| CISCIS(D)

 The 
CIS method keyword requests a calculation on excited states using single-excitation 
CI (CI-Singles) [108]. Chapter 9 of Exploring 
Chemistry with Electronic Structure Methods [308] 
provides a detailed discussion of this method and its uses. The CIS(D) 
keyword and option is used to request the related CIS(D) method [426,427]. 
You can also follow a CIS job with a CIS(D) job to compute the excitation 
energies for additional states (see the examples). CIS jobs can include 
the Density keyword; without options, this 
keyword causes the population analysis to use the current (CIS) density rather 
than its default of the Hartree-Fock density. Note that Density cannot 
be used with CIS(D). STATE SELECTION OPTIONSSingletsSolve only for singlet excited states. This option only affects calculations on 
closed-shell systems, for which it is the default.
 TripletsSolve only for triplet excited states. This option only affects calculations on 
closed-shell systems.
 50-50Solve for half triplet and half singlet 
states. This option only affects calculations on closed-shell systems.
 Root=NSpecifies the "state of interest" for which the generalized density is to be computed. 
The default is the first excited state (N=1).
 NStates=MSolve for M states (the default is 3). If 50-50 is requested, NStates 
gives the number of each type of state for which to solve (i.e., the default is 
3 singlets and 3 triplets).
 Add=NRead converged 
states off the checkpoint file and solve for an additional N states. This 
option implies Read as well. NStates cannot be used with this option.
 DENSITY-RELATED 
OPTIONAllTransitionDensities
 Computes the transition 
densities between every pair of states.
 PROCEDURE- AND ALGORITHM-RELATED 
OPTIONSFCAll frozen core options are 
available with CIS and CIS(D).
 DirectForces solution 
of the CI-Singles equation using AO integrals which are recomputed as needed. 
CIS=Direct should be used only when the approximately 4O2N2 
words of disk required for the default (MO) algorithm are not available, 
or for larger calculations (over 200 basis functions).
 MOForces 
solution of the CI-Singles equations using transformed two-electron integrals. 
This is the default algorithm in Gaussian 03. The transformation 
attempts to honor the MaxDisk keyword, thus further moderating the disk 
requirements.
 AOForces solution of the CI-Singles equations 
using the AO integrals, avoiding an integral transformation. The AO basis is seldom 
an optimal choice, except for small molecules on systems having very limited disk 
and memory.
 Conver=NSets the convergence calculations 
to 10-N on the energy and 10-(N+2) on the wavefunction. 
The default is N=4 for single points and N=6 for gradients.
 ReadReads initial guesses for the CI-Singles states off the checkpoint file. Note 
that, unlike for SCF, an initial guess for one basis set cannot be used for a 
different one.
 RestartRestarts the CI-Singles iterations off 
the checkpoint file. Also implies SCF=Restart.
 RWFRestartRestarts the CI-Singles iterations off the read-write file. Useful when using 
non-standard routes to do successive CI-Singles calculations.
 EqSolvWhether to perform equilibrium or non-equilibrium PCM solvation. NonEqSolv 
is the default.
 NoIVOGuessForces the use of canonical single 
excitations for the guess. IVOGuess, which uses improved virtual orbitals, 
is the default.
 DEBUGGING OPTIONSICDiagForces in-core 
full diagonalization of the CI-Singles matrix formed in memory from transformed 
integrals. This is mainly a debugging option.
 MaxDiag=NLimits the submatrix diagonalized in the Davidson procedure to dimension N. 
This is mainly a debugging option. MaxDavidson is a synonym for this option.
 
 Energies, 
analytic gradients, and analytic frequencies for CIS, and energies for 
CIS(D). 
 ZINDO, 
TD, MaxDisk, 
Transformation, Density 
 CIS 
Output. There are no special features or pitfalls with CI-Singles input. Output 
from a single point CI-Singles calculation resembles that of a ground-state CI 
or QCI run. An SCF is followed by the integral transformation and evaluation of 
the ground-state MP2 energy. Information about the iterative solution of the CI 
problem comes next; note that at the first iteration, additional initial guesses 
are made, to ensure that the requested number of excited states are found regardless 
of symmetry. After the first iteration, one new vector is added to the solution 
for each state on each iteration. The change in excitation energy and wavefunction 
for each state is printed for each iteration (in the #P output): Iteration   3 Dimension    27 
Root  1 not converged, maximum delta is   0.002428737687607 
Root  2 not converged, maximum delta is   0.013107675296678 
Root  3 not converged, maximum delta is   0.030654755631835 
Excitation Energies [eV] at current iteration: 
Root  1 :      3.700631883679401   Change is   -0.001084398684008 
Root  2 :      7.841115226789293   Change is   -0.011232152003400 
Root  3 :      8.769540624626156   Change is   -0.047396173133051 The 
iterative process can end successfully in two ways: generation of only vanishingly 
small expansion vectors, or negligible change in the updated wavefunction. When 
the CI has converged, the results are displayed, beginning with this banner: ***************************************************************** 
Excited States From <AA,BB:AA,BB> singles matrix: 
***************************************************************** The transition dipole moments between the ground and each excited state 
        are then tabulated. Next, the results on each state are summarized, including 
        the spin and spatial symmetry, the excitation energy, the oscillator strength, 
        and the largest coefficients in the CI expansion (use IOp(9/40=N) 
        to request more coefficients: all that are greater than 10-N): Excitation energies and oscillator strengths:
                     symmetry                              excitation energy                                       oscillator strength
Excited State    1:  Singlet-A"        3.7006 eV      335.03 nm       f=0.0008
       8 -> 9         0.69112                   CI expansion coefficients for each excitation.
Excitation is from orbital 8 to orbital 9 
This state for opt. and/or second-order corr.           => This is the "state of interest.
Total Energy, E(Cis)  =   - 113.696894498                                                     CIS energy is repeated here for convenience.Normalization. For closed shell calculations, the sum of the squares 
        of the expansion coefficients is normalized to total 1/2 (as the beta 
        coefficients are not shown). For open shell calculations, the normalization 
        sum is 1. Finding Additional States. 
The following route will read the CIS results from the checkpoint file 
and solve for 6 additional states beyond the second state: # CIS=(D,Read,Root=2,NStates=6) 
 The same procedure will work using CIS(D) in the follow-up job. |