIS calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-CIS ($\equiv$ RI-CIS) calculation is performed (that is, options CIS, DF-CIS, and RI-CIS are synonyms). If you are still interested in the CIS energy without DF, set ccprog=mrcc, dfbasis_scf=none, and dfbasis_cor=none.
Iterative doubles correction to configuration interaction singles [CIS(D${}_{\infty}$)] calculation [53, 96]. Note that CIS(D${}_{\infty}$) calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-CIS(D${}_{\infty}$) [$\equiv$ RI-CIS(D${}_{\infty}$)] calculation is performed [that is, options CIS(Di), DF-CIS(Di), and RI-CIS(Di) are synonyms].
Second-order algebraic diagrammatic construction [ADC(2)] calculation [141, 96]. Note that ADC(2) calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-ADC(2) [$\equiv$ RI-ADC(2)] calculation is performed [that is, options ADC(2), DF-ADC(2), and RI-ADC(2) are synonyms].
Second-order coupled-cluster singles and doubles (CC2) calculation [18, 96]. Efficient CC2 calculations are only possible with the density-fitting (resolution-of-identity) approximation, and, by default, a DF-CC2 ($\equiv$ RI-CC2) calculation is performed (that is, options CC2, DF-CC2, and RI-CC2 are synonyms). If you are still interested in the CC2 energy without DF, set ccprog=mrcc, dfbasis_scf=none, and dfbasis_cor=none.
The corresponding single-reference CC calculation with perturbative corrections (see Ref. 77).
The corresponding single-reference CC calculation with perturbative corrections (see Ref. 77).
The corresponding CCSD(T)${}_{\Lambda}$, CCSDT(Q)${}_{\Lambda}$, etc. calculation (see Ref. 77).
The corresponding iterative approximate single-reference CC calculation (see Ref. 77).
The corresponding iterative approximate single-reference CC calculation (see Ref. 77).
The corresponding iterative approximate single-reference CC calculation (see Ref. 77).
The corresponding iterative approximate single-reference CC calculation (see Ref. 77).
The corresponding single-reference CC calculation with perturbative corrections using ansatz A (see Ref. 79).
The corresponding single-reference CC calculation with perturbative corrections using ansatz B (see Ref. 79).
The corresponding single-reference CC calculation with perturbative corrections using ansatz A (see Ref. 79).
The corresponding single-reference CC calculation with perturbative corrections using ansatz B (see Ref. 79).
In the above options $n$ is a positive integer, which is the excitation level of the highest excitation. $n$ is supposed to be equal to or greater than 6 since for smaller $n$’s the CC($<$n$>$) and similar options are equivalent to one of the other options, e.g., CC(5) is equivalent to CCSDTQP or CC(3)(4) is identical with CCSDT(Q).
For excited-state calculations with the TD-HF, TDA, TD-DFT, CIS, CIS(D${}_{\infty}$), ADC(2), CC2 and various CC and CI methods the number of states should be greater than one (keywords nsing, ntrip, or nstate). If more than one state is requested for CC calculations, the corresponding linear-response (LR) CC (for excitation energies it is equivalent to equation-of-motion CC, EOM-CC) calculation is performed automatically for the excited states. If more than one state is requested and calc=SCF, TD-HF (dft=off) or TD-DFT (dft$\neq$off) calculations will be carried out for the excited states.
The active orbitals can be selected and the MRCI/CC calculations can be controlled by keywords nacto, nactv, active, maxex, and maxact.
In principle, all methods can be used with the density fitting (resolution-of-identity) approximation. It is possible in two ways. You can attach the prefix DF- or RI- to the corresponding option from the above list. Then, for a HF calculation keyword dfbasis_scf will be set to auto, while for a correlated calculation both dfbasis_scf and dfbasis_cor will be given the value auto. Alternatively, you can also set the values for keywords dfbasis_scf and dfbasis_cor, see their description.
Local correlation methods can be run if the prefix “L” is added to the corresponding option of the keyword, e.g., as LMP2, LdRPA, LCCSD(T), etc. Additionally, the prefix “LNO-” can also be used as a synonym in the case of local coupled-cluster approaches, e.g., as LNO-CCSD, LNO-CCSD(T), LNO-CCSDT, etc. Both options are equivalent to setting localcc=on.
For the dRPA, RPA, and SOSEX methods the use of PBE orbitals is recommended.
For the RPAX2 method the use of PBEx orbitals is recommended.
calc=SCF
To run a CCSD(T) calculation the user should set calc=CCSD(T)
For DF-HF (RI-HF) calculations type:
calc=DF-HF
which is equivalent to the following input:
calc=SCF
dfbasis_scf=auto
For a local CCSD(T) calculation using the local natural orbital approximation set calc=LCCSD(T) or calc=LNO-CCSD(T)
For a RI-MP2 calculation set calc=MP2
For a DFT calculation with the B3LYP functional set calc=B3LYP
Direct RPA calculation with Kohn–Sham orbitals calculated with the
PBE functional:
calc=dRPA
dft=PBE
TD-DFT calculation for the 3 lowest singlet excited states of a molecule
using the PBE functional:
calc=TDDFT
dft=PBE
nsing=4
A somewhat less complicated input for the same purpose:
calc=PBE
nsing=4
Maximum number of iteration steps in correlated calculations (CC, CI, RPA, …).
$<$any positive integer$>$
ccmaxit=50
to increase the maximum number of CC iterations to 100 give ccmaxit=100
Specifies the CC program to be used.
The automated, string-based CC program mrcc will be called.
The very fast, hand-coded CCSD(T) codes, ccsd or uccsd, will be executed (currently the spatial symmetry cannot be utilized).
The very fast, hand-coded, integral direct DF-CIS code cis will be executed (currently the spatial symmetry cannot be utilized).
Please note that the mrcc code was optimized for high-order CC calculations, such as CCSDT(Q) and CCSDTQ, which require different algorithms than CCSD(T). Thus it is slow for CCSD(T), but optimal for high-order CC models.
ccprog=ccsd for CCSD and CCSD(T) calculations, ccprog=cis for CIS, CIS(D${}_{\infty}$), ADC(2), and CC2 calculations, ccprog=mrcc otherwise.
to use the mrcc code for CCSD or CCSD(T) calculations give ccprog=mrcc
Convergence threshold for the energy in correlated calculations (CC, CI, dRPA, RPA, etc.). The energy will be accurate to $10^{-{\tt cctol}}$ E${}_{h}$.
$<$any integer$>$
cctol=8 for property calculations,
cctol=[-$\log_{10}$(optetol)]+2 for geometry optimizations,
cctol=5 for localcc=2016 and
localcc=2018,
cctol=6 otherwise
for an accuracy of $10^{-8}$ E${}_{h}$ one must give cctol=8
Charge of the system.
$<$any integer$>$
charge=0
for the Cl${}^{-}$ ion one should give charge=-1
Specifies what type of algorithm is to be used in CIS, TDA, TD-HF, and TD-DFT calculations.
Conventional algorithm, two-electron integrals are stored on disk
Completely I/O-free, integral-direct algorithm, two-electron integrals are recalculated in each iteration step.
Partially I/O-free, integral-direct algorithm; recommended if the I/O is fast and/or few states are required.
Variant of direct2, but usually slower.
Based on the size of the molecule the program will automatically select the most efficient one from the above options.
cialg=auto
to use disk-based algorithm set cialg=disk
The initial guess vectors for CI and LR-CC calculations can be specified using this keyword.
The initial trial vectors are supplied by the user and
should be given in the subsequent lines as follows. For each state
the corresponding initial guess vector must given by the number of
non-zero elements of the vector on the first line, followed by as many
lines as the number of non-zero elements. In each line the
corresponding excitation operator and the value for this element of the
vector must be provided in the following format:
$<n><sp_{1}><sp_{2}>\dots<sp_{n}><a_{1}><a_{2}>\dots<a_{n}><i_{1}><i_{2}>\dots<%
i_{n}><coeff>$
where $<n>$ is the level of excitation, and the electrons are
promoted from occupied orbitals $<i_{1}><i_{2}>\dots<i_{n}>$ to virtual
orbitals $<a_{1}><a_{2}>\dots<a_{n}>$ with spins
$<sp_{1}><sp_{2}>\dots<sp_{n}>$ ($<sp_{k}>$ is 1 for alpha and 0
for beta), respectively. $<coeff>$ is the corresponding coefficient.
Initial trial vectors are not specified, the program applies simple unit vectors as initial guess. The unit vectors are determined on the basis of the diagonal elements of the Hamiltonian: if $n$ roots are requested, $n$ unit vectors corresponding to the $n$ lowest diagonals will be used.
ciguess=off
Suppose that we have two excited states in a LR-CC
calculation. Then the initial guess can be given as follows.
ciguess=on
1
1 1 6 4 1.0
3
1 1 7 3 0.1
2 1 0 7 7 5 5 1.0
2 1 1 7 6 3 4 0.1
For the first state there is only one entry, a single
excitation of the alpha electron from orbital 4 to orbital 6
with a coefficient of 1.0. For the second root the initial guess
vector contains three entries. A single excitation from orbital
3 to orbital 7 with alpha spin and a relative weight of 0.1, a
double excitation from orbital 5 to orbital 7 with a weight of
1.0, and another double excitation of the alpha electrons from
orbitals 3 and 4 to orbitals 6 and 7 with a weight of 0.1.
For $M_{S}=0$ states the vector is automatically spin-adapted, and you do not need to specify the coefficients for the corresponding spin-reversed excitations. E.g., in the above example, for root 1 the 1 0 6 4 1.0 entry is unnecessary.
The guess vector is not required to be normalized, it is done automatically.
In the case of four-component relativistic calculations (Dirac interface) the serial numbers of the spinors should be specified. In addition, the second number in the above strings must be 1 (that is, all excitations are formally considered as excitations of alpha electrons).
Specifies the computational point group. All calculations will use the specified Abelian group. See Sect. 13 for more details.
The molecular symmetry is automatically recognized.
Schönflies symbol of the Abelian point group such as C1, Ci, Cs, C2, C2v, C2h, D2, D2h
cmpgrp=C1 is equivalent to symm=off
cmpgrp=auto
to use $C_{2v}$ point group for benzene set cmpgrp=C2v
Specifies whether the core electrons are correlated.
Frozen core approximation
All core electrons are correlated
The lowest (according to orbital energy order) $n$ pieces of spatial orbitals (the lowest $n$ pieces of alpha and $n$ pieces of beta spin orbitals for UHF/semicanonical ROHF reference) will be dropped.
core=frozen
to correlate all core electrons set core=corr or core=0
This keyword controls the models and subsystems selected for multi-level local correlation methods. Currently it is only available for closed-shell systems using density-fitting.
Conventional case, a single model defined by calc is used for the entire system.
Multi-level calculation is performed with different local correlation methods for the active (high-level) and the environmental (low-level) subsystems. The three input lines following corembed define the list of active atoms, the computational model for the environment level, and the number of embedded orbitals (if it is specified). The syntax for these three lines is analogous with that for keyword embed. (See the description of keyword embed.) The high-level method for the active region should be specified by the keyword calc.
corembed=off
Local correlation methods available with localcc=2015,
localcc=2016, and localcc=2018 (e.g., MP2
or arbitrary single-reference CC) can be chosen for both the active and
the environmental subsystem. Additionally, HF or HF+LRC are also
available choices for the low-level model. If the latter is set, the
environment is treated at the HF level but the long-range correlation
(LRC) between the active subsystem and its environment is also taken into
account (see Ref. 62). Note that models with KS-DFT
reference, such as dRPA, SOSEX, etc., are not available for multi-level
local correlation calculations.
The threshold settings of the local correlation method chosen for the high-level model can be given (as in the case of corembed=off) by the keywords controlling the local correlation methods (see their list in Sect. 6.8). Default settings according to lcorthr=normal and localcc=2018 (or for previous versions according to lcorthr=loose and localcc=2015 or localcc=2016) are employed for the low-level model of the environment.
LNO-CCSD(T)-in-LMP2 scheme, where LNO-CCSD(T) is performed for
the active orbitals with tight thresholds,
atoms 1 and 2 are included in the high-level region, and the number
of the active orbitals is determined automatically:
calc=LNO-CCSD(T)
lcorthr=tight
corembed=on
1-2
LMP2
0
LNO-CCSDT-in-LNO-CCSD scheme, where the local CCSDT
calculation is performed
with the mrcc program for the active orbitals and the local
CCSD is calculation performed
with the ccsd program for the environment:
calc=LCCSDT
corembed=on
1-2
LCCSD
0
LNO-CCSD(T)-in-HF+LRC embedding where only HF is used for the
environment but the additional LRC term accounts for the interaction of
the active and environmental parts. Atoms 1, 2, 3, and 5 define the
active subsystem, and 10 orbitals are included in the active region:
calc=LNO-CCSD(T)
corembed=on
1-3,5
HF+LRC
10
Diagonal Born–Oppenheimer correction (DBOC) (available only with Cfour).
on or off
dboc=off
for a DBOC calculation set dboc=on
Selects the algorithm for the decomposition of energy denominators, Cholesky-decomposition or Laplace transform, for canonical SOS-MP2 and dRPA (also required for SOSEX) as well as for local MP2 and dRPA calculations. The dRPA calculation is performed using the modified algorithm of Heßelmann [58] based on the decomposition of energy denominators. For the calculation of the SOS-MP2 energy, in practice one dRPA iteration is performed with the aforementioned algorithm. In the case of local MP2 and dRPA calculations the correlation energy contributions are also evaluated with the aid of the decomposition of energy denominators (see Ref. 85). The algorithm for the decomposition can be set using this keyword in all of the above cases. The number of retained Cholesky vectors/quadrature points can be controlled by keyword nchol.
Cholesky decomposition will be used
Laplace transform will be used
dendec=Laplace for SOS-MP2, dendec=Cholesky otherwise
The algorithms based on the Laplace-transformed technique use minimax quadratures obtained from Ref. 150.
The default quadratures are taken from the Quad file which is located in the BASIS directory created at the installation. In addition to the default quadratures, any further quadrature can be used by adding it to the BASIS/Quad file or alternatively to the GENBAS file to be placed in the directory where Mrcc is executed. The format is as follows. On the first line give the label of the quadrature as KNNRXXX, where NN is the number of the quadrature points and XXX is the upper limit of the interval in which the Laplace transform is approximated (variable $R$ in Ref. 150). The subsequent NN lines must contain, respectively, the weights and quadrature points.
to use Laplace transform give dendec=Laplace
Construction of density, derivative density, and transition density matrices for property calculations. If mod(dens,2)=1, only one-particle, if mod(dens,2)=0, both one- and two-particle density matrices will be calculated and contracted with the available property integrals. See Refs. 74, 75, 76, 78, 112, 113 for more details.
Density-matrix calculation (for geometry optimizations, first-order properties, etc.)
Density-matrix first derivatives (for second-order property calculations, available only with Cfour)
Transition density matrices (for transition moment calculations)
Second and third derivatives of the density-matrix (for third-order property calculations, available only with Cfour)
dens=2 for geometry optimizations and QM/MM calculations, dens=0 otherwise
Transition moment as well as excited-state gradient calculations can be performed for only one excited state at a time, that is, nsing, ntrip, or nstate cannot exceed 2. To compute the transition moment or gradient for a higher excited state you need to converge the equations to that root. The best practice is to run a calculation with the desired number of excited states, and then restart the calculation selecting a higher solution (see the description of keyword rest). You can also try to start the calculation from a good initial guess (see the description of keyword ciguess).
If dens $\neq$ 0, a population analysis is also performed, and Mulliken and Löwdin atomic charges as well as Mayer bond orders are computed.
for the calculation of both one- and two-particle density matrices set dens=2
Specifies how the inverse of the two-center Coulomb integral matrix is decomposed in density fitting direct SCF calculations.
The fitting coefficients are computed by solving the corresponding system of linear equations. It is efficient and numerically stable. It is the best choice for very large auxiliary basis sets for which the diagonalization of the two-center integral matrix is prohibitive.
Inverse square root of the two-center integral matrix is used. It is relatively stable numerically, but the diagonalization is slow and requires much memory.
Cholesky decomposition of the inverse of the two-center integral matrix is used. It is an efficient algorithm but numerically unstable if the two-center matrix tends to be singular.
dfalg=InvSqrt for property calculations, dfalg=LinEq otherwise
to use Cholesky decomposition set dfalg=Cholesky
Specifies whether the density fitting approximation will be used in the correlated calculations and also specifies the fitting basis set.
The density fitting approximation is not used for the correlated calculation.
The density fitting approximation is invoked, and the specified basis set is used as fitting basis set. For the specification of the basis the same rules apply as for keyword basis, see the description of keyword basis.
This option can only be used if Dunning’s (aug-)cc-pV$X$Z, Weigend and Ahlrichs’ def2, the augmented def2 basis sets of Rappoport and Furche, Peterson’s cc-pV$X$Z-F12 or (aug-)cc-pV$X$Z-PP, or Pople’s basis sets are used as the normal basis set. In this case, if dfbasis_cor=auto, the density fitting approximation is invoked. For the (aug-)cc-pV$X$Z(-PP) basis sets the corresponding (aug-)cc-pV$X$Z(-PP)-RI basis sets will be used automatically as the fitting basis sets, while for a cc-pV$X$Z-F12 basis set the corresponding aug-cc-pV$X$Z-RI basis will be taken. For the (augmented) def2 basis sets also the corresponding RI basis sets will be used, e.g., def2-TZVPP-RI for def2-TZVPP, def2-QZVPP-RI for def2-QZVPP, def2-TZVPPD-RI for def2-TZVPPD, etc. For Pople-type minimal and double-$\zeta$ basis sets (i.e., STO-3G, 3-21G, 6-31G**, etc.) the cc-pVDZ-RI basis set, while for triple-$\zeta$ basis sets (i.e., 6-311G, 6-311G**, etc.) the cc-pVTZ-RI basis set will be used as the auxiliary basis; if the basis also includes diffuse functions (i.e., 6-31+G**, 6-311++G**, etc.) the aug-cc-pVDZ-RI and aug-cc-pVTZ-RI basis sets are employed by default.
For the available fitting basis sets see the notes for keyword basis on page 1..
The density fitting approximation can also be invoked by attaching the prefix DF- or RI- to the corresponding option of keyword calc, see the description of calc.
dfbasis_cor=auto for all the correlation methods that use the density fitting approximation by default as well as for local correlation calculations (i.e., localcc $\neq$ off), dfbasis_cor=none otherwise.
To use the cc-pVTZ-RI fitting basis in the correlated calculation for all atoms the input must include dfbasis_cor= cc-pVTZ-RI
Consider the water molecule and use the cc-pVTZ-RI
fitting basis set for the hydrogens and aug-cc-pVTZ-RI for the oxygen.
The following inputs are equivalent:
dfbasis_cor=atomtype
O:aug-cc-pVTZ-RI
H:cc-pVTZ-RI
or
dfbasis_cor=aug'-cc-pVTZ-RI
Consider the water molecule and use the cc-pVTZ
(cc-pVTZ-RI) basis set (fitting basis set) for the hydrogens and
aug-cc-pVTZ (aug-cc-pVTZ-RI.) for the oxygen in a local correlation
calculation.
The following inputs are equivalent:
calc=CCSD(T)
localcc=on
basis=aug'-cc-pVTZ
dfbasis_scf=aug'-cc-pVTZ-RI
dfbasis_cor=aug'-cc-pVTZ-RI
or
calc=LCCSD(T)
basis=aug'-cc-pVTZ
To run a DF-HF calculation with the cc-pVTZ-F12 basis set
and the aug-cc-pVTZ-RI auxiliary basis the input should only include the
following lines:
basis=cc-pVTZ-F12
calc=DF-HF
Specifies whether the density fitting approximation will be used in the HF- or KS-SCF calculation and also specifies the fitting basis set. For the syntax see the description of keyword dfbasis_cor. The important difference is that, if dfbasis_scf=auto, the (aug-)cc-pV$X$Z-RI-JK basis sets will be used as auxiliary basis sets for Dunning’s, Peterson’s, and Pople’s basis sets, while for the def2 basis sets the def2-QZVPP-RI-JK auxiliary basis is taken. For the augmented def2 as well as for the aug-cc-pV$X$Z-PP basis sets the def2-QZVPPD-RI-JK auxiliary basis will be used.
dfbasis_scf=auto if dfbasis_cor$\neq$none and for DFT calculations, dfbasis_scf=none otherwise.
Specifies the integral transformation program to be used for the transformation of three-center Coulomb integrals.
the drpa program will be called
the ovirt program will be called
dfintran=ovirt if ovirt$\neq$off, dfintran=drpa otherwise.
to use the ovirt code set dfintran=ovirt
Use this keyword to perform DFT calculations and to specify the functional.
No DFT calculation is carried out.
The name of the functional, see Table LABEL:FuncTable for the available functionals.
The identifier of a functional implemented in the Libxc library (if installed), such as LDA_X, LDA_C_VWN_1, GGA_X_B88, etc. (see the homepage of the Libxc project [59]).
User-defined functional. Any combination of the following contributions can be defined:
the available standalone functionals, see column “User” in Table LABEL:FuncTable.
the functionals available in the Libxc library (if installed), use simply the Libxc identifier of the functionals (see the homepage of the Libxc project [59]).
the HF exchange, denoted by HFx
the MP2, dRPA, and SOSEX correlation, denoted, respectively, by MP2, dRPA, and SOSEX;
the antiparallel- and parallel-spin components of the latter correlation corrections, add the s and t postfix to the above labels, respectively, e.g., instead of the MP2 label, the MP2s and MP2t labels should be used.
Note that for hybrid functionals, such as B97, the HF exchange will be
neglected. The combination should be specified in the
subsequent lines as follows (see also the examples below):
$<$number of entries$>$
$<$coefficient 1$>$ $<$functional name 1$>$
$<$coefficient 2$>$ $<$functional name 2$>$
$<$coefficient 3$>$ $<$functional name 3$>$
…
User-defined functional, but different functionals
are used for the calculation of the density and the energy. It is useful
for defining special double-hybrid functionals.
The combination should be specified in the
subsequent lines as follows (see also the examples below):
$<$number of entries for density$>$
$<$coefficient 1$>$ $<$functional name 1$>$
$<$coefficient 2$>$ $<$functional name 2$>$
$<$coefficient 3$>$ $<$functional name 3$>$
…
$<$number of entries for energy$>$
$<$coefficient 1’$>$ $<$functional name 1’$>$
$<$coefficient 2’$>$ $<$functional name 2’$>$
$<$coefficient 3’$>$ $<$functional name 3’$>$
…
See option user for the possible values of
$<$functional name n$>$ and $<$functional name n’$>$.
The weight of the HF exchange (HFx), if any, can be different for
the density and the energy, and, in contrast to previous versions of
Mrcc, must be specified also in the second block.
Functional | Description | User |
LDA exchange functionals | ||
LDA | Slater–Dirac exchange (local density approximation) [27, 144, 69] | Yes |
LDA correlation functionals | ||
VWN1 | functional I of Vosko, Wilk, and Nusair [153] | Yes |
VWN2 | functional II of Vosko, Wilk, and Nusair [153] | Yes |
VWN3 | functional III of Vosko, Wilk, and Nusair [153] | Yes |
VWN4 | functional IV of Vosko, Wilk, and Nusair [153] | Yes |
VWN5 | functional V of Vosko, Wilk, and Nusair [153] | Yes |
PZ | Perdew–Zunger 1981 correlation functional [117] | Yes |
PW | Perdew–Wang 1992 correlation functional [116] | Yes |
GGA exchange functionals | ||
B88 | Becke’s 1988 exchange functional [8] | Yes |
PBEx | functional of Perdew, Burke, and Ernzerhof [118] | Yes |
PBEh | 1988 revision of PBEx by Ernzerhof and Perdew [31] | Yes |
PW91x | Perdew–Wang 1991 exchange functional [114] | Yes |
G96 | exchange functional of Gill [118] | Yes |
mPW91x | modified PW91x functional of Adamo and Barone [2] | Yes |
GGA correlation functionals | ||
LYP | correlation functional of Lee, Yang, and Parr [86] | Yes |
P86 | Perdew’s 1986 correlation functional [120] | Yes |
PBEc | functional of Perdew, Burke, and Ernzerhof [118] | Yes |
PW91c | Perdew–Wang 1991 correlation functional [114] | Yes |
GGA exchange-correlation functionals | ||
BLYP | Becke’s 1988 exchange functional [8] and the correlation functional of Lee, Yang, and Parr (B88 + LYP) [86] | No |
BP86 | BP86 exchange-correlation functional (B88 + P86) [8, 120] | No |
PBE | exchange-correlation functional of Perdew, Burke, and Ernzerhof (PBEx + PBEc) [118] | No |
PW91 | Perdew and Wang 1991 exchange-correlation functional (PW91x + PW91c) [114] | No |
HCTH120 | HCTH120 exchange-correlation functional of Boese and co-workers [13] | Yes |
HCTH147 | HCTH147 exchange-correlation functional of Boese and co-workers [13] | Yes |
HCTH407 | HCTH407 exchange-correlation functional of Boese and Handy [14] | Yes |
XLYP | exchange-correlation functional of Xu and Goddard [162] | Yes |
mPWLYP1w | exchange-correlation functional of Dahlke and Truhlar optimized for water [22] | Yes |
Hybrid GGA exchange-correlation functionals | ||
BHLYP | Becke’s half-and-half exchange in combination with the LYP correlation functional (0.5 B88 + 0.5 HF exchange + LYP) [8, 86, 9] | No |
B3LYP | Becke’s three-parameter hybrid functional including the correlation functional of Lee, Yang, and Parr (0.08 LDA + 0.72 B88 + 0.2 HF exchange + 0.19 VWN5 + 0.81 LYP) [8, 27, 144, 153, 10, 86] | No |
B3LYP3 | Becke’s three-parameter hybrid functional including the correlation functional of Lee, Yang, and Parr (0.8 LDA + 0.72 B88 + 0.2 HF exchange + 0.19 VWN3 + 0.81 LYP) [8, 27, 144, 153, 10, 86, 146]. Note that this is equivalent to the B3LYP functional of the Gaussian package. | Yes |
B3PW91 | Becke’s three-parameter hybrid functional including the 1991 correlation functional of Perdew and Wang (0.08 LDA + 0.72 B88 + 0.2 HF exchange + 0.19 VWN5 + 0.81 PW91c) [8, 27, 144, 153, 10, 114] | No |
B1LYP | modified B3LYP functional of Adamo and Barone [1] | Yes |
O3LYP | modified B3LYP functional of Cohen and Handy [20] | Yes |
B97 | Becke’s 1997 exchange-correlation functional (including 0.1943 HF exchange) [11] | Yes |
PBE0 | hybrid functional of Perdew, Burke, and Ernzerhof (0.75 PBEx + 0.25 HF exchange + PBEc) [118, 119] | No |
X3LYP | hybrid functional of Xu and Goddard [162] | Yes |
Meta-GGA exchange functionals | ||
TPSSx | exchange functional of Tao, Perdew, Staroverov, and Scuseria [151] | Yes |
revTPSSx | revised TPSS exchange of Perdew et al. [115] | Yes |
SCANx | exchange functional of Sun, Ruzsinszky, and Perdew [149] | Yes |
Meta-GGA correlation functionals | ||
B95 | Becke’s 1995 correlation functional [6] | Yes |
TPSSc | correlation functional of Tao, Perdew, Staroverov, and Scuseria [151] | Yes |
revTPSSc | revised TPSS correlation of Perdew et al. [115] | Yes |
SCANc | correlation functional of Sun, Ruzsinszky, and Perdew [149] | Yes |
Meta-GGA exchange-correlation functionals | ||
TPSS | exchange-correlation functional of Tao, Perdew, Staroverov, and Scuseria [151] | No |
revTPSS | revised TPSS functional of Perdew et al. [115] | No |
M06-L | 2006 exchange-correlation functional of Zhao and Truhlar [167, 166] | No |
B97M-V | exchange-correlation functional of Mardirossian and Head-Gordon [91] | Yes |
SCAN | exchange-correlation functional of Sun, Ruzsinszky, and Perdew [149] | No |
Hybrid meta-GGA exchange-correlation functionals | ||
M06-2X | 29-parameter exchange-correlation functional of Zhao and Truhlar including 0.54 HF exchange [167] | No |
M08-HX | 47-parameter exchange-correlation functional of Zhao and Truhlar including 0.5223 HF exchange [168] | Yes |
M08-SO | 44-parameter exchange-correlation functional of Zhao and Truhlar including 0.5679 HF exchange [168] | Yes |
TPSSh | hybrid version of TPSS including 0.1 HF exchange [145] | Yes |
revTPSSh | revised TPSSh of Csonka, Perdew, and Ruzsinszky including 0.1 HF exchange [145, 21] | Yes |
mPW1B95 | mixture of mPW91x and B95 by Zhao and Truhlar [164] | Yes |
PW6B95 | mixture of PW91x and B95 by Zhao and Truhlar [165] | Yes |
SCAN0 | hybrid version of SCAN including 0.25 HF exchange [149, 60] | No |
Double hybrid functionals | ||
B2PLYP | Grimme’s two-parameter double hybrid functional including MP2 correction (0.47 B88 + 0.53 HF exchange + 0.73 LYP + 0.27 MP2 correlation) [47] | No |
B2GPPLYP | two-parameter double hybrid functional including MP2 correction of Martin and co-workers (0.35 B88 + 0.65 HF exchange + 0.64 LYP + 0.36 MP2 correlation) [64] | No |
DSDPBEP86 | dispersion corrected, spin-component scaled double hybrid functional of Kozuch and Martin (0.30 PBEx + 0.70 HF exchange + 0.43 P86 + 0.53 MP2 antiparallel-spin correlation + 0.25 MP2 parallel-spin correlation) [70, 71]. Note that the dispersion correction is only included if the -D3 postfix is added (see the note below). | No |
DSDPBEhB95 | dispersion corrected, spin-component scaled double hybrid functional of Kozuch and Martin (0.34 PBEh + 0.66 HF exchange + 0.55 B95 + 0.47 MP2 antiparallel-spin correlation + 0.09 MP2 parallel-spin correlation) [71]. Note that the dispersion correction is only included if the -D3 postfix is added (see the note below). | No |
XYG3 | double hybrid functional of Zhang, Xu, and Goddard (0.2107 B88 - 0.014 LDA + 0.8033 HF exchange + 0.6789 LYP + 0.3211 MP2 correlation evaluated with B2LYP orbitals) [163, 42] | No |
SCAN0-2 | SCAN-based double-hybrid of Hui and Chai (0.793701 HF exchange + 0.206299 SCANx + 0.5 SCANc + 0.5 MP2 correlation [149, 60] | No |
dRPA75 | the dual-hybrid random phase approximation (dRPA75) method of Mezei et al. [99]. The KS orbitals are obtained with the “0.25 PBEx + 0.75 HF exchange + PBEc” functional, while the energy is calculated using the “0.25 PBEx + 0.75 HF exchange + dRPA correlation” expression. Dispersion correction [17] can be included if the -D3 postfix is added. | No |
SCS-dRPA75 | the spin-component scaled dual-hybrid random phase approximation (SCS-dRPA75) method of Mezei et al. [99, 100]. The KS orbitals are obtained with the “0.25 PBEx + 0.75 HF exchange + PBEc” functional, while the energy is calculated using the “0.25 PBEx + 0.75 HF exchange + 1.5 dRPA antiparallel-spin correlation + 0.5 dRPA parallel-spin correlation” expression. | No |
van der Waals density functionals | ||
VV10NL | the nonlocal part (the $\beta N$ term is ignored) of the 2010 van der Waals density functional of Vydrov and Van Voorhis [154], both self-consistent and non-self-consistent implementations are available, see also the the comment below | Yes |
dft=off
Empirical dispersion corrections can be calculated for particular
functionals and also for the HF energy using the DFT-D3 approach of
Grimme and co-workers [44, 45] by attaching the
-D3 postfix to the corresponding options: BLYP-D3,
BHLYP-D3, B3LYP-D3, B3PW91-D3, BP86-D3,
PBE-D3, PBE0-D3, HCTH120-D3, B2PLYP-D3,
mPW1B95-D3, TPSS-D3, TPSSh-D3,
B2GPPLYP-D3, DSDPBEP86-D3, DSDPBEhB95-D3,
dRPA75-D3,
HF-D3.
See also the description of keyword edisp.
For a simple DFT calculation (i.e., without subsequent correlation calculations) the value of keyword calc can be SCF, HF, RHF, or UHF. Note that you do not need to set its value since it is set to SCF by default. Alternatively, you can select the DFT functional using keyword calc, and in this case you do not have to set keyword dft (see the description of calc).
For a correlated calculation with KS orbitals you should select the functional with this keyword, and the value of keyword calc must be set to the desired correlation method. Note that you can also accelerate the post-KS calculation using local correlation schemes (e.g., local dRPA). See the examples below.
For a correlated calculation with KS orbitals (excluding calculations with double hybrid functionals) the HF energy computed with KS orbitals is used as reference energy.
For the B2PLYP, B2GPPLYP, DSDPBEP86, DSDPBEhB95, dRPA75, etc. double hybrid functionals as well as for user-defined double hybrid functionals including MP2 (SCS-MP2), dRPA, etc. correlation calc is automatically set to MP2, dRPA, etc. Note that you can accelerate the MP2, dRPA, …part of a double hybrid DFT calculation for large molecules using local correlation approaches. For the built-in double hybrid functionals just add the “L” prefix, while for the user-defined functionals set localcc=on. See the examples below.
The DSDPBEP86, DSDPBEhB95, and dRPA75 functionals use special parameters for the calculation of the D3 correction which are read by the DFT-D3 program from the .dftd3par.$HOST file located in your home directory. This file will be created by the program, but you must be sure that the program is able to access your home directory. Also note that, if you already have this file in your home, it will be overwritten, so please do not forget to save it before executing Mrcc.
For the VV10 van der Waals functional you can modify parameters $b$ and $C$ (see Ref. 154) if it is used with the user or userd options. For that purpose the two parameters should be specified after the VV10NL flag separated by spaces, see the example below. If the parameters are not set, those of Ref. 154 will be used.
To perform a DFT calculation with the B3LYP functional give dft=B3LYP or calc=B3LYP
The B3LYP functional can also be defined using the
user option as
calc=scf
dft=user
5
0.08 LDA
0.72 B88
0.20 HFx
0.19 VWN5
0.81 LYP
The B2PLYP double-hybrid functional can also be defined
using the user option as
calc=scf
dft=user
4
0.47 B88
0.73 LYP
0.53 HFx
0.27 MP2
The DSDPBEP86 double-hybrid functional can also be defined
using the user option as
calc=SCF
dft=user
5
0.30 PBEx
0.43 P86
0.70 HFx
0.53 MP2s
0.25 MP2t
SOSEX calculation with Kohn–Sham orbitals calculated with the
LDA exchange functional:
calc=SOSEX
dft=LDA
To perform a DFT calculation with the B2PLYP double-hybrid functional and add the D3 dispersion correction set dft=B2PLYP-D3 or calc=B2PLYP-D3
B2PLYP calculation, the MP2 contribution is evaluated using local
MP2 approximation:
calc=LB2PLYP
User-defined functional, different functionals are used for the
calculation of the density (0.25 PBEx + 0.75 HF exchange +
PBEc) and the energy (0.50 PBEx + 0.50 HF exchange +
MP2 correlation).
dft=userd
3
0.75 HFx
0.25 PBEx
1.00 PBEc
3
0.50 HFx
0.50 PBEx
1.00 MP2
The dRPA75 dual-hybrid functional can also be defined
using the userd option as
dft=userd
3
0.75 HFx
0.25 PBEx
1.00 PBEc
3
0.75 HFx
0.25 PBEx
1.00 dRPA
Local dRPA calculation with Kohn–Sham orbitals calculated with the
PBE functional:
calc=LdRPA
dft=PBE
To perform a DFT calculation with the B3LYP functional using its Libxc implementation set calc=HYB_GGA_XC_B3LYP5
The B3LYP functional can also be defined using the user option
and the functionals implemented in the Libxc library as
dft=user
5
0.08 LDA_X
0.72 GGA_X_B88
0.20 HFx
0.19 LDA_C_VWN
0.81 GGA_C_LYP
DFT calculation with a user-defined PBE0-VV10 functional. Parameter $b$
of VV10 is modified, while for $C$ its default value, 0.0093, is used.
If you do not want to modify either $b$ or $C$, simply drop the two
numbers for the VV10NL entry.
dft=userd
3
0.75 PBEx
0.25 HFx
1.00 PBEc
4
0.75 PBEx
0.25 HFx
1.00 PBEc
1.00 VV10NL 8.0 0.0093
Type of diagonalization algorithm used for the CI and LR-CC calculations.
Standard Davidson diagonalization
Davidson diagonalization with root-following, recommended for excited-state calculations if the initial guess is given manually or the calculation is restarted
diag=david
for root-following type diag=follow
Radius of atom domains for the local correlation method of Ref. 138 (localcc=2013). For each localized MO (LMO), using the Boughton–Pulay procedure [16], we assign those atoms to the LMO on which it is localized. Then, for each LMO an atom domain is constructed in two steps, the LMO is called the central LMO of the domain. In the first step, those atoms are included in the domain whose distance from the atoms assigned to the central LMO is smaller than domrad. In the second step, those LMOs are identified which are localized on the atoms selected in the first step, and the domain is extended to include all atoms assigned to these LMOs.
In the first step of the construction of atom domains all atoms whose distance from the atoms assigned to the central LMO is smaller than this number (in bohr) will be included in the domain.
Infinite radius will be applied, i.e., there is only one atom domain including all atoms.
domrad=10.0
To use the local CC methods as defined in Ref. 135 set domrad=inf, that is, use only one atom domain including all atoms.
to set a threshold of 12.0 bohr type domrad=12.0
Specifies the type of the algorithm for the solution of the dRPA equations or the calculation of SOS-MP2 energies. See Ref. 85 for more details.
The algorithm of Ref. 58 will be used, the fitting of integral lists will be performed before the dRPA iterations (SOS-MP2 calculation).
The algorithm of Ref. 85 will be executed, the fitting of the integrals is not performed. This algorithm is efficient for large molecules.
The dRPA correlation energy is calculated using the plasmon formula.
The algorithm is automatically selected on the basis of the size of the molecule (canonical dRPA) or the HOMO-LUMO gap (local dRPA).
For SOSEX calculations drpaalg=fit is the only option, which is forced by the program.
For canonical dRPA the algorithm using the plasmon formula scales as $N^{6}$, it is only competitive for smaller molecules but inefficient for bigger ones. It avoids, however, the problems of the other algorithms, that is, convergence problems and unphysical solutions. Thus, it is useful for testing.
For local dRPA drpaalg=plasmon is also linear scaling but typically 2- to 4-times slower than drpaalg=fit. It is advantageous for the aforementioned reasons. If drpaalg=auto, the plasmon formula-based algorithm is executed if the HOMO-LUMO gap is lower than 0.05 E${}_{h}$.
drpaalg=fit and drpaalg=auto for canonical and local dRPA, respectively.
to set the second option give drpaalg=nofit
Activates dual basis set calculations. For these calculations two basis sets must be specified: a smaller one by keyword basis_sm (see the description of the keyword) and a bigger basis defined by keyword basis. The energy evaluated with the bigger basis set is estimated from a small-basis calculation. See Ref. for more details.
off No dual basis calculation.
on Dual basis set calculation for conventional SCF and correlated methods. First, an SCF calculation will be performed using the small basis set. Second, one iteration of a SCF calculation is carried out with the large basis, and the energy is extrapolated using a first-order formula. If a correlation calculation is requested, the orbitals obtained in the second SCF step will be used for that purpose.
e1 Dual basis set embedding, Ansatz 1 of Ref. . A Huzinaga-embedding calculation is performed with the small basis set. The steps of the large-basis Huzinaga-embedding calculation are non-iterative. See also the description of keyword embed.
e2 Dual basis set embedding, Ansatz 2 of Ref. . Similar to e1, but there is also an iterative step with the large basis.
dual=off
To perform a dual basis set PBE calculation with the cc-pVTZ and cc-pVDZ
basis sets you need:
basis=cc-pVTZ
basis_sm=cc-pVDZ
dual=on
calc=PBE
Dual basis set PBE-in-LDA calculation with Ansatz 1 using the cc-pVTZ
and cc-pVDZ basis sets as large and small basis set, respectively;
atoms 1 to 5 are included in the embedded subsystem:
basis=cc-pVTZ
basis_sm=cc-pVDZ
calc=PBE
dual=e1
embed=Huzinaga
1-5
LDA
0
Dual basis set PBE-in-LDA calculation with Ansatz 1 using a mixed large
basis (cc-pVTZ for atoms 1 to 5, cc-pVDZ otherwise) and the cc-pVDZ
basis sets as the small basis set;
atoms 1 to 5 are included in the embedded subsystem:
basis=embed
cc-pVTZ
cc-pVDZ
basis_sm=cc-pVDZ
calc=PBE
dual=e1
embed=Huzinaga
1-5
LDA
0
Specifies the effective core potential (ECP) used in all calculations. By default the ECPs are taken from the files named by the chemical symbol of the elements, which can be found in the BASIS directory created at the installation. The ECPs are stored in the format used by the Cfour package. In addition to the ECPs provided by default, any ECP can be used by adding it to the corresponding files in the BASIS directory. Alternatively, you can also specify your own ECP in the file GENBAS which must be copied to the directory where Mrcc is executed.
No ECPs will be used.
The ECPs will be automatically selected: no ECP will be used for atoms with all-electron basis sets, while the ECP adequate for the basis set of the atom will be selected otherwise.
If the same ECP is used for all atoms, the label of the ECP can be given here.
If different ECPs are used or no ECP is used for particular atoms, but the atoms of the same type are treated in the same way, ecp=atomtype should be given, and the user must specify the ECP for each atomtype (for which an ECP is used) in the subsequent lines as $<$atomic symbol$>$:$<$ECP label$>$ .
In the general case, if different ECPs are used for each atom, then one should give ecp=special and specify the ECP for each atom in the subsequent lines by giving the label of the corresponding ECP (or none if no ECP is used for that atom) in the order the atoms appear at the specification of the geometry.
By default the following ECP are available for elements Na to Rn in Mrcc:
Please note that some of the above ECPs are not available for all elements.
If you use your own ECPs, these must be copied to the end of the corresponding file in the BASIS directory. Alternatively, you can also create a file called GENBAS in the directory where Mrcc is executed, and then you should copy your ECPs to that file.
The labels of the ECPs must be identical to those used in the BASIS/* files (or the GENBAS file). For the default ECPs just type the name of the ECPs as given above, e.g., LANL2DZ-ECP-10, def2-ECP-28, etc. If you employ non-default ECPs, you can use any label.
ecp=auto
To use the MCDHF-ECP-10 pseudopotential for all atoms the input must include ecp=MCDHF-ECP-10
Consider the PbO molecule and use the def2-SVP basis set
for both elements as well as the def2-ECP-60 pseudopotential for Pb.
The following inputs are equivalent.
Input 1:
basis=def2-SVP
geom
Pb
O 1 R
R=1.921813
Input 2:
basis=def2-SVP
ecp=atomtype
Pb:def2-ECP-60
geom
Pb
O 1 R
R=1.921813
Input 3:
basis=def2-SVP
ecp=special
def2-ECP-60
none
geom
Pb
O 1 R
R=1.921813
This keyword controls the calculation of empirical dispersion corrections for DFT and HF calculations using the DFT-D3 approach of Grimme and co-workers [44, 45]. The corrections are evaluated by the dftd3 program of the latter authors, which is available at http://www.thch.uni-bonn.de/tc/ and interfaced to Mrcc. You need to separately install this code and add the directory where the dftd3 executable is located to your PATH environmental variable.
No dispersion correction will be computed.
The dispersion correction will be automatically evaluated to the KS or HF energy. Note that it is only possible for particular functionals listed in the description of keyword dft (and the HF method). For these methods, however, you can also turn on the calculations of the dispersion corrections by attaching the -D3 postfix to the corresponding options, e.g., as BLYP-D3, B3LYP-D3, B2PLYP-D3, etc. (see the description of keyword dft).
You can directly give any options of the dftd3 code. The options will be passed over to dftd3 without any consistency check, the user should take care of the compatibility of these options with the calculation performed by Mrcc. Note that the coordinate file name must not be specified here, the coordinates will be taken from the COORD.xyz file generated by Mrcc.
If edisp=auto or the -D3 postfix is added to the corresponding options, the empirical dispersion correction is by default evaluated with the Becke and Johnson (BJ) damping function [45].
edisp=off
to calculate the D3 dispersion correction including BJ damping to the B3LYP energy give calc=B3LYP-D3
to calculate the D3 dispersion correction to the
B3LYP energy without the BJ damping the input should include:
calc=B3LYP
edisp=-func b3-lyp -zero
This keyword controls DFT embedding calculations. Currently it is only available for closed-shell systems using density-fitting.
No embedding.
The Huzinaga-equation-based embedding approach [62] will be used. The embedded atoms and the low-level DFT approach (or HF) used for the embedding must be specified and the number of embedded orbitals can be given in the subsequent lines as follows. The embedded atoms must be given by their serial numbers in the first line as $<n_{1}>$,$<n_{2}>$,…,$<n_{k}>$-$<n_{l}>$,…, where $n_{i}$’s are the serial numbers of the atoms. Serial numbers separated by dash mean that $<n_{k}>$ through $<n_{l}>$ are embedded atoms. Note that the numbering of the atoms must be identical to that used in the Z-matrix or Cartesian coordinate specification, but dummy atoms must be excluded. The low-level DFT (LDA, GGA, or hybrid) or HF approach must be specified in the second line using the corresponding option of keyword dft (for HF simply HF). The high-level method (any DFT, HF, or any correlation method) for the active region should be specified by the keyword calc (or keywords calc and dft if a KS reference is used in a correlation calculation). In the third line an integer should be given which is the number of the embedded orbitals or zero if the latter is determined automatically. In addition, the algorithm for the selection of the orbitals can also be given in the third line after the integer. The options are aMul and bopu, which mean the Mulliken population- and the Boughton–Pulay algorithm-based schemes of Refs. 62 and , respectively. For aMul you can also specify the Mulliken population threshold (see the appendix of Ref. ). The threshold for the bopu algorithm can be controlled by the bpcompo keyword. The default is aMul with a threshold of 0.3. See also examples below.
The projector-based embedding approach of Manby and co-workers [90] will be used. The embedded atoms and the low-level DFT approach can be specified as described above.
embed=off
CCSD(T)-in-PBE embedding with the Huzinaga-equation-based
approach, atoms 1 and 2 are included in the embedded region, the number
of the embedded orbitals is determined automatically, the aMul
algorithm is used for the selection of the orbitals with the default
threshold:
calc=DF-CCSD(T)
embed=huzinaga
1-2
PBE
0
The same as example 1, but the aMul algorithm is
used with a threshold of 0.25:
calc=DF-CCSD(T)
embed=huzinaga
1-2
PBE
0 amul 0.25
The same as example 1, but the bopu algorithm is
used:
calc=DF-CCSD(T)
embed=huzinaga
1-2
PBE
0 bopu
Same as example 1, but a mixed basis set is used, cc-pVDZ
for the environment and cc-pVTZ for the embedded subsystem:
calc=DF-CCSD(T)
basis=embed
cc-pVDZ
cc-pVTZ
embed=huzinaga
1-2
PBE
0
dRPA@PBE-in-PBE embedding with the Huzinaga-equation-based
approach, atoms 1, 2, 3, and 5 as well as 10 orbitals are included in
the active region:
calc=dRPA
dft=PBE
embed=huzinaga
1-3,5
PBE
10
Use this option to add an external perturbation to the Hamiltonian, e.g., an external electric dipole field.
No perturbations are added.
the number of the
operators added to the Hamiltonian. The operators and the corresponding
coefficients (in a.u.) should be specified in the subsequent lines as
follows:
$<$operator 1$>$ $<$coefficient 1$>$
$<$operator 2$>$ $<$coefficient 2$>$
$<$operator 3$>$ $<$coefficient 3$>$
…
where the operator can be x, y, z, xx, yy,
zz, xy, xz, yz, xxx, xxy,
xxz, xyy, xyz, xzz, yyy, yyz,
yzz, zzz.
The symmetry of the perturbation is not taken care of automatically. If the perturbation lowers the symmetry of the system, you must change the computational point group (keyword cmpgrp) or turn off symmetry (symm=off).
epert=none
to add the $\hat{y}$ and $\hat{z}$ dipole length
operators to the Hamiltonian with coefficients 0.01 and 0.001 a.u.,
respectively, the input should include the following lines
epert=2
y 0.01
z 0.001
Threshold for the cumulative populations of MP2 natural orbitals (NOs) or optimized virtual orbitals (OVOs), to be used together with keyword ovirt. The cumulative population for an MO is calculated by summing up the occupation number of that particular MO and all the MOs with larger occupation numbers, and then this number is divided by the number of electrons. See Ref. 136 for more details.
Virtual orbitals with cumulative populations of higher than this number will be dropped.
eps=0.975
to set a threshold of 0.95 type eps=0.95
Sets the radius of local fitting domains for the exchange contribution in direct density-fitting SCF calculations [130, 105]. In direct DF-SCF calculations, in each iteration step, the MOs are localized. For each localized MO Löwdin atomic charges are computed, and all atoms are selected which have a charge greater than 0.05. All further atoms will be included in the fitting domain of the MO for which the electron repulsion integrals including the corresponding AOs and the basis functions residing on the atoms selected in the first step are estimated to be greater than a threshold.
Threshold for the integrals (in E${}_{h}$).
A threshold of zero will be applied, i.e., a conventional direct DF-SCF calculation will be executed.
Local fitting domains are currently available only for RHF and RKS wave functions.
For average organic molecules with localized electronic structure excrad=1.0 is a good choice. For more complicated systems other thresholds may be necessary. For excrad=1.0 excrad_fin is set to $10^{-3}$, which is fine with basis sets excluding diffuse functions. For basis sets with diffuse functions excrad_fin=1e-5 or tighter is recommended.
excrad=0
to set a threshold of 1.0 E${}_{h}$ type excrad=1.0
In density-fitting SCF calculations, if excrad and excrad_fin differ, an extra iteration is performed to get an accurate SCF energy. excrad_fin specifies the radius of local fitting domains for the exchange contribution in this iteration step. See also notes for keyword excrad.
See the description of keyword excrad.
excrad_fin=excrad/1000
to avoid the use of local fitting domains in the extra iteration step give excrad_fin=0.0
Requests harmonic vibrational frequency calculation (numerical). Ideal gas thermodynamic properties will also be evaluated in the rigid-rotor harmonic-oscillator approximation. If geometry optimization is also carried out, i.e., gopt $\neq$ off, the frequencies are calculated at the optimized geometry.
on or off
You should also set this keyword if you are interested thermodynamic properties of atoms.
freq=off
for a frequency calculation set freq=on
Specifies whether spherical harmonic or Cartesian Gaussian basis functions will be used.
Spherical harmonic Gaussians will be used
Cartesian Gaussians will be used
For calculations using the density fitting (DF) approximation, if intalg=os or intalg=auto, the Coulomb integrals are evaluated by algorithms [3, 139] which only enable the use of spherical harmonic Gaussians. Consequently, Cartesian Gaussians are only available with intalg=rys in DF calculations (see the description of keyword intalg).
The derivative integrals are evaluated by the solid-harmonic Hermite scheme [133] (see the description of keyword intalg), consequently, differentiated integrals, and thus energy derivatives cannot be evaluated with Cartesian Gaussian basis sets.
gauss=spher
for Cartesian Gaussians the user should set gauss=cart
Specifies the format of molecular geometry. The geometry must be given in the corresponding format in the subsequent lines.
Usual Z-matrix format. In the Z-matrix the geometrical parameters can only be specified as variables, and the variables must be defined after the matrix, following a blank line. Another blank line is required after the variables. This Z-matrix format is compatible to that of Cfour and nearly compatible to that for Gaussian and Molpro. Z-matrices can be generated by Molden (see also Sect. 14.1), then the Gaussian-style Z-matrix format must be chosen. The symbol for dummy atoms is “X”.
Cartesian coordinates in xyz format, that is, the number of atoms, a blank line, then for each atom the atomic symbol or atomic number and the $x$, $y$, and $z$ components of Cartesian coordinates. Cartesian coordinates in xyz format can also be generated by Molden (see also Sect. 14.1).
Cartesian coordinates in a format similar to that used by the Turbomole package, that is, the number of atoms, a blank line, then for each atom the $x$, $y$, and $z$ components of Cartesian coordinates and the atomic symbol or atomic number.
Cartesian coordinates and connectivity in .mol format, that is, the number of atoms and number of bonds in the first line, then for each atom the $x$, $y$, and $z$ components of Cartesian coordinates and the atomic symbol, then for each bond the serial number of the atoms connected by the bond and the type of the bond (1 for single bond, etc.). This geometry specifications is needed if the specified method requires the connectivity.
For the use of ghost atoms see the description of keyword ghost.
geom=zmat, which is equivalent to geom, i.e., if it is not specified whether the geometry is supplied in Z-matrix format or in other formats, Z-matrix format is supposed. Nevertheless, the coordinates must be given in the subsequent lines in any case.
the following five geometry inputs for H${}_{2}$O${}_{2}$ are equivalent
Z-matrix format, bond lengths in Å:
geom
H
O 1 R1
O 2 R2 1 A
H 3 R1 2 A 1 D
R1=0.967
R2=1.456
A=102.32
D=115.89
xyz format, coordinates in bohr, atoms are specified by
atomic symbols:
unit=bohr
geom=xyz
4
H 0.00000000 0.00000000 0.00000000
O 1.82736517 0.00000000 0.00000000
O 2.41444411 2.68807873 0.00000000
H 3.25922198 2.90267673 1.60610134
xyz format, coordinates in bohr, atoms are specified by
atomic numbers:
unit=bohr
geom=xyz
4
1 0.00000000 0.00000000 0.00000000
8 1.82736517 0.00000000 0.00000000
8 2.41444411 2.68807873 0.00000000
1 3.25922198 2.90267673 1.60610134
Turbomole format, coordinates in bohr, atoms are
specified by atomic symbols:
unit=bohr
geom=tmol
4
0.00000000 0.00000000 0.00000000 H
1.82736517 0.00000000 0.00000000 O
2.41444411 2.68807873 0.00000000 O
3.25922198 2.90267673 1.60610134 H
.mol format, coordinates in bohr:
unit=bohr
geom=mol
4 3
0.00000000 0.00000000 0.00000000 H
1.82736517 0.00000000 0.00000000 O
2.41444411 2.68807873 0.00000000 O
3.25922198 2.90267673 1.60610134 H
1 2 1
2 3 1
3 4 1
Ghost atoms can be specified using this keyword, e.g., for the purpose of basis set superposition error (BSSE) calculations with the counterpoise method.
There are no ghost atoms.
Using this option one can select the ghost atoms specifying their serial numbers. The latter should be given in the subsequent line as $<n_{1}>$,$<n_{2}>$,…,$<n_{k}>$-$<n_{l}>$,…, where $n_{i}$’s are the serial numbers of the atoms. Serial numbers separated by dash mean that $<n_{k}>$ through $<n_{l}>$ are ghost atoms. Note that the numbering of the atoms must be identical to that used in the Z-matrix or Cartesian coordinate specification, but dummy atoms must be excluded.
ghost=none
Rectangular HF dimer, the atoms of the second HF molecule
are ghost atoms:
geom
H
F 1 R1
H 2 R2 1 A
F 3 R1 2 A 1 D
R1=0.98000000
R2=2.00000000
A=90.00000000
D=0.000000000
ghost=serialno
3-4
Ammonia, the third hydrogen is a ghost atom (note that the
serial number of the hydrogen is 4 instead of 5 because of the dummy
atom:
geom
X
N 1 R
H 2 NH 1 AL
H 2 NH 1 AL 3 A
H 2 NH 1 AL 3 B
R=1.00000000
NH=1.01000000
AL=115.40000000
A=120.00000000
B=-120.00000000
ghost=serialno
4
Requests geometry optimization. Currently only the full geometry optimization is supported, geometrical parameters cannot be frozen.
no geometry optimization.
full geometry optimization.
The coordinates in the MINP file are replaced by the converged ones at the end of the geometry optimization. The initial MINP file is saved as MINP.init.
The Abelian symmetry of the molecule is utilized at the calculation of gradients and update of the coordinates, thus, the computational point group is preserved during the optimization.
gopt=off
to carry out a full geometry optimization set gopt=full
Threshold for automatic point group recognition. Two atoms will be considered symmetry-equivalent if the difference in any component of their Cartesian coordinates after the symmetry operation is less than $10^{-{\tt gtol}}$ bohr.
$<$any integer$>$
gtol=7
for a tolerance of $10^{-4}$ bohr give gtol=4
This keyword is useful for the analysis of HF, KS, or correlated (MP2, CI, CC, …) one-electron density and its derivatives. The one-electron density, its gradient, and Laplacian will be calculated on a grid used for DFT calculations (see keywords agrid and rgrid) and saved for external use. In the case of correlated calculations the densities are evaluated using the relaxed density matrices.
Densities are not evaluated.
The one-electron density and its derivatives are
calculated in the grid points. These values together with the grid are
written to the unformatted Fortran file DENSITY. If a correlation
calculation is performed the densities calculated with the
correlation method are stored in the DENSITY file, while the SCF
densities are saved to the file DENSITY.SCF.
For restricted orbitals the files use the following format:
$N$
$\mathbf{r}_{1}$ $w_{1}$ $\rho(\mathbf{r}_{1})$ $\nabla\rho(\mathbf{r}_{1})$ $\nabla^{2}\rho(\mathbf{r}_{1})$
$\mathbf{r}_{2}$ $w_{2}$ $\rho(\mathbf{r}_{2})$ $\nabla\rho(\mathbf{r}_{2})$ $\nabla^{2}\rho(\mathbf{r}_{2})$
⋮
$\mathbf{r}_{N}$ $w_{N}$ $\rho(\mathbf{r}_{N})$ $\nabla\rho(\mathbf{r}_{N})$ $\nabla^{2}\rho(\mathbf{r}_{N})$
where $N$ is the number of grid points, $\mathbf{r}_{i}$ = ($x_{i}$, $y_{i}$,
$z_{i}$) is the Cartesian coordinate of grid point $i$ with $w_{i}$ as
the corresponding weight, and $\rho(\mathbf{r}_{i})$ is the density in
point $i$. For unrestricted calculations the corresponding $\alpha$ and
$\beta$ quantities are stored separately, and the lines of the files
change as
$\mathbf{r}_{i}$ $w_{i}$ $\rho_{\alpha}(\mathbf{r}_{i})$ $\rho_{\beta}(\mathbf{r}_{i})$ $\nabla\rho_{\alpha}(\mathbf{r}_{i})$ $\nabla\rho_{\beta}(\mathbf{r}_{i})$ $\nabla^{2}\rho_{\alpha}(\mathbf{r}_{i})$ $\nabla^{2}\rho_{\beta}(\mathbf{r}_{i})$
grdens=off
to save the densities give grdens=on
The keyword controls the fineness of the angular and radial integration grids employed in DFT calculations. The tolerance for the accuracy of angular integrals will be $10^{-{\tt grtol}}$, while the number of radial grid points increases linearly with grtol. See also the description of keywords agrid and rgrid.
$<$any positive integer$>$
meta-GGA functionals or molecules with special bonding characteristics may require larger integration grids, and it is recommended to run test calculations to decide if the default value of grtol is sufficient.
grtol=10
for a fine integration grid give grtol=12
Specifies what type of Hamiltonian is used in relativistic calculations. This keyword has only effect if iface=Dirac.
exact 2-component molecular-mean-field Hamiltonian [143]
other types of relativistic Hamiltonians such as the full Dirac–Coulomb Hamiltonian or the exact 2-component Hamiltonian
hamilton=DC
if you use the exact 2-component molecular-mean-field Hamiltonian, set hamilton=X2Cmmf
Specifies whether Mrcc is used together with another program system. In this case the transformed MO integrals are calculated by that program and not by Mrcc. See Sect. 5 for the description of various interfaces.
Transformed MO integrals are calculated by Mrcc.
Mrcc is interfaced to Cfour.
Mrcc is interfaced to Columbus.
Mrcc is interfaced to Dirac.
Mrcc is interfaced to Molpro.
If you use Mrcc together with Cfour or Molpro, you do not need to use this keyword. The Mrcc input file is automatically written and Mrcc is automatically called by these program systems. The user is not required to write the Mrcc input file, most of the features of Mrcc can be controlled from the input files of these programs. With Cfour the user has the option to turn off the automatic construction of the Mrcc input file by giving INPUT_MRCC=OFF in the Cfour input file ZMAT. In the latter case one should use this keyword.
If you use Mrcc together with Columbus or Dirac, this keyword must be always given.
iface=none, that is, all calculations will be performed by Mrcc.
to carry out four-component relativistic calculations using the Dirac interface give iface=Dirac
Specifies the algorithm used for the evaluation of two-electron integrals over primitive Gaussian-type orbitals.
Depending on the angular momenta the program automatically determines which of the two algorithms is executed. For integrals of low angular momentum functions the Rys procedure is used, while the Obara–Saika algorithm is executed otherwise.
The integrals over contracted Gaussians are evaluated by the solid-harmonic Hermite scheme of Reine et al. [133].
For calculations using the density fitting (DF) approximation intalg=auto is equivalent intalg=os since the Obara–Saika algorithm is more efficient for any integrals.
For DF methods option herm is not available.
For DF methods, if intalg=os or intalg=auto the Coulomb integrals are evaluated by the algorithm of Ref. 139, which only enables the use of spherical harmonic Gaussians. Consequently, Cartesian Gaussians are only available with intalg=rys in DF calculations (see the description of keyword gauss).
The derivative integrals are evaluated by the solid-harmonic Hermite scheme even if another option is used for the undifferentiated integrals. Consequently, differentiated integrals, and thus energy derivatives cannot be evaluated with Cartesian Gaussian basis sets.
intalg=auto
to use the Obara–Saika scheme for all angular momenta add intalg=os
Threshold for integral calculation. Integrals less than $10^{-{\tt itol}}$ E${}_{h}$ will be neglected.
$<$any integer$>$
itol=max(10, scftol+4, scfdtol), but itol is changed to itol+1 if basis functions are dropped because of linear dependence (see keyword ovltol)
for an accuracy of $10^{-15}$ E${}_{h}$ one must give itol=15
Specifies the accuracy of the numerical Laplace transform in the (T) correlation energy term of local CCSD(T) calculations with localcc=2016 or 2018. See also the description of keyword talg and Ref. 104.
The (T) energy denominator will be approximated using its numerical Laplace transform. The number of quadrature points ($n_{\mathrm{q}}$), and hence the accuracy is determined by this number. The minimum value of $n_{\mathrm{q}}$ is also set by this number as $n_{\mathrm{q}}>|\mathrm{log}_{10}(\texttt{laptol})|$.
laptol=$10^{-2}$, but laptol=$10^{-3}$ is set if lcorthr=tight. See also the description of lcorthr for further details.
to use a threshold of $10^{-3}$ type laptol=1e-3
Use this keyword to restart local CC calculations in the case of localcc=2015, localcc=2016, and localcc=2018, e.g., after power failure. For the restart with lccrest=on the LMP2 calculation and integral transformations have to be completed, and for the remaining domains the DFINT_AI.*, DFINT_AB.*, DFINT_IJ.*, ajb.*, 55.*, 56, localcc.restart, and VARS files are required. In the case of localcc=2016 or localcc=2018 and talg=lapl or topr the laplbas.* files are also needed.
If the loop for the extended domains has started but was not finish in the LMP2 calculation or in the LMP2 part of and LNO-CC calculation with localcc=2016 or localcc=2018, the calculation can be restarted with the lccrest=domain option. In this case all intermediate files located in the folder of execution have to be kept intact, and only the updated MINP file should be overwritten before the calculation is restarted. Note that the beginning of the computation up to the pair energy evaluation is repeated in the restarted run, and the loop over the extended domains will continue from the index of the first unfinished domain.
on, off, or domain.
lccrest=off
to restart a local CCSD(T) calculation set lccrest=on or lccrest=domain depending on the point of interruption
Controls the accuracy of local correlation calculations by setting the relevant thresholds: bp*, lnoepso, lnoepsv, laptol, naf_cor, osveps, wpairtol, spairtol (see also Refs. 85, 105, and 106 for details).
The truncation thresholds will be set so that the canonical energy be reproduced, it is only useful for testing.
Expected accuracy. Using the Normal settings for local MP2 and CCSD(T), if localcc=2018, 1 kJ/mol (1 kcal/mol) average (maximum) errors are expected in energy differences even for relatively complicated or sizable systems (see Refs. 105 and 106). In the case of localcc=2015 considering local dRPA and dRPA related methods the expected average (maximum) errors for energy differences are 2 kJ/mol (2 kcal/mol) with Loose and 1 kJ/mol (1 kcal/mol) with Tight settings (see Ref. 85).
For local MP2 naf_cor=off is set if localcc=2015. Keywords lnoepso, lnoepsv, and laptol are irrelevant for local MP2 calculations.
calc | MP2 | CC | all | ||||
---|---|---|---|---|---|---|---|
localcc | 2018 | 2018 | |||||
lcorthr | Loose | Normal | Tight | Loose | Normal | Tight | 0 |
bpedo | 0.9999 | 0.9999 | 0.99995 | 0.9999 | 0.9999 | 0.99995 | 1.0 |
wpairtol | 3e-5 | 1e-5 | 3e-6 | 3e-5 | 1e-5 | 3e-6 | 0.0 |
lnoepso | - | - | - | 3e-5 | 1e-5 | 3e-6 | 0.0 |
lnoepsv | - | - | - | 3e-6 | 1e-6 | 3e-7 | 0.0 |
laptol | - | - | - | 1e-1 | 1e-2 | 1e-3 | - |
naf_cor | 2e-3 | 2e-3 | 2e-3 | 1e-2 | 1e-2 | 1e-2 | off |
bpcompo | 0.985 | 0.985 | 0.985 | 0.985 | 0.985 | 0.985 | 1.0 |
bpcompv | 0.98 | 0.98 | 0.98 | 0.98 | 0.98 | 0.98 | 1.0 |
bppdo | 0.999 | 0.999 | 0.999 | 0.999 | 0.999 | 0.999 | 1.0 |
bppdv | 0.98 | 0.98 | 0.98 | 0.98 | 0.98 | 0.98 | 1.0 |
bpedv | 0.995 | 0.995 | 0.995 | 0.995 | 0.995 | 0.995 | 1.0 |
osveps | off | off | off | off | off | off | off |
spairtol | off | off | off | off | off | off | off |
calc | MP2, dRPA, CC | MP2 | CC | all | |||
---|---|---|---|---|---|---|---|
localcc | 2015 | 2016 | 2016 | ||||
lcorthr | Normal | Tight | Normal | Tight | Normal | Tight | 0 |
bpedo | - | - | 0.9998 | 0.9999 | 0.9999 | 0.99995 | 1.0 |
wpairtol | 1e-6 | 1e-7 | 1.5e-5 | 1e-5 | 1e-5 | 3e-6 | 0.0 |
spairtol | 1e-4 | 1e-5 | off | off | off | off | 0.0 |
osveps | 1e-3 | 1e-4 | off | off | off | off | 0.0 |
lnoepso | 3e-5 | 1e-5 | - | - | 2e-5 | 1e-5 | 0.0 |
lnoepsv | 1e-6 | 3e-7 | - | - | 1e-6 | 5e-7 | 0.0 |
laptol | - | - | - | - | 1e-2 | 1e-3 | - |
naf_cor | 1e-2 | 8e-3 | 2e-3 | 2e-3 | 1e-2 | 1e-2 | off |
bpcompo | 0.985 | 0.985 | 0.985 | 0.985 | 0.985 | 0.985 | 1.0 |
bpcompv | 0.98 | 0.98 | - | - | - | - | 1.0 |
bppdo | - | - | 0.999 | 0.999 | 0.999 | 0.999 | 1.0 |
bppdv | - | - | 0.98 | 0.98 | 0.98 | 0.98 | 1.0 |
bpedv | - | - | 0.995 | 0.995 | 0.995 | 0.995 | 1.0 |
lcorthr=Normal
to use tight thresholds set lcorthr=Tight
Determines whether the MP2 density matrix fragments are calculated using the “correct” expressions derived for the general type of orbitals, or using the expressions derived for the canonical case (as described in Ref. 135).
The MP2 density matrix fragments are calculated using the correct, non-canonical expressions.
The MP2 density matrix fragments are calculated using the approximate canonical expressions (as defined in Ref. 135).
To reproduce the method described in Ref. 135 use lmp2dens=off.
The use of lmp2dens=on is recommended since in this case the local CC energy can be corrected by the difference of the local MP2 energy and the approximate local MP2 energy calculated in the local interacting subspaces (see Total CC… energy + correction in the output). This correction usually improves the local CC energy.
lmp2dens=on
to use the canonical expressions give lmp2dens=off
Threshold for the occupation numbers of occupied local natural orbitals (LNOs) in the case of local correlation calculations, or for state-averaged MP2/CIS(D) occupied natural orbitals for reduced-cost excited-state calculations, see also keyword lnoepsv. See Ref. 138 as well as Refs. 96 and for more details.
Orbitals with occupation numbers greater than 1-lnoepso will be frozen.
For default settings with options other than localcc=2018 and lcorthr=Normal, see the description of lcorthr.
lnoepso=1e-5 for local correlation, lnoepso=0 for excited-states
to set a threshold of $5\cdot 10^{-6}$ type lnoepso=5e-6
Threshold for the occupation numbers of virtual local natural orbitals (LNOs) in the case of local correlation calculations, or for state-averaged MP2/CIS(D) virtual natural orbitals for reduced-cost excited-state calculations, see also keyword lnoepso. See Ref. 138 as well as Refs. 96 and for more details.
Orbitals with occupation numbers smaller than this number will be dropped.
For default settings with options other than localcc=2018 and lcorthr=Normal, see the description of lcorthr.
lnoepsv=1e-6 for local correlation, lnoepsv=7.5e-5 for excited-states
to set a threshold of $5\cdot 10^{-7}$ type lnoepsv=5e-7
Specifies if local correlation calculation is performed. See Refs. 135, 138, 85, 105, 104, and 106 for more details.
Local correlation methods can also be run if the prefix “L” (or “LNO-” in the case of CC methods) is added to the corresponding option of keyword calc, see the description of calc. Local SCS-MP2 (SOS-MP2) calculations can be run with calc=LSCS-MP2 (calc=LSOS-MP2).
localcc=off
for local correlation calculations give localcc=on
Maximum number of inactive labels. One can impose restrictions on the cluster operator using this keyword. The maximum number of virtual/occupied inactive labels on the singly, doubly, … excited clusters can be specified.
on or off. If maxact=on, the maximum number of virtual and occupied inactive labels must be specified in the subsequent line as an integer vector. The integers must be separated by spaces. The vector should contain as many elements as the excitation rank of the highest excitation in the cluster operator. The integers are maximum number of virtual/occupied inactive labels allowed on amplitudes of single, double, … excitations, respectively.
maxact=off
Suppose that we have up to quadruple excitations,
and the single, double, triple, and quadruple excitations are allowed to
have maximum of 1, 2, 2, and 1 inactive virtual and occupied labels,
respectively. Then the input file should include the following lines:
maxact=on
1 2 2 1
Maximum number of trial vectors in the Davidson procedure in the case of CIS, TDA, TD-HF, and TD-DFT calculations. The procedure will be restarted if the dimension of the reduced subspace reaches maxdim.
$<$any positive integer$>$
maxdim=max(100, 3*max(ntrip, nsing))
for a maximum of 50 expansion vectors set maxdim=50
Level of highest excitation included in the cluster operator in the case of MRCI/CC calculations. In an MR calculation all single, double (or higher) excitations out of the reference determinants are included in the cluster operator (see the description of keyword nacto), however, the very high excitations are frequently irrelevant. Using this option the latter can be dropped. If maxex is set to a positive integer $n$, only up to $n$-fold excitations will be included in the cluster operator. The excitation manifold can be further selected by imposing constrains on the number of active/inactive labels of the excitations (see keyword maxact). See Refs. 83 and 74 for more details.
The excitation manifold is not truncated.
The excitation manifold is truncated at $n$-fold excitations, see above.
maxex=0
to truncate the excitation manifold at triple excitations set maxex=3
Specifies the core memory used.
The amount of memory to allocate is specified in megabytes
The amount of memory to allocate is specified in gigabytes
mem=256MB
to allocate 8 GB core memory the user should set mem=8GB
Specifies whether input file for the Molden program and an xyz-file containing the Cartesian coordinates are written (see also Sect. 14).
Cartesian coordinates, basis set information, and MO coefficients are saved to file MOLDEN. This file can be opened by Molden and used to visualize the structure of the molecule and the MOs. In addition, Cartesian coordinates are also written to file COORD.xyz in xyz (XMol) format, which can be processed by many molecular visualization programs.
The construction of the MOLDEN input and the COORD.xyz file is turned off.
molden=on
if you do not need Molden input and the COORD.xyz file, add molden=off
Specifies the multipole approximation used for the evaluation of pair energies of distant pairs.
The simplified dipole-dipole estimate of Ref. 134 will be used.
Full dipole-dipole estimate [128].
All the terms are included in the multipole expansion up to the contributions of the quadrupole moment [105].
All the terms are included in the multipole expansion up to the contributions of the octapole moment [105].
mulmet=3 if localcc=2016 or 2018,
mulmet=0 otherwise
to use the octapole approximation set mulmet=3
Spin multiplicity ($2S+1$) of the Hartree–Fock or Kohn–Sham wave function. If a CI or CC calculation is also performed, the same multiplicity is supposed for the ground-state wave function. For excited states the multiplicity will be arbitrary, only $M_{S}$ is conserved. For closed-shell reference determinants the multiplicity (strictly speaking the parity of $S$) can be controlled by keywords nsing and ntrip, see below.
$<$any positive integer$>$
for atoms the corresponding experimental multiplicity is set, for molecules mult=1 (singlet) for an even number of electrons, mult=2 (doublet) otherwise
for a triplet state one should give mult=3
Number of active occupied spinorbitals. By default, nacto pieces of spinorbitals under the Fermi level are supposed to be active. This can be overwritten using keyword active, which enables the user to select the active orbitals manually (see the description of keyword active). In a MRCI/CC calculation a complete active space (CAS) is supposed defined by keywords nacto and nactv (or alternatively by active) and up to $n$-fold excitations from the reference determinants of this space are included in the excitation manifold, where $n$ is determined by keyword calc (2 for CCSD, 3 for CCSDT, …). See Ref. 83 for more details. See also keywords nactv, maxex, and maxact.
$<$any positive integer$>$ or 0
nacto=0
for two active occupied spin-orbitals give nacto=2
Number of active virtual spinorbitals. By default, nactv pieces of spinorbitals above the Fermi level are supposed to be active, which can be overwritten using keyword active. For a detailed description see keyword nacto.
$<$any positive integer$>$ or 0
nactv=0
for two active virtual spin-orbitals give nactv=2
Specifies how natural auxiliary functions (NAFs) will be constructed in the case spin-unrestricted MOs. NAFs can be calculated by diagonalizing ($\mathbf{W}^{\alpha}$ $+$ $\mathbf{W}^{\beta}$)/2 or $\mathbf{W}^{\alpha}$ (see Ref. 84 for the definitions). The latter option is somewhat more efficient but can be dangerous for processes involving atoms.
NAFs are constructed from ($\mathbf{W}^{\alpha}$ $+$ $\mathbf{W}^{\beta}$)/2.
NAFs are constructed from $\mathbf{W}^{\alpha}$.
nafalg=albe
to use $\mathbf{W}^{\alpha}$ set nafalg=alpha
Specifies whether natural auxiliary functions (NAFs) will be used for density-fitting correlated calculations and also specifies the threshold for the occupation numbers of NAFs (see Ref. 84).
NAFs will not be constructed.
A NAF basis will be constructed and NAFs with occupation numbers smaller than this number will be dropped.
Equivalent to naf_cor=1e-2 for local correlation methods, and to naf_cor=5e-3 otherwise.
according to the value of lcorthr for local correlation methods, naf_cor=0.1 for the reduced-cost excited-state approaches of Refs. 96 and (see keyword redcost_exc), naf_cor=off otherwise.
to use NAFs and set a threshold of $10^{-2}$ type naf_cor=1e-2
Specifies whether NAFs will be used for density-fitting SCF calculations and also specifies the threshold for the occupation numbers of NAFs (see Ref. 84). The syntax is analogous with that for keyword naf_cor.
Specifies how NAFs will be constructed in the case of local correlation calculations. NAFs are constructed by diagonalizing the $\mathbf{W}=\mathbf{J}^{\mathrm{T}}\mathbf{J}$ matrix where $\mathbf{J}$ is a particular block of the three-center Coulomb integral matrix (see Refs. 84 and 106 for details).
NAFs are constructed from $J^{P}_{ai}$
NAFs are constructed from $J^{P}_{pi}$
NAFs are constructed from $J^{P}_{pq}$
NAFs are constructed from $J^{P}_{\mu i}$
naftyp=Jpq for local CC and localcc=2016 or 2018 as well as for the reduced-cost excited-state approaches of Refs. 96 and (see keyword redcost_exc), naftyp=Jai for local MP2 and localcc=2016 or 2018
to construct NAFs using $J^{P}_{pq}$ set naftyp=Jpq
Number of Cholesky vectors/quadrature points for the Laplace integral in the case methods based on the decomposition of energy denominators. See also the description of keyword dendec.
The number of Cholesky vectors/quadrature points will be automatically determined to achieve the required precision.
The number of Cholesky vectors/quadrature points will also be automatically determined but the maximum number of the vectors cannot exceed this number.
nchol=auto
to use ten Cholesky vectors/quadrature points give nchol=10
Step size for the numerical differentiation in atomic units.
$<$any positive real number$>$
ndeps=1e-3
for a step size of $5\cdot 10^{-4}$ a.u. for numerical Hessian evaluation set ndeps=5e-4
Number of electronic states including the ground state and excited states. In non-relativistic calculations, for closed-shell reference determinants nstate is supposed to be the number of singlet states. See also keywords nsing and ntrip.
$<$any positive integer$>$
nstate=max(1, nsing+ntrip)
for three states give nstate=3
Number of singlet electronic states (strictly speaking the number of of states with $M_{S}=0$ and $S$ is even) including the ground state and excited states. Use this option only for non-relativistic calculations and closed-shell reference determinants, it should be zero otherwise. In the case of closed-shell reference determinants a partial spin-adaptation is possible, see Ref. 82. This enables us to search for singlet and triplet roots separately. See also keywords nstate and ntrip.
$<$any positive integer$>$
nsing=1 for closed-shell reference determinants, nsing=0 otherwise
for two singlet states give nsing=2
Number of triplet electronic states (strictly speaking the number of of states with $M_{S}=0$ and $S$ is odd) including the ground state and excited states. Use this option only for non-relativistic calculations and closed-shell reference determinants, it should be zero otherwise. See the description of keywords nstate and ntrip.
$<$any positive integer$>$
ntrip=0
for two triplet states give ntrip=2
Specifies the occupation of the Hartree–Fock determinant.
If this keyword is not given, the occupation is automatically determined in the SCF calculations.
For RHF calculations the occupation should be given in the following
format:
occ=$<n_{1}>,<n_{2}>,\dots,<n_{N_{ir}}>$
where $<n_{i}>$ is the number of occupied orbitals in irrep $i$, and
$N_{ir}$ is the number of irreps.
For ROHF and UHF calculations the occupation should be given as
occ=$<n^{\alpha}_{1}>,\dots,<n^{\alpha}_{N_{ir}}>$/$<n^{\beta}_{1}>,\dots,<n^{\beta}_{N_{ir}}>$
where $<n^{\sigma}_{i}>$ is the number of occupied $\sigma$ spinorbitals in irrep $i$.
occ is not specified, that is, the occupation is set by the SCF program.
Water, RHF calculation:
occ=3,1,1,0
Water, UHF calculation:
occ=3,1,1,0/3,1,1,0
Carbon atom, ROHF or UHF calculation:
occ=2,0,0,0,0,1,0,1/2,0,0,0,0,0,0,0
Specifies the optimization algorithm used for geometry and basis set optimizations. For basis set optimization, at the moment, the downhill simplex method of Nelder and Mead [108] is the only available option. A geometry optimization can be carried out by either the Broyden–Fletcher–Goldfarb–Shanno (BFGS) or the simplex algorithm.
the simplex method of Nelder and Mead.
the BFGS algorithm.
optalg=simplex for basis set optimization, optalg=BFGS otherwise.
To run a geometry optimization with the simplex algorithm set optalg=simplex
Maximum number of iteration steps allowed in a geometry or basis set optimization. If the simplex algorithm is used, i.e., optalg=simplex, the maximum number of function evaluations is also controlled by the parameter optmaxit: it is set to 15$\times$optmaxit. If the optimization is terminated with a message “the maximum number of function evaluation is exceeded”, then you can increase the value of optmaxit appropriately.
$<$any positive integer$>$
optmaxit=50
to allow 60 iteration steps set optmaxit=60
Convergence threshold for geometry or basis set optimization. If the simplex algorithm is used, i.e., optalg=simplex, the optimization is terminated when the energy difference (in E${}_{h}$) becomes less then this value and the optstol criterion is also fulfilled. In addition to the criterion for the gradient (optgtol) and the step-size (optstol) the energy change between the cycles is also monitored. For a successful geometry optimization it is required that the optgtol criterion is satisfied and either the energy difference between the last two steps becomes less than this value (in E${}_{h}$) or the optstol criterion is met.
$<$any positive real number$>$
optetol=1e-6
for a convergence threshold of $5\cdot 10^{-6}$ E${}_{h}$ set optetol=5e-6
Convergence threshold for geometry optimization, upper limit (in E${}_{h}$/bohr) for the maximum gradient component. For a successful geometry optimization this criterion must be fulfilled.
$<$any positive real number$>$
optgtol=1e-4
for a convergence threshold of $3\cdot 10^{-4}$ E${}_{h}$/bohr set optgtol=3e-4
Convergence threshold for geometry or basis set optimization. For the latter the optimization is terminated when the maximum change in the parameters becomes less then this value and the optetol criterion is also fulfilled, for the former this criterion is met when the maximum step-size from the previous step (in bohr) is lower than this value. The geometry optimization is terminated successfully if, in addition to the optgtol criterion obeyed, either this criterion is met or the energy difference between the last two steps becomes less than optetol.
$<$any positive real number$>$
optstol=1e-3 for a basis set optimization, optstol=1e-4 otherwise.
to set a threshold of $10^{-5}$ bohr for a geometry optimization type optstol=1e-5
Specifies what type of orbital localization is performed for the core molecular orbitals.
All the options introduced for keyword orbloco also work for orblocc, see the description of keyword orbloco for details.
orblocc=orbloco if localcc=2013, or core=corr and
localcc$\neq$off;
orblocc=off otherwise
to localize of core orbitals with the Pipek–Mezey algorithm specify orblocc=on
Initial guess for the orbital localization.
Guess orbitals are calculated by the Cholesky decomposition of the one-particle density matrix [5].
Guess orbitals for the localization are read from
the
MOCOEF.LOC file produced in a previous run where orbital
localization was performed.
Orbitals are read from the MOCOEF.LOC file and directly employed at later steps of the calculation without any change. The locality of the orbitals is not checked and the orbital localization is skipped entirely.
The combination of orblocguess=restart (or orblocguess=read) with scfiguess=off can be particularly useful if the result files of the converged SCF iteration and orbital localization steps are available and only the local correlation step should be repeated with different settings. See also the description of scfiguess=off for this option.
orblocguess=cholesky
to speed up the orbital localization by using the localized orbitals of a previous calculation as guess specify orblocguess=restart.
Specifies what type of orbital localization is performed for occupied molecular orbitals.
orbloco=off in the general case, orbloco=boys for local correlation calculations
to carry out Pipek–Mezey localization for the occupied orbitals type orbloco=pm
Specifies what type of orbital localization is performed for virtual molecular orbitals.
All the options introduced for keyword orbloco excepting IBO also work for orblocv, see the description of keyword orbloco for details. In addition, for local correlation calculations there is one more option:
Projected atomic orbitals.
orblocv=off in the general case, orblocv=pao for local correlation calculations
to carry out Boys localization for the virtual orbitals type orblocv=boys
Threshold for the occupation numbers of orbital specific virtual orbitals (OSVs) used at the evaluation of pair correlation energies in local MP2 and dRPA calculations. See the description of keyword wpairtol for more details.
OSVs are not constructed and not dropped
Orbitals with occupation numbers smaller than this number will be dropped.
osveps=1e-3 for localcc=2015, osveps=off for localcc=2016 or 2018
to set a threshold of $10^{-4}$ type osveps=1e-4
This keyword controls the cost reduction approaches based on natural orbital (NO) or optimized virtual orbitals (OVOs) techniques. For a ground-state correlation calculation, if this keyword is set, the virtual MOs will be transformed to MP2 NOs or OVOs [109]. Subsequently the virtual space will be truncated on the basis of the populations of the orbitals, which can be controlled by keywords eps and ovosnorb. See Ref. 136 for more details.
The virtual MOs are not changed.
MP2 NOs will be used.
Optimized virtual orbitals will be used.
ovirt=off
to use MP2 NOs for a ground-state CC calculation give ovirt=MP2
Tolerance for the eigenvalues of the AO overlap matrix. Eigenvectors corresponding to the eigenvalues lower that ovltol will be removed to cure the linear dependence of the AO basis set.
This number will be used as the threshold for the eigenvalues of the overlap matrix.
ovltol=1e-7
to keep all the basis functions set ovltol=0.0
Specifies the retained percentage of virtual orbitals in an optimized virtual orbitals (OVOs) calculations. ovosnorb % of virtual orbitals will be retained.
$<$any number between 0 and 100$>$
ovosnorb=80.0
to retain only 70 % of the virtuals give ovosnorb=70.0
This keyword controls the wave function analysis.
No wave function analysis is performed.
In addition to the above parameters, intrinsic atomic orbitals (IAOs) are constructed and IAO partial charges are calculated [68].
popul=Mulli if dens $\neq$ 0, popul=off otherwise
to calculate IAO charges set popul=IAO
The pressure in Pa at which the thermodynamic properties are evaluated (see also keyword freq).
$<$any positive integer$>$
pressure=100000
for 1 atm set pressure=101325
This keyword tells Mrcc that a QM/MM calculation is performed and the point charges included in the input file must be processed. This keyword is automatically added to the MINP file by the MM program conducting the QM/MM calculations, and you do need to bother with it. Use this keyword in the only case if you want to add point charges manually.
QM/MM calculation is not performed and no point charges are added.
Currently this is the only option, the Amber MD code will be used for the QM/MM calculation or point charges will be added.
Point charges can be manually added to the end of the
input file in the following format:
pointcharges
$<$number of point charges$>$
$<x_{1}>$ $<y_{1}>$ $<z_{1}>$ $<q_{1}>$
$<x_{2}>$ $<y_{2}>$ $<z_{2}>$ $<q_{2}>$
⋮
where $x_{i}$, $y_{i}$, and $z_{i}$ are the Cartesian coordinates and $q_{i}$
is the charge for point charge $i$. The charge must be given in a.u.,
while for the coordinates the same unit must be used as for the
specification of the molecular geometry.
qmmm=off
to add two point charges with coordinates
(0, 0, 1) and (0, 1, 0) a.u. (provided that the geometry is also given
in bohr) and charges of 0.5 and -0.5 a.u. qmmm=Amber should be
set anywhere in the MINP file, and the following lines should be
added to the end the file:
pointcharges
2
0.0 0.0 1.0 0.5
0.0 1.0 0.0 -0.5
Use this option to carry out quadratic SCF calculations. One can use either Newton or trust region iterations with optional line search.
No quadratic SCF, conventional SCF algorithm will be executed.
Simple Newton iteration.
Simple Newton iteration with line search.
Trust region method with augmented Hessian algorithm without line search. The trust radius is updated according to the scheme described in Ref. 55.
Trust region method with augmented Hessian algorithm using line search. The trust radius update scheme is similar to the above one but uses different coefficients.
Trust region method with augmented Hessian algorithm using line search. The trust radius is updated as described in Ref. 55, but this method takes into account the step length found by the line search.
Trust region method with augmented Hessian algorithm using line search. The trust radius update scheme takes into account the change of the gradient in the consecutive iterations.
The simple Newton iteration schemes are only efficient in the vicinity of a minimum and not recommended in the general case. We recommend the use of the AugHessG or AugHessL options in difficult cases.
qscf=off
UKS calculation with the B3LYP functional using the
AugHessG algorithm:
calc=B3LYP
scftype=UHF
qscf=AugHessG
This keyword controls the cost reduction approaches based on natural orbital (NO) and natural auxiliary function (NAF) techniques for excited states. For a CIS(D${}_{\infty}$), ADC(2), and CC2 calculation, if redcost_exc$\neq$off, the reduced-cost approach of Refs. 96 and is invoked, and truncated state-averaged MP2/CIS(D) NOs as well as NAFs will be used. The lnoepso, lnoepsv, naf_cor, and naftyp keywords will be automatically set depending on the selected option for redcost_exc. For CIS, TD-HF, TDA, TD-DFT calculations the NAF approximation will be invoked if redcost_exc=8.
The cost reductions techniques will not be used.
Reduced-cost calculation will be executed with default settings (see also Table 4).
Reduced-cost calculation will be executed with
customized truncation thresholds. The threshold for the complete MO
space NAFs (CS-NAFs), CIS coefficients, orbital energies, and
linear dependency must be specified in the subsequent line,
respectively, as
$<$threshold 1$>$ $<$threshold 2$>$ $<$threshold 3$>$
$<$threshold 4$>$
The default values of these thresholds are 0.1 a.u., 0.35, 0.15 a.u.,
$10^{-7}$, respectively. These are used with if any other option is
chosen. See Ref. for the detailed description of
these parameters.
See Table 4.
redcost_exc=off
Reduced-cost ADC(2) calculation for the lowest
singlet excited state with the
default settings proposed in Ref. :
calc=ADC(2)
nsing=2
redcost_exc=on
Reduced-cost TD-DFT calculation with the PBE0 functional for the lowest
3 singlet excited states of a molecule:
calc=PBE0
redcost_exc=8
nstate=4
Option | CS-NAF | NO | Can. | RS-NAF | Note |
off | no | no | no | no | Default |
on | yes/no | yes | yes | yes | Equivalent to 1 or 6 depending on keyword localcc |
cust | yes | yes | yes | yes | Customized thresholds |
1 | yes | yes | yes | yes | The approach presented in Ref. , default if localcc=off and redcost_exc=on |
2 | no | yes | no | yes | The approach presented in Ref. 96 |
3 | no | no | no | yes | The approach presented in Ref. 96 without NOs |
4 | no | yes | no | no | The approach presented in Ref. 96 without NAFs |
5 | no | yes | yes | no | |
6 | no | yes | yes | yes | Default if localcc=2016 and redcost_exc=on |
7 | yes | yes | no | yes | |
8 | yes | no | no | no | For reduced-cost CIS, TD-HF, TDA, TD-DFT, … |
9 | yes | yes | yes | no | |
10 | yes | yes | no | no |
The reference determinant (Fermi-vacuum) for CI/CC calculations can be specified using this keyword. By default the reference determinant is identical to the HF determinant, but sometimes it is necessary to change this.
The reference determinant is identical to the HF determinant.
Using this option one can define the occupation of the correlated orbitals in the reference determinant specifying their serial numbers. This option requires three more lines. In the first line the serial numbers of the doubly-occupied orbitals must be given, while in the second and third lines those orbitals should be specified which are singly-occupied by an alpha or a beta electron, respectively. For the format of these lines see the description of the serialno option of the active keyword. For relativistic calculations the occupation of the spinors (i.e., not that of the Kramers-pairs) should be given. For technical reasons all electrons are treated as alpha electrons and the serial numbers of the occupied spinors must be given in the second line, the first and third lines must be left blank.
Using this option one can set the occupation numbers for each correlated orbital. In the subsequent line an integer vector should be supplied with as many elements as the number of correlated orbitals (correlated spinors for relativistic calculations, not Kramers-pairs!). The integers must be separated by spaces. In the case of non-relativistic calculations type 2 for doubly-occupied orbitals, 1 for open-shell orbitals with alpha electron, -1 for open-shell orbitals with beta electron, 0 otherwise. In the case of relativistic calculations type 1 for each occupied spinor, 0 otherwise.
Frozen orbitals must not be considered here in any case.
If the MO integrals are taken over from another program, the numbering of orbitals may be different from that of the parent program. Here the order of MOs: doubly occupied, open shell, virtual; and in each of this blocks the MOs are reordered according to the orbital energies (natural orbital occupations in the case of MCSCF orbitals).
If the MO integrals are taken over from another program, and this line is omitted, the program will fill the orbitals with electrons from the bottom automatically. In this manner we do not need this line for closed shells or a doublet ref. det., but e.g. for high spin states the Fermi vacuum must be defined here.
For relativistic calculations (Dirac interface) this line is always required. The spinors are symmetry-blocked according to the Fermion irreps of the corresponding double group. Complex conjugate irreps follow each other. Within each irrep the spinors are numbered according to orbital energies. Please note that this line is automatically printed by the dirac_mointegral_export program, and you do not have to do it by hand. However, for technical reasons, always a closed-shell occupation is generated, and you may need to remove or add some electrons.
refdet=none, that is, the reference determinant is identical to the HF determinant.
We have 20 correlated orbitals, 10 electrons, and we are
interested in a high-spin triplet state. Suppose that orbitals 1 to 4
are doubly-occupied while orbitals 5 and 6 are singly occupied by alpha
electrons. Using the serialno option the input should include the
following four lines (note the blank line at the end):
refdet=serialno
1-4
5,6
The same using the vector option:
refdet=vector
2 2 2 2 1 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0
We perform a relativistic calculation for the Be atom with
20 correlated spinors. We have 6, 6, 4, and 4 spinors in the four
Fermion
irreps, E${}_{1/2g}$, E${}_{-1/2g}$, E${}_{1/2u}$, and E${}_{-1/2u}$ of the
$C_{2h}^{*}$ double group, respectively, and two occupied spinors in both
of the gerade irreps. Thus using the vector option the occupation
vector should be given as:
refdet=vector
1 1 0 0 0 0 1 1 0 0 0 0 0 0 0 0 0 0 0 0
The same using the serialno option (note the blank
lines):
refdet=serialno
1,2,7,8
Use this keyword to restart canonical (i.e., not local) CI and CC calculations from previously calculated wave function parameters (cluster amplitudes, CI coefficients, $\lambda$ amplitudes, etc.) if ccprog=mrcc. For restarting local correlation calculations see keyword lccrest.
The program restarts from the previously calculated parameters.
The program executes automatically the lower-level calculations of the same type consecutively (e.g., CCSD, CCSDT, and CCSDTQ if CCSDTQ is requested) and restarts each calculation from the previous one (this is only available for energy calculations).
Same as rest=1, however, only selected roots from
the previous calculation will be used as initial guess. The serial
number of the roots must be specified in the subsequent line as
$<n_{1}><n_{2}><n_{3}>\dots$
where $<n_{i}>$ is the serial number of the states. The number of states
given here must be equal to nstate or nsing + ntrip.
Please note that the ground state solution is not automatically
selected, it should also be given here if needed. It is recommended to
use root following (diag=follow) together with this option.
Same as rest=2 but the initial vectors are selected as in the case of rest=3.
use the restart option, e.g.,
after system crash.
if the iteration procedure did not converge in the given number of steps.
for geometry optimization.
for potential curve calculations.
if you are interested in high-order CC/CI energies. Then it is worth restarting the calculations with higher excitations using the converged vectors of the same method including lower excitations, e.g., CCSDT using the converged CCSD amplitudes, CCSDTQ using the CCSDT amplitudes, and so on. With this trick 1-3 iteration steps can be saved usually, but more ones in the case of strong static correlation (i.e., large cluster amplitudes). Use exclusively rest=2 for this purpose (that is, not rest=1)!
if you are interested in calculating the energies for all methods in a hierarchy (e.g., executing all CC methods up to CCSDTQP). Use exclusively rest=2 for this purpose (that is, not rest=1)!
to generate brute-force initial guess for excited-state calculations (rest=3 or 4). That is, if you do not want to bother with the initial guess for excited states, but you know approximately the energy of the excited states, then execute a low-level method for many roots. Use LR-CCS (calc=CCS) and CIS (calc=CIS), respectively, for higher-order LR-CC and CI calculations. Select the desired roots on the basis of their energies, and use them as initial guess in high-level calculations. (For other options for the initial guess for excited-state calculations see keyword ciguess.)
Please note that the program always needs the file fort.16 from the previous calculation for the restart and also fort.17, if more than one root is sought or for geometry optimization.
rest=0
to restart a CC calculation after power failure set rest=1
to restart a LR-CCSD calculation using the
first, third, and fifth roots of a previous LR-CCS calculation the input
should include the following two lines:
rest=3
1 3 5
Specifies the radial integration grid for DFT calculations. For the details of the grid construction see the description of keyword agrid. See also the description of keyword grtol.
the number of grid points is calculated by the max{20,5*(3*grtol/2+$i$-8)} formula with $i$ as the number of the row in the periodic table where the atom is located [72]. To change the number of radial integration points set the value of grtol.
rgrid=Log3
to use the Euler–Maclaurin scheme set rgrid=EM
to use the default Log3 grid with more points set grtol=12
Specifies the type of the ROHF orbitals. See also the description of keyword scftype.
Standard ROHF orbitals obtained by diagonalizing the ROHF Fock-matrix.
Semicanonical ROHF orbitals obtained by separately diagonalizing the alpha and beta UHF Fock-matrices constructed using the converged ROHF orbitals.
rohftype=semicanonical is required for perturbative CC methods if ROHF orbitals are used, otherwise the expressions for the perturbative corrections are not correct. Iterative CC and CI methods are invariant to the choice of ROHF orbitals (if all electrons are correlated).
It is very important to give this keyword if Mrcc is used together with another code and ROHF orbitals are used since this keyword tells Mrcc what type of ROHF orbitals are taken over from the other code.
rohftype=standard for iterative CC and CI
methods,
rohftype=semicanonical for perturbative methods.
to use semicanonical ROHF orbitals for iterative CC methods give rohftype=semicanonical
Specifies what type of SCF algorithm is to be used.
Conventional SCF algorithm, two-electron integrals are stored on disk.
Direct SCF algorithm, two-electron integrals are recalculated in each iteration step.
Based on the size and geometry of the molecule the program will automatically select the more efficient one from the above options.
scfalg=auto
to run direct SCF add scfalg=direct
Specifies whether damping of the SCF density matrices is performed.
No damping.
In each SCF iteration cycle the new and old SCF density matrices are mixed by factors (1-scfdamp) and scfdamp, respectively.
Equivalent to scfdamp=0.7
scfdamp=off
to use a damping factor of $0.8$ type scfdamp=0.8
Specifies if DIIS convergence acceleration is used in the SCF calculations.
on or off
scfdiis=on
to turn off DIIS convergence accelerator add scfdiis=off
Specifies the last iteration step in which the DIIS convergence acceleration is applied.
$<$any positive integer$>$
scfdiis_end=scfmaxit, that is, the DIIS procedure is not turned off.
to turn off the DIIS convergence accelerator after iteration step 20 give scfdiis_end=20
Specifies the first iteration step in which the DIIS convergence acceleration is applied.
$<$any positive integer$>$
scfdiis_start=1, that is, the DIIS procedure is active from the first iteration.
to turn on the DIIS convergence accelerator in iteration step 5 give scfdiis_start=5
Specifies the frequency of DIIS extrapolations. The extrapolation will be carried out in every scfdiis_step’th iteration cycle.
$<$any positive integer$>$
scfdiis_step=1, that is, the DIIS extrapolation is performed in each iteration step.
to carry out DIIS extrapolation only in every second iteration step give scfdiis_step=2
Convergence threshold for the density matrix in SCF calculations. The RMS change in the density matrix will be smaller than $10^{-{\tt scfdtol}}$.
$<$any integer$>$
scfdtol=scftol+2 for frequency calculations,
otherwise
scfdtol=scftol+1 for correlation calculations,
scfdtol=scftol for SCF calculations
for an accuracy of $10^{-8}$ one must give scfdtol=8
Specifies the number of Fock-matrices used for the DIIS extrapolation in SCF calculations.
$<$any positive integer$>$
scfext=10
to increase the number of DIIS vectors to 15 give scfext=15
Initial guess for the SCF calculation.
Superpositions of atomic densities. For each atom a density-fitting UHF calculation is performed, and the initial one-particle density matrix is constructed from the averaged alpha and beta atomic densities.
Atomic density initial guess. The initial one-particle density matrix is constructed from diagonal atomic densities derived from the occupation of the atoms. It is efficient for Dunning’s basis sets.
Core Hamiltonian initial guess. The initial MOs are obtained by diagonalizing the one-electron integral matrix.
The SCF calculation will use the MO coefficients obtained in a previous calculation and stored in the MOCOEF file. The calculation can only be restarted from the MOs computed with the same basis set.
The SCF calculation will use the density matrices obtained in a previous calculation and stored in the SCFDENSITIES file. If the calculation is restarted from the densities obtained with another basis set, the VARS file is also required.
No SCF calculation will be performed, but the Fock-matrix and the MO coefficients obtained in a previous calculation will be used in the correlation calculations. This requires the FOCK, MOCOEF, and VARS files from the previous calculation.
A density fitting SCF calculation will be performed using the cc-pVTZ-min minimal basis set (see the description of keyword basis), and the resulting density will be used as initial guess. In the minimal-basis SCF calculation the AO basis set is used as the auxiliary basis, and loose convergence thresholds are employed, consequently, the energy is unreliable and should not be used for any purpose.
A density fitting SCF calculation will be performed using a smaller basis set which must be specified by keyword basis_sm (see the description of keyword basis_sm), and the resulting density will be used as initial guess.
Restarting from densities obtained with a bigger basis set is not allowed.
To restart SCF runs from the results of DFT embedding calculations with the Huzinaga-equation- or projector-based approaches use MO coefficients, i.e., scfiguess=mo, since only the subsystem densities are stored at the end of the embedding calculation but the MOs are available for the entire system.
scfiguess=sad
For a core Hamiltonian initial guess set scfiguess=core
For restarting the SCF calculation from the results of a calculation performed with the same basis set type scfiguess=restart. Note that you need the SCFDENSITIES file from the previous run.
You would like to generate a good initial guess for an aug-cc-pVTZ SCF
calculation. First, run a calculation with the cc-pVTZ basis set
(cc-pVTZ-min is also a good option), that is, your input file should
contain the
basis=cc-pVTZ
line. Then, restart your aug-cc-pVTZ calculation from the cc-pVTZ
density matrix. To that end the MINP file should include the
following lines:
basis=aug-cc-pVTZ
scfiguess=restart
Note that the SCFDENSITIES and the VARS files from the
cc-pVTZ run must be copied to the directory where the aug-cc-pVTZ
calculation is executed.
The calculations in the previous example can be run more
simply, in one step using the small option and the
basis_sm keyword as
basis=aug-cc-pVTZ
basis_sm=cc-pVTZ
scfiguess=small
Level shift parameter for the SCF calculation.
No level shifting.
The value of the level shift parameter in a.u.
Equivalent to scflshift=0.2
scflshift=off
To use a level shift value of 0.5 a.u. give scflshift=0.5
Maximum number of iteration steps in SCF calculations.
$<$any positive integer$>$
scfmaxit=50
to increase the maximum number of SCF iterations to 200 give scfmaxit=200
Convergence threshold for the energy in SCF calculations. The energy will be accurate to $10^{-{\tt scftol}}$ E${}_{h}$.
$<$any integer$>$
scftol=max(8,cctol) for property
calculations,
scftol=max(6,cctol) otherwise
for an accuracy of $10^{-8}$ E${}_{h}$ one must give scftol=8
Specifies the type of the Hartree–Fock/Kohn–Sham SCF procedure, or the type of the molecular orbitals if the MO integrals are computed by other programs. See also the description of keyword rohftype.
RHF, ROHF, UHF, or MCSCF
scftype=MCSCF is only available if Mrcc is used together with Columbus or Molpro. In that case the MCSCF calculation is performed by the aforementioned codes and the transformed MO integrals are passed over to Mrcc.
It is very important to give this keyword if Mrcc is used together with another code and ROHF or MCSCF orbitals are used since this keyword tells Mrcc that the orbitals are not canonical HF orbitals. Please also set keyword rohftype in this case.
If a HF-SCF calculation is run, the type of the SCF wave function can also be controlled by keyword calc. See the description of calc.
For DFT calculations only the RHF and UHF options can be used, which, in that case, instruct the code to run RKS or UKS calculations, respectively.
scftype=RHF for closed-shell systems, scftype=UHF for open shells.
to use ROHF for open-shell systems type scftype=ROHF
Scaling factor for the antiparallel-spin component of the correlation energy in spin-component scaled MP2 (SCS-MP2) calculations [46].
the antiparallel-spin component of the correlation energy will be scaled by this number.
scsps=6/5
to set a scaling factor of 1.5 type scsps=1.5
Scaling factor for the parallel-spin component of the correlation energy in spin-component scaled MP2 (SCS-MP2) calculations [46].
the parallel-spin component of the correlation energy will be scaled by this number.
scspt=1/3
to set a scaling factor of 0.5 type scspt=0.5
Threshold for the selection of strong pairs in local MP2, dRPA, and CC methods. For each orbital pair an estimate of the pair correlation energy is calculated (see the description of keyword wpairtol). An orbital pair will be considered as strong pair if the absolute value of the pair correlation energy estimate is greater than spairtol. In the subsequent calculations strong pairs will be treated at a higher level, while for the other pairs (weak and distant) the corresponding pair correlation energy estimates will be added to the correlation energy. See also Refs. 85 and 106 for more details.
the local MP2 or dRPA pair correlation energy estimate is not calculated, an orbital pair will be considered as strong pair in this case if the absolute value of the available pair correlation energy estimate is greater than wpairtol. See also the description of keyword wpairtol and Ref. 105.
Orbital pairs with pair correlation energy estimates greater than this number (in E${}_{h}$) will be considered as strong pairs.
spairtol=1e-4 for localcc=2015, spairtol=off for
localcc=2016 and localcc=2018
to set a threshold of $10^{-5}$ E${}_{h}$ type spairtol=1e-5
Spatial symmetry (irreducible representation) of the state. See Sect. 13 for the implemented point groups, conventions for irreps, etc.
Irreps can only be specified by their serial numbers if Mrcc is used with another program. In that case please check the manual or output of the other program system for the numbering of irreps.
by default the state symmetry is determined on the basis of the occupation of the HF determinant.
for the second irrep of the point group type symm=2
for the B${}_{1u}$ irrep of the $D_{2h}$ point group type symm=B1u
Specifies the algorithm for the calculation of the (T) correction in the case of the CCSD(T) method.
The outmost loops run over the occupied indices of the triples amplitudes.
The outmost loops run over the virtual indices of the triples amplitudes.
Laplace transformed (T) energy expression for localcc=2016 or 2018 according to Ref. 104. See also the laptol keyword to set the accuracy of the numerical Laplace transform.
The T0${}^{\prime}$ semi-canonical approximation of the local (T) expression according to Ref. 104.
talg=occ for conventional CCSD(T) calculations, talg=lapl for the local CCSD(T) scheme of localcc=2016 or 2018, and talg=virt for local CCSD(T) with localcc=2015 or 2013.
For algorithmic reasons in the case of previous local CCSD(T) schemes (localcc=2015 or 2013) talg=virt is the only option. For localcc=2016 or 2018, the default is talg=lapl, and talg=virt is used if lcorthr=0 is set.
For conventional CCSD(T) calculations talg=occ is recommended since the algorithm is somewhat faster than the other one. In turn, its memory requirement is higher. The program checks automatically if the available memory is sufficient for the first algorithm (i.e., talg=occ). If this is not the case, talg will be automatically set to virt.
In the case of localcc=2016 or 2018 the talg=topr algorithm is approximately three times faster than the talg=lapl with its default settings, but considerably less accurate. For quick exploratory calculations the talg=lapl algorithm is recommended in combination with laptol=0.1.
to change the default for a conventional CCSD(T) calculation set talg=virt
The temperature in K at which the thermodynamic properties are evaluated (see also keyword freq).
$<$any positive real number$>$
temp=298.15
for 300 K set temp=300.0
A keyword for testing Mrcc. If an energy value is specified using this keyword, it will be compared to the energy calculated last time [e.g., the CCSD(T) energy and not the CCSD or HF energy if calc=CCSD(T)] in the Mrcc run. An error message will be displayed and the program exits with an error code if the test energy and the calculated energy differ. This keyword is mainly used by the developers of the program to create test jobs to check the correctness of the computed energies. (See Sect. 8 for the further details.)
No testing.
The energy to be tested.
test=off
to set a test energy of -40.38235315 E${}_{h}$ type test=-40.38235315
Controls the printing of converged cluster amplitudes/CI coefficients if ccprog=mrcc.
No printing.
Cluster amplitudes/CI coefficients whose absolute value is greater than this number will be printed.
The value of the cluster amplitude/CI coefficient and the corresponding spin-orbital labels (serial number of the orbital + a or b for alpha or beta spin orbitals, respectively) will be printed. The numbering of the orbitals corresponds to increasing orbital energy order. Note that orbital energies are printed at the end of the SCF run if verbosity$\geq$3. You can also identify the orbitals using Molden (see Sect. 14.1).
tprint=off
to set a threshold of 0.01 give tprint=0.01
Uncontract contracted basis sets.
on or off
uncontract=off
to uncontract the basis set add uncontract=on
Specifies the units used for molecular geometries.
Ångströms will be used
Atomic units will be used
unit=angs
to use bohrs rather than ångströms the user should set unit=bohr
Controls the verbosity of the output.
0, 1, 2, 3. The verbosity of the output increases gradually with increasing value of the option. Error messages are not suppressed at any level.
verbosity=2
to increase the amount of information printed out
give
verbosity=3
Threshold for the selection of weak pairs in local MP2, RPA, and CC methods. For each orbital pair the estimate of the pair correlation energy is calculated with a multipole approximation [57, 134, 105]. An orbital pair will be considered as distant pair if the absolute value of the multipole-based pair correlation energy estimate is smaller than wpairtol. For the distant pairs the corresponding multipole-based pair correlation energy estimates will be added to the correlation energy, and distant pairs will be neglected in the subsequent calculations.
In the case of localcc=2015, for the remaining pairs a more accurate pair correlation energy estimate will be calculated using orbital specific virtuals (OSVs) controlled by keyword osveps, and these pairs will be further classified as weak and strong pairs controlled by keyword spairtol, see the description of keyword spairtol. The extended domain of an occupied orbital will include those orbitals for which the latter accurate pair correlation energy estimate is greater than spairtol. See also Ref. 85 for more details.
In the case of localcc=2016 or 2018, spairtol=off is set as default, and the extended domain of an occupied orbital will include those orbitals for which the multipole-based pair correlation energy is greater than wpairtol. See also Refs. 105 and 106 for more details.
Note that for local CC methods if spairtol$\neq$off is specified as a non-default option in the case of localcc=2016 or 2018, accurate MP2 pair energies are computed in the extended domains for the remaining non-distant pairs. Then the non-distant pairs are further divided into weak and strong categories according to the value of spairtol, as discussed above. In this case the MP2 pair energies of the weak pairs are added to the correlation energy, and new, somewhat smaller extended domains are constructed to proceed with the higher-level computation as above using solely the strong pair list. See also Ref. 106 for more details.
Orbital pairs with multipole-based pair correlation energy estimates smaller than this number (in E${}_{h}$) will be considered as distant pairs.
wpairtol=1e-5 for local MP2 and CC if localcc=2018,
wpairtol=min(1e-6, 0.01*spairtol)
for localcc=2015
For defaults with other than the above settings, see the description of lcorthr
to set a threshold of $5\cdot 10^{-6}$ E${}_{h}$ type wpairtol=5e-6