CIS
CIS(D)

DESCRIPTION

TheCISmethod keyword requests a calculation on excited states using single-excitation CI (CI-Singles)[Foresman92]. This implementation works for both closed shell and open shell systems. Chapter 9 ofExploring Chemistry with Electronic Structure Methods[Foresman96b]provides a detailed discussion of this method and its uses.

CIS(D)is used to request the related CIS(D) method (i.e. theDoption)[Head-Gordon94a,Head-Gordon95]. You can also follow aCISjob with aCIS(D)job to compute the excitation energies for additional states (see the examples).

CISjobs can include theDensitykeyword; 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 withCIS(D).

An energy range can be specified forCISexcitation energies using some options found under the energy range options below.

STATE SELECTION OPTIONS

Singlets
Solve only for singlet excited states. This option only affects calculations on closed-shell systems, for which it is the default.

Triplets
Solve only for triplet excited states. This option only affects calculations on closed-shell systems.

50-50
Solve for half triplet and half singlet states. This option only affects calculations on closed-shell systems.

Root=N
Specifies the “state of interest” for which the generalized density is to be computed. The default is the first excited state (N=1).

NStates=M
Solve forMstates (the default is 3). If50-50is requested,NStatesgives the number of each type of state for which to solve (i.e., the default is 3 singletsand3 triplets).

Add=N
Read converged states off the checkpoint file and solve for an additionalNstates. This option impliesReadas well.NStatescannot be used with this option.

ENERGY RANGE OPTIONS

An energy range can be specified forCISandTDexcitation energies using the following options toCIS,TDandTDA.

GOccSt=N
Generate initial guesses using only active occupied orbitalsNand higher.

GOccEnd=N
Generate initial guesses: ifN>0, use only the firstNactive occupied orbitals; ifN<0, do not use the highest |N| occupieds.

GDEMin=N
Generate guesses having estimated excitation energies ≥N/1000 eV.

DEMin=N
Converge only states having excitation energy ≥N/1000 eV; ifN=-2, read threshold from input; ifN<-2, set the threshold to |N|/1000 Hartrees.

IFact=N
Specify factor by which the number of states updated during initial iterations is increased.

WhenReduce=M
Reduce to the desired number of states after iterationM.

The default forIFactisMax(4,g) wheregis the order of the Abelian point group. The default forWhenReduceis 1 forTDand 2 forTDAandCIS. Larger values may be needed if there are many states in the range of interest.

DENSITY-RELATED OPTION

AllTransitionDensities
Computes the transition densities between every pair of states.

PROCEDURE- AND ALGORITHM-RELATED OPTIONS

FC
All frozen core options are available with this keyword. See the discussion of theFCoptions for full information.

Direct
Forces solution of the CI-Singles equation using AO integrals which are recomputed as needed.CIS=Directshould be used only when the approximately 4O2N2words of disk required for the default (MO) algorithm are not available, or for larger calculations (over 200 basis functions).

MO
Forces solution of the CI-Singles equations using transformed two-electron integrals. This is the default algorithm in Gaussian 09. The transformation attempts to honor theMaxDiskkeyword, thus further moderating the disk requirements.

AO
Forces 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=N
Sets the convergence calculations to 10-Non the energy and 10-(N-2)on the wavefunction. The default isN=4 for single points andN=6 for gradients.

Read
Reads 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.

Restart
Restarts the CI-Singles iterations off the checkpoint file. Also impliesSCF=Restart.

RWFRestart
Restarts the CI-Singles iterations off the read-write file. Useful when using non-standard routes to do successive CI-Singles calculations.

EqSolv
Whether to perform equilibrium or non-equilibrium PCM solvation.NonEqSolvis the default except for excited state optimizations and when the excited state density is requested (e.g., withDensity=CurrentorAll).

NoIVOGuess
Forces the use of canonical single excitations for the guess.IVOGuess, which uses improved virtual orbitals, is the default.

DEBUGGING OPTIONS

ICDiag
Forces in-core full diagonalization of the CI-Singles matrix formed in memory from transformed integrals. This is mainly a debugging option.

MaxDiag=N
Limits the submatrix diagonalized in the Davidson procedure to dimensionN. This is mainly a debugging option.MaxDavidsonis a synonym for this option.

AVAILABILITY

Energies, analytic gradients, and analytic frequencies forCIS(including open shell systems), and energies forCIS(D).

RELATED KEYWORDS

ZIndo,TD,MaxDisk,Transformation,Density

EXAMPLES

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#Poutput):

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  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 (useIOp(9/40=N)to request more coefficients: all that are greater than 10-N):

Excitation energies and oscillator strengths:Symmetry, excitation energy, oscillator strengthExcited State 1: Singlet-A' 3.7006 eV 335.03 nm f=0.0008 8 -> 9 0.69112CI expansion coeffs. for each excitation (here, orbital 8 to 9)This state for opt. and/or second-order corr.The state of interestTotal Energy, E(CIS) = -113.696894498CIS energy is repeated here for convenience

CI expansion coefficients give the importance of excited determinants in the excited state wavefunction.

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 theCISresults from the checkpoint file and solve for 6 additional states beyond the second state:

# CIS=(Read,Root=2,NStates=6)


Last update: 2 August 2013

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