The derivation of the CI-singles (CIS) energy and wave
function
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begins by selecting the HF
single-determinant wave function as reference for the ground state of the system:
(7.1) |
where is the number of electrons, and the spin orbitals
(7.2) |
are expanded in a finite basis of atomic orbital basis functions. Molecular orbital coefficients are usually found by SCF procedures which solve the Hartree-Fock equations
(7.3) |
where S is the overlap matrix, C is the matrix of molecular orbital coefficients, is a diagonal matrix of orbital eigenvalues and F is the Fock matrix with elements
(7.4) |
involving the core Hamiltonian and the anti-symmetrized two-electron integrals
(7.5) |
On solving Eq. (7.3), the total energy of the ground state single determinant can be expressed as
(7.6) |
where is the HF density matrix and is the nuclear repulsion energy.
Equation (7.1) represents only one of many possible determinants made from orbitals of the system; there are in fact possible singly substituted determinants constructed by replacing an orbital occupied in the ground state (, , ) with an orbital unoccupied in the ground state (, , ). Such wave functions and energies can be written
(7.7) |
(7.8) |
where we have introduced the anti-symmetrized two-electron integrals in the molecular orbital basis
(7.9) |
These singly excited wave functions and energies could be considered crude approximations to the excited states of the system. However, determinants of the form Eq. (7.7) are deficient in that they:
do not yield pure spin states
resemble more closely ionization rather than excitation
are not appropriate for excitation into degenerate states
These deficiencies can be partially overcome by representing the excited state wave function as a linear combination of all possible singly excited determinants,
(7.10) |
where the coefficients can be obtained by diagonalizing the many-electron Hamiltonian, A, in the space of all single substitutions. The appropriate matrix elements are:
(7.11) |
According to Brillouin’s, theorem single substitutions do not interact directly with a reference HF determinant, so the resulting eigenvectors from the CIS excited state represent a treatment roughly comparable to that of the HF ground state. The excitation energy is simply the difference between HF ground state energy and CIS excited state energies, and the eigenvectors of A correspond to the amplitudes of the single-electron promotions.
CIS calculations can be performed in Q-Chem using restricted
(RCIS),
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J. Chem. Phys.
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unrestricted (UCIS), or restricted
open-shell
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(ROCIS) spin orbitals. See Section 7.2.4
for a list of CIS-related job control variables.
$molecule 0 1 C O 1 CO H 1 CH 2 A H 1 CH 2 A 3 D CO = 1.2 CH = 1.0 A = 120.0 D = 180.0 $end $rem JOBTYPE = opt EXCHANGE = hf BASIS = 6-31G* $end @@@ $molecule read $end $rem EXCHANGE = hf BASIS = 6-311(2+)G* CIS_N_ROOTS = 15 Do 15 states CIS_SINGLETS = true Do do singlets CIS_TRIPLETS = false Don’t do Triplets $end
While CIS excitation energies are relatively inaccurate, with errors of the
order of 1 eV, CIS excited state properties, such as structures and
frequencies, are much more useful. This is very similar to the manner in
which ground state Hartree-Fock (HF) structures and frequencies are much
more accurate than HF relative energies. Generally speaking, for low-lying
excited states, it is expected that CIS vibrational frequencies will be
systematically 10% higher or so relative to
experiment.
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If the excited states are of
pure valence character, then basis set requirements are generally similar to
the ground state. Excited states with partial Rydberg character require the
addition of one or preferably two sets of diffuse functions.
Q-Chem includes efficient analytical first and second derivatives of the CIS
energy,
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to yield analytical gradients, excited
state vibrational frequencies, force constants, polarizabilities, and infrared
intensities. Analytical gradients can be evaluated for any job where the CIS
excitation energy calculation itself is feasible, so that efficient
excited-state geometry optimizations and vibrational frequency calculations are
possible at the CIS level. In such cases, it is necessary to specify on which
Born-Oppenheimer potential energy surface the optimization should proceed, and
care must be taken to ensure that the optimization remains on the excited state
of interest, as state crossings may occur. (A state-tracking algorithm,
as discussed in Section 9.8.5, can aid with this.
1435
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)
Sometimes it is precisely the crossings between Born-Oppenheimer potential
energy surfaces (i.e., conical intersections) that are of interest, as these
intersections provide pathways for nonadiabatic transitions between electronic
states.
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A feature of Q-Chem that is not
otherwise widely available in an analytic implementation (for both CIS and
TDDFT) of the nonadiabatic couplings that define the topology around conical
intersections.
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Due to the
analytic implementation, these couplings can be evaluated at a cost that is not
significantly greater than the cost of a CIS or TDDFT analytic gradient
calculation,
1433
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and the availability of these couplings allows for much more
efficient optimization of minimum-energy crossing points along seams of conical
intersection, as compared to when only analytic gradients are
available.
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These features, including a brief overview of the
theory of conical intersections, can be found in Section 9.8.1.
For CIS vibrational frequencies, a semi-direct algorithm similar to that used
for ground-state Hartree-Fock frequencies is available, whose computer time
scales as approximately for large molecules.
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The main complication associated with analytical CIS frequency calculations is
ensuring that Q-Chem has sufficient memory to perform the calculations.
Default settings are adequate for many purposes but if a large calculation
fails due to a memory limitation, then the following additional information may be useful.
The memory requirements for CIS (and HF) analytic frequencies primarily come from dynamic memory, defined as
dynamic memory = MEM_TOTAL MEM_STATIC .
This quantity must be large enough to contain several arrays whose size is . Meanwhile the value of the $rem variable MEM_STATIC, which obviously reduces the available dynamic memory, must be sufficiently large to permit integral evaluation, else the job may fail. For most purposes, setting MEM_STATIC to about 80 MB is sufficient, and by default MEM_TOTAL is set to a larger value that what is available on most computers, so that the user need not guess or experiment about an appropriate value of MEM_TOTAL for low-memory jobs. However, a memory allocation error will occur if the calculation demands more memory than available.
Note: Unlike Q-Chem’s MP2 frequency code, the analytic CIS second derivative code currently does not support frozen core or virtual orbitals. These approximations do not lead to large savings at the CIS level, as all computationally-expensive steps are performed in the atomic orbital basis.
$molecule 0 1 C O 1 CO H 1 CH 2 A H 1 CH 2 A 3 D CO = 1.2 CH = 1.0 A = 120.0 D = 150.0 $end $rem JOBTYPE = opt EXCHANGE = hf BASIS = 6-31+G* CIS_STATE_DERIV = 1 Optimize state 1 CIS_N_ROOTS = 3 Do 3 states CIS_SINGLETS = true Do do singlets CIS_TRIPLETS = false Don’t do Triplets $end @@@ $molecule read $end $rem JOBTYPE = freq EXCHANGE = hf BASIS = 6-31+G* CIS_STATE_DERIV = 1 Focus on state 1 CIS_N_ROOTS = 3 Do 3 states CIS_SINGLETS = true Do do singlets CIS_TRIPLETS = false Don’t do Triplets $end
The Random Phase Approximation (RPA),
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also known
as time-dependent Hartree-Fock (TD-HF) theory, is an alternative to CIS for
uncorrelated calculations of excited states. An RPA calculation is requested using the RPA
$rem variable that is described in Section 7.2.4.1.
RPA offers some advantages for
computing oscillator strengths, e.g., exact satisfaction of the
Thomas-Reike-Kuhn sum rule,
and is roughly comparable in
accuracy to CIS for singlet excitation energies, but is inferior for triplet
states. RPA energies are non-variational, and in moving around on excited-state
potential energy surfaces, this method can occasionally encounter singularities
(arising from triplet instabilities in the underlying reference state)
that prevent numerical solution of the RPA equations.
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In Q-Chem, these instabilities are generally accompanied by an error message to the effect
that an imaginary root has been detected in the RPA equations.
This is mathematically impossible in CIS calculations, which decouple the excitation energy problem
from the stability problem.
DFT/CIS
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is a semi-empirical method that uses Kohn-Sham orbitals instead of Hartree-Fock orbitals with a CIS-like formalism.
This leads to added correlation energy from the Kohn-Sham orbitals and, perhaps more importantly, orbital energy differences
that better resemble excitation energies, and bound virtual orbitals that better approximate localized excited states
as compared to Hartree-Fock virtual orbitals, which are typically unbound.
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Along with certain semi-empirical corrections, DFT/CIS significantly improves conventional Hartree–Fock-based CIS.
Two parameterizations of the DFT/CIS Hamiltonian are available in Q-Chem: Grimme’s original one,
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which is designed
for use with the B3LYP functional, and a new parameterization designed for CAM-B3LYP.
The latter (CAM-B3LYP/CIS) implementation has specific parameterizations aimed at accurately reproducing X-ray spectra,
whereas B3LYP/CIS is suitable only for valence excitations.
The nature of the parameterization limits use of DFT/CIS to the aforementioned two functionals, and primarily to two basis sets.
The CAM-B3LYP/CIS method is parameterized for use with def2-TZVPD while B3LYP/CIS is parameterized for use with TZVP.
The DFT/CIS method is controlled by the DFTCIS and DFTCIS_PARAMS job control variables that are described in Section 7.2.4.1.
$molecule 0 1 O H 1 0.960652 H 1 0.960652 2 103.913458 $end $rem JOBTYPE = sp METHOD = b3lyp UNRESTRICTED = false BASIS = TZVP DFTCIS = true DFTCIS_PARAMS = 1 !0=CIS, 1=B3LYP/CIS, 2=CAM-B3LYP/CIS CIS_N_ROOTS = 5 CIS_TRIPLETS = false SCF_ALGORITHM = diis $end