CASSCF Keyword
Last Update:
6/26/2001
DESCRIPTION
This method keyword requests a Complete Active Space
Multiconfiguration SCF (MC-SCF) [79-80,89-90,110,190]. An MC-SCF calculation is a combination of an SCF
computation with a full CI involving a subset of the orbitals; this subset is
known as the active space. The number of electrons (N) and the
number of orbitals (M) in the active space for a CASSCF must be
specified following the keyword:
CASSCF(N,M). Note that options
may be interspersed with N and M in any order.
By default, the active space is defined assuming that the
electrons come from the highest occupied orbitals in the initial guess
determinant and that the remaining orbitals required for the active space come
from the lowest virtuals of the initial guess. Thus, for a 4-electron,
6-orbital CAS--specified as CASSCF(4,6)--on a closed-shell system, the
active space would consist of:
Similarly, a 4 electron, 6 orbital CAS on a triplet would include
the highest 3 occupied orbitals (one of which is doubly occupied and two singly
occupied in the guess determinant) and the lowest 3 virtual orbitals. In
Gaussian 98, algorithmic improvements make an active space of up to
about 10 orbitals feasible [82-83]. Above 8 orbitals, the CASSCF code automatically
uses this new direct method for matrix elements.
Normally, Guess=Alter is necessary to ensure that the
orbitals which are selected involve the electrons of interest and that they are
correlated correctly. A prior run with Guess=Only can be used to quickly
determine the orbital symmetries (see the first example below). Alternatively,
a full Hartree-Fock single point calculation may be done, and the subsequent
job will include (Guess=Read,Alter) in order to retrieve and then modify
the computed initial guess from the checkpoint file. You need to include
Pop=Regular in the route section of the preliminary job in order to
include the orbital coefficient information in the output (use Pop=Full
for cases where you need to examine more than just the few lowest virtual
orbitals). You may also choose to view the orbitals in a visualization package.
By default, CASSCF calculations use a direct algorithm to avoid
disk storage of integrals. A conventional algorithm may be selected by
including SCF=Conven in the route section.
CAS is a synonym for CASSCF.
Use #P in the route section to include the final
eigenvalues and eigenvectors in addition to the energy and one-electron density
matrix in the CASSCF output.
A brief overview of the CASSCF method is given in chapter 9
(exercises 5 and 6) and appendix A of Exploring Chemistry with Electronic
Structure Methods304. See reference [90] for a detailed discussion on the choice of an
active space. See chapter 5 for a discussion of efficiency considerations for
CASSCF calculations.
Note: CASSCF is a powerful but advanced method with many
subtleties. We strongly recommend that you study the cited references before
attempting to run production CASSCF calculations (this is especially true for
CASSCF MP2). Example applications are discussed in references [191,192,193,194,195,196].
VARIATIONS
- An MP2-level electron correlation correction to the CASSCF
energy may be computed during a CASSCF calculation by specifying the MP2
keyword in addition to CASSCF within the route section [81].
-
Calculations on excited states of molecular systems may be
requested using the NRoot option. Note that a value of 1 specifies the
ground state, not the first excited state (in contrast to usage with the
CIS keyword).
-
State-averaged CASSCF calculations may be performed using the
StateAverage and NRoot options to specify the states to be used.
-
Conical intersections and avoided crossings may be computed
by including Opt=Conical in the route section of a CASSCF job (see the
examples) [105-106].
-
Approximate spin orbit coupling between two spin states can
be computed during CASSCF calculations by including the Spin option [145,146,147,148,149]. The method used in Gaussian 94 is based on
reference [149]. It is available for the elements H
through Cl.
In order to compute the spin orbit coupling, the integrals are
computed in a one-electron approximation involving relativistic terms, and then
effective charges are used that scale the Z value for each atom to empirically
account for 2 electron effects. Note that such calculations will be
state-averaged by default, using the state specified by the NRoot option
(or the ground state by default), and the next higher state.
OPTIONS
NRoot=j Requests that the jth root of the
CI be used, so that an excited state is obtained when
j > 1. The option defaults to the ground state
(j=1). The state specified by NRoot is referred to as the "state
of interest."
StateAverage Used to specify a state-averaged CASSCF
calculation. All states up to NRootare averaged. This option requires
the weighting for the various states to be input in format nF10.8 (no trailing
blank line). State Average is not allowed in combination with
Opt=Conical or CASSCF=Spin, both of which perform state-averaged
calculations by default.
Spin Compute approximate spin orbit coupling between
the state of interest (NRoot) and the next higher state. Implies a
state-averaged CASSCF calculation. Spin orbit coupling may be computed for the
elements H through Cl only.
OrbLocal[=n] Localize the first n
strongly-occupied orbitals (the default is to localize all active orbitals).
DavidsonDiag Requests the use of the Davidson
diagonalization method for the CI matrix instead of the Lanczos iterations.
Lanczos is the default for NRoot values of 1 or 2; otherwise, Davidson
is the default.
FullDiag Requests the use of the full (Jacobi)
diagonalization method for the CI matrix instead of Lanczos or Davidson
iterations. The default is full diagonalization if there are 6 or fewer active
orbitals. NoFullDiag suppresses the use of the full diagonalization
method.
The full Jacobi diagonalization method must be used if quadratic
converence is required (see the QC option below), and when one knows
nothing at all about the CI eigenvector (in the latter case, specify
FullDiag for calculations involving more than 6 active orbitals)
StateGuess=k Set the starting vector for the Lanczos
method to configuration k. For example, this option can be useful for
selecting a configuration of the correct symmetry for a desired excited state
(different from that of the ground state). In such cases, running a preliminary
calculation to determine the orbital symmetries may be required.
k may also be set to the special value Read, which
says to read in the entire eigenvector from the input stream (format:
NZ , (Ind(I), C(Ind(I)), I=1, NZ).
The default diagonalization method is most efficient if the size
of the CI problem is greater than about 50, or the user can identify one or
more dominant components in the eigenvector from the onset of the calculation,
via the initial trail vector. By default, the starting vector is initialized in
j+1 positions, where j is the value given to the NRoot
option (or its default value). The positions correspond to the lowest
j+1 energy diagonal elements of the CI Hamiltonian. This usually results in
good convergence for the lowest j roots.
The StateGuess option (below) may be used to change this
default. CASSCF(…,StateGuess=k) sets
C(k) to 1.0. The central requirement for this vector is that it not be
deficient in the eigenvector that is required. Thus, if the CI eigenvector is
dominated by configuration k, setting the StateGuess option to
k will generate a good starting vector (e.g. State Guess=1 is
appropriate if the Cl vector is dominated by the SCF wavefunction). However, if
the coefficient of configuration k is exactly zero (e.g., by symmetry)
in the desired root, then that eigenvector will be missing, and the calculation
will converge to a higher state.
OrbRot Includes and NoCPMCSCF excludes the
orbital rotation derivative contributions from the CP-MC-SCF equations in an
Opt=Conical calculation. OrbRot is the default.
SlaterDet Use Slater determinants in the CASSCF
calculation. This option is needed to locate a conical intersection between a
singlet state and a triplet state.
HWDet Use Hartree=Waller determinants instead of
Slater. This is the default for CAS calculations involving 10 or more orbitals.
It implies NoFullDiag.
RFO Requests the RFO quadratic step. At most, one of
QC and RFO should be specified; RFO is the default.
QC Requests a quadratically convergent algorithm for
the CAS. This option should be used with caution; it works well only with a
very good guess. Only one of QC and RFO should be specified;
RFO is the default.
UNO Requests that the initial orbitals for the CAS be
produced from the natural orbitals generated from a previous UHF calculation
[197-198]. Normally used
with Guess=Read.
The UNO guess must be used with caution. Often, some of the
natural orbitals which have modest occupation are not the important ones for
the process of interest. Consequently, unless the entire valence space is being
correlated (which is usually prohibitively expensive), one normally runs one
job which does a UHF calculation with Pop=NaturalOrbital, and then
examines the resulting orbitals. The orbitals which belong in the active space
are then selected, and a single-point CASSCF(…,UNO) Guess=(Read, Alter)
calculation is performed. The resulting converged orbitals are then
examined to verify that the correct active space has been located, and finally
an optimization can be run with CASSCF(…,UNO) Guess=Read. For
singlets, this entire process depends on the user being able to coax the UHF
wavefunction to converge to the appropriate broken spin-symmetry (non-RHF)
result.
NPairs=n Number of GVB pairs outside of the CAS active
space in a CAS-GVB calculation.
Restart Restart a CASSCF calculation. Note that
SCF=Restart performs the same function.
CASSCF MP2-SPECIFIC OPTIONS
DoOff Include off diagonal contributions within the
computation.
Thresh=n Set the cutoff for CI vector components
that are included to 10-n.
MP2States=mask Compute the MP2 correction for
the specified states. Mask is interpreted as a binary bit mask
specifying the desired states. For example, mask=1011 means to compute
states 1, 2 and 4. The default is to compute the correction only for the state
of interest.
NFC=n Set the number of frozen core orbitals.
NFV=n Set the number of frozen virtual
orbitals.
Note: NFC and NFV provide analogous functionality to
the Window option for regular MP2 calculations.
UseL906 Use the CAS MP2 facility that was the
default in Gaussian 94.
AVAILABILITY AND RESTRICTIONS
Energies, analytic gradients, and analytic and numerical
frequencies. CASSCF may not be combined with any semi-empirical method.
Analytic polarizabilites may not be performed with the
CASSCF method. Use CASSCF Polar=Numer.
When restarting a CASSCF optimization, the keywords CASSCF
Opt=Restart Extralinks=L405 must be included in the job's route section.
RELATED KEYWORDS
Opt=Conical,
MP2, Guess,
Pop, SCF
EXAMPLES
We will consider several of the most important uses of the CASSCF
method in this section.
Preliminary Examination of the Orbitals (Guess=Only). The
following route section illustrates one method of quickly examining the
orbitals in order to determine their symmetries and any alterations needed to
produce the desired initial state. We include Pop=Reg to obtain the
molecular orbital output in the population analysis section:
# HF/3-21G Guess=Only Pop=Reg Test
The molecule being investigated is 1,3-cyclobutadiene, a singlet
with D2h symmetry. We are going to run a 4x4 CAS, so there will be
four orbitals in the active space: 2 occupied and 2 virtual. We want all four
orbitals to be
orbitals.
The HOMO is orbital 14; therefore, orbitals 13 through 16 will
comprise the active space. When we examine these orbitals, we see that only
orbitals 14 and 15 are of the correct type. The molecule lies in the YZ-plane,
so orbitals will have significantly non-zero coefficients in the X
direction. Here are the relevant coefficients for orbitals 10 and 13-16:
Molecular Orbital Coefficients
10 13 14 15 16
O O O V V
3 1 C 2PX 0.29536 0.00000 0.34716 0.37752 0.00000
7 3PX 0.16911 0.00000 0.21750 0.24339 0.00000
12 2 C 2PX 0.29536 0.00000 0.34716 -0.37752 0.00000
16 3PX 0.16911 0.00000 0.21750 -0.24339 0.00000
21 3 C 2PX 0.29536 0.00000 -0.34716 -0.37752 0.00000
25 3PX 0.16911 0.00000 -0.21750 -0.24339 0.00000
30 4 C 2PX 0.29536 0.00000 -0.34716 0.37752 0.00000
34 3PX 0.16911 0.00000 -0.21750 0.24339 0.00000
Orbital 10 is clearly also a
orbital. If we look at higher virtual orbitals, we will find that orbital 19 is
also a
orbital. We have found our four necessary orbitals, and can now use
Guess=Alter to move them into the active space. Here is the input file
for the CASSCF calculation:
# CASSCF(4,4)/3-21G Guess=Alter Pop=Reg Test
1,3-Cyclobutadiene Singlet, D2H, Pi 4x4 CAS
0 1
molecule specification
10,13 Interchange orbitals 10 and 13.
16,19 Interchange orbitals 16 and 19.
CASSCF Energy and the One-Electron Density Matrix.
When we run this CASSCF calculation on cyclobutadiene, we will obtain a
prediction for the energy. It appears in the CASSCF output as follows:
TOTAL -152.836259
... energy at each iteration
ITN= 9 MaxIt= 64 E= -152.8402786733 DE=-1.17D-05 Acc= 1.00D-05
ITN= 10 MaxIt= 64 E= -152.8402826495 DE=-3.98D-06 Acc= 1.00D-05
...
DO AN EXTRA-ITERATION FOR FINAL PRINTING
The value of E for the final iteration is the predicted energy:
-152.8402826495 hartrees in this case. It is also important to examine the
one-electron density matrix, which appears next in the output:
Final one electron symbolic density matrix:
1 2 3 4
1 0.191842D+01
2 -0.139172D-05 0.182680D+01
3 0.345450D-05 0.130613D-05 0.172679D+00
4 0.327584D-06 0.415187D-05 0.564187D-06 0.820965D-01
MCSCF converged.
The diagonal elements indicate the approximate occupancies for
each successive orbital in the active space. If any of these values is
(essentially) zero, then that orbital was empty throughout the calculation;
similarly, if any of them is essentially 2, then that orbital was doubly
occupied throughout the CAS. In either case, there were no excitations into or
out of the orbital in question, and there is probably a problem with the CASSCF
calculation. In our case, the two “occupied” orbitals have values
less than 2, and the other two orbitals in the active space have non-zero
occupancies, so things are fine.
CASSCF MP2 Energy. When you run a CASSCF calculation with
correlation (CASSCF MP2 in the route section), the following additional
lines will appear in the CASSCF output (with the first one coming significantly
before the second):
MP2 correction to the MCSCF energy is computed
Indicates a CASSCF MP2 job.
...
E2 = -0.2635549296D+00 EUMP2 = -0.15310383973610D+03
The string EUMP2 labels the electron correlation-corrected CASSCF
energy; in this case, the value is -153.1038397361 hartrees.
CAS Configuration Information. The beginning of the CASSCF
output lists the configurations, in the following format:
PRIMARY BASIS FUNCTION= 1 2 1 2
2 SYMMETRY TYPE = 0
1 3
1 2
3 SYMMETRY TYPE = 0
2 3
1 2
The first line indicates the electron assignments for the lowest
configuration. This is a 4x4 CAS, so the primary basis function output
indicates that there is an
and
electron in both orbitals 13 and 14 (the numbers refer to the orbitals in the
active space, from lowest to highest, and the electron order in the output is:
      ). In configuration 2, the
electron in orbital 13 remains there, the
electron from orbital 14 has been excited to orbital 15, the
electron in orbital 13 remains there, as does the
electron in orbital 14. Similarly, in configuration 3, there is a
electron in orbital 13, an
(from 13) and
electron in orbital 14, and a
electron in orbital 15.
Using CASSCF to Study Excited States. The following
two-step job illustrates one method for studying excited state systems using
the CASSCF method. The first step assumes that a preliminary Hartree-Fock
single point calculation has been done in order to examine the orbitals; it
takes advantage of the initial guess computation done by that job, which it
retrieves from the checkpoint file:
%chk=CAS1
# CASSCF(2,4) 6-31+G(D) Guess=(Read,Alter)
# Pop=NaturalOrbital Test Geom=Check
Alter the guess so that the three LUMOs are all
the desired symmetry, and run the CAS.
0,1
orbital alterations
--Link1--
%chk=CAS1
%nosave
# CASSCF(2,4,NRoot=2) 6-31+G(D) Guess(Read)
# Pop(NaturalOrbital) Geom=Check Test
Excited state calculation
0,1
The second job step uses the NRoot option to CASSCF
to specify the first excited state. The first excitation energy for the
system will then be computed by taking the energy difference between the two
states (see exercise 5 in chapter 9 of Exploring Chemistry with Electronic
Structure Methods[304] for a more detailed
discussion of this technique).
Predicting Conical Intersections. Including
Opt=Conical keyword in the route section changes the job from an
optimization of the specified state using CASSCF to a search for a conical
intersection or avoided crossing involving that state. The optimized structure
will be that of the conical intersection or avoided crossing. Distinguishing
between these two possibilities may be accomplished by examining the final
eigenvalues in the CASSCF output for the final optimization step (it precedes
the optimized structure):
FINAL EIGENVALUES AND EIGENVECTORS
VECTOR EIGENVALUES CORRESPONDING EIGENVECTOR
state energy
1 -154.0503161 0.72053292 -0.48879229 ...
-0.16028934E-02 0.31874441E-02 ...
...
2 -154.0501151 0.45467877 0.77417416 ...
If the two eigenvalues (the first entry in the lines labelled with
a state number) are essentially the same, then the energies of the two states
are the same, and it is a conical intersection. Otherwise, it is an avoided
crossing.
Spin Orbit Coupling. Here is the output from a CASSCF
calculation where the spin orbit coupling has been requested with the
Spin option (the coupling is between the state specified to the
NRoot option and the next lower state):
****************************
spin-orbit coupling program
****************************
Number of configs= 4
1st state is 1 Identifies the two states between which the spin orbit coupling is computed.
2nd state is 2
Transition Spin Density Matrix
1 2
1 .000000D+00 .141313D+01
2 .553225D-01 .000000D+00
magnitude in x-direction= .0000000 cm-1
magnitude in y-direction= .0000000 cm-1
magnitude in z-direction= 55.2016070 cm-1
total magnitude= 55.2016070 cm-1 Spin orbit coupling.
MCSCF converged.
The spin orbit coupling is broken down into X, Y, and Z
components, followed by its total magnitude, which in this case is 55.2016070
cm-1.
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