Chem Topic: Excited States



 Hello all,
 	I have written the following short essay for my users and am
 posting it here for your enjoyment and comments.  Please let me know
 if I missed any important techniques.
 	My compilation of chemical topics can be accessed via the web
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                                 Dave Young
                                 youngd2-0at0-mail.auburn.edu
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                        Calculating Electronic Excited States
    				   David Young
 			Division of University Computing
                        		 144 Parker Hall
                       	        Auburn University
                        		Auburn, AL 36849
 INTRODUCTION
 	This is an introduction to the techniques used for the calculation
 of electronic excited states of molecules (sometimes called eximers).
 Specifically, these are methods for obtaining wave functions for the
 excited states of a molecule from which energies and other molecular properties
 (such as dipole moments) can be calculated.  These calculations are an
 important tool for the analysis of spectroscopy, reaction mechanisms
 and other excited state phenomena.
 	These same techniques may also be necessary to find the ground state
 wave function.  Determining the ground state electron configuration can
 be particularly difficult for compounds with very low energy excited states.
 	This document is concerned only with ab initio calculations.  These
 are calculations in which only the theory of quantum mechanics is applied
 with no experimental data used in the calculation.  Some of these techniques
 are also applicable to certain classes of semiempirical calculations.
 	This write up is not intended to be a detailed description.
 It is meant to be a short introduction with a discussion of strengths and
 weaknesses of various methods.  This should also serve as a check list
 of available methods when faced with computational difficulties.  References
 are provided for more detailed discussions information.
 SPIN STATES
 	Ab initio programs attempt to compute the lowest energy state of
 a specified multiplicity.  Thus calculations for different spin states
 will give a lowest energy state and a few of the excited states.  This
 is most often done to determine singlet - triplet gaps in organic molecules.
 CIS
 	A single excitation configuration interaction (CIS) calculation is
 probably the most common way to get excited state energies.  This is because
 it is one of the easiest calculations to perform.
 	A configuration interaction calculation uses molecular orbitals
 that have been optimized typically with a Hartree-Fock (HF) calculation.
 Generalized Valence Bond (GVB) and multi-configuration self consistent
 field (MCSCF) calculations can also be used as a starting point for
 a configuration interaction calculation.
 	A CIS calculation starts with this initial set of orbitals and
 moves one electron to one of the virtual orbitals from the original
 calculation.  This gives a description of one of the excited states of
 the molecule, but does not change the quality of the description of the
 ground state as double excitation CIs do.  This gives a wave function of
 somewhat lesser quality than the original calculation since the orbitals
 have been optimized for the ground state.  Often this results in the ground
 state energy being a bit low relative to the other states.
 	A CIS calculation is not extremely accurate.  However, it has the
 advantage of being able to compute many excited state energies easily.
 INITIAL GUESS
 	If the initial guess for a calculation is very close to an
 excited state wave function, the calculation may converge to that
 excited state.  This is typically done by doing an initial calculation
 then using it's wave function with some of the orbitals switched as
 the initial guess for another calculation.
 	The advantage of this method is that the orbitals have been
 optimized for the excited state.
 	The disadvantage is that there is no guarantee that it will work.
 If there is no energy barrier between the initial guess and the ground state
 wave function, the entire calculation will converge back to the ground state.
 The convergence path may take the calculation to an undesired state in
 any case.
 	A second disadvantage of this technique applies if the state is the
 same symmetry as a lower energy state.  There is no guarantee that the
 state obtained is completely orthogonal to the ground state.  This means
 that the wave function obtained may be some mix of the lower energy
 state and a higher energy state.  In practice, this type of calculation
 only converges to a higher state if a fairly reasonable description of
 the excited state wave function is obtained.  Mixing tends to be a significant
 concern if the orbital energies are very close together or the system is very
 sensitive to correlation effects.
 BLOCK DIAGONAL HAMILTONIANS
 	Most ab initio calculations use symmetry adapted molecular orbitals.
 Under this scheme, the Hamiltonian matrix is block diagonal meaning that
 every molecular orbital will behave according to the symmetry of one of the
 irreducible representations of the point group.  No orbitals will be described
 by a mixing of different irreducible representations.
 	Some programs such as COLUMBUS, DMOL and GAMESS actually set up a
 separate matrix for each irriducible representation and solve them separately.
 Such programs give the user the option of defining how many electrons
 are of each irreducible representation.  This defines the symmetry of the
 wave function.  In this case the resulting wave function is the lowest
 energy wave function of a particular symmetry.
 	This is a very good way to get excited states which differ in
 symmetry from the ground state and are the lowest energy state within that
 symmetry.
 HIGHER ROOTS OF A CI
 	For configuration interaction calculations of double excitations
 or higher, it is possible to solve the CI super-matrix for the second root,
 third root, fourth root, etc.
 	This is a very reliable way to get a high quality wave function for
 the first few excited states.  For higher excited states, CPU times become
 very large since more iterations are generally needed to converge the
 CI calculation.
 NEGLECTING A BASIS FUNCTION
 	Some programs, such as COLUMBUS, allow a calculation to be done
 with some orbitals completely neglected from the calculation.  For example,
 in a transition metal compound you could work with four d functions so that
 the calculation would have no way to occupy the function that was left out.
 	This is a reliable way to get an excited state wave function even
 when it is not the lowest energy wave function of that symmetry.  However
 it might take a bit of work to construct the input file depending upon the
 individual program.
 IMPOSING ORTHOGONALITY - DFT TECHNIQUES
 	Traditionally, excited states have not been one of the strong
 points of density functional theory.  This is due to the difficulty
 in ensuring orthogonality to the ground state wave function when
 no wave functions are being used in the calculation.
 	The easiest excited states to find using density functional
 theory techniques are those which are the lowest state of a given
 symmetry thus using a ground state calculation.
 	A promising techniques is one which uses a variational bound
 for the average of the first M states of a molecule.
 	A few other options have been examined.  However, there is not
 yet a large enough volume of work applying DFT to excited states to
 predict the reliability of any of these techniques.
 IMPOSING ORTHOGONALITY - QMC TECHNIQUES
 	Quantum Monte Carlo (QMC) methods are computations which use a
 statistical integration to calculate integrals which could not be
 evaluated analytically.  These calculations can be extremely accurate,
 but often at the expense of enormous CPU times.
 	There are a number of methods for getting excited state energies
 from QMC calculations.  These methods will only be mentioned here and
 are explained more fully in the text by Hammond, Lester and Reynolds
 referenced at the end of this document.
 	Computations done in imaginary time can yield an excited state
 energy by a transformation of the energy decay curve.
 	If an accurate description of the ground state is already available,
 an excited state description can be obtained by forcing the wave function
 to be orthogonal to the ground state wave function.
 	Diffusion and Green's function QMC calculations are often done
 using a fixed node approximation.  Within this scheme, the nodal surfaces
 used define the state that is obtained as well as ensuring an antisymmetric
 wave function.
 	Matrix QMC procedures similar to configuration interaction
 treatments have been devised in an attempt to calculate many states
 concurrently.  These methods are not yet well developed as evidenced
 by oscillatory behavior in the excited state energies.
 FURTHER INFORMATION
 There are many books on the principles of quantum mechanics and every
 physical chemistry text has an introductory treatment.  The
 work which I am listing here is a two volume set with each chapter
 broken into a basic and advanced sections making it excellent for
 both intermediate and advanced users.
 C. Cohen-Tannoudji, B. Diu, F. Laloe "Quantum Mechanics Volumes I &
 II"
 Wiley-Interscience (1977)
 For an introduction to quantum chemistry see
 D. A. McQuarrie "Quantum Chemistry" University Science Books (1983)
 A graduate level text on quantum chemistry is
 I. N. Levine "Quantum Chemistry" Prentice Hall (1991)
 For quantum Monte Carlo methods, order the following book using
 ISBN 981-02-0322-5 because the title is listed incorrectly in
 'Books in Print'.
 B. L. Hammond, W. A. Lester, Jr., P. J. Reynolds "Monte Carlo Methods
 in Ab Initio Quantum Chemistry" World Scientific (1994)
 For density functional theory see
 R. G. Parr, W. Yang "Density-Functional Theory of Atoms and Molecules"
 Oxford (1989)
 There is a comprehensive listing of all available molecular modeling
 software and structural databanks, free or not, in appendix 2 of
 "Reviews in Computational Chemistry Volume 6"
 Ed. K. B. Lipkowitz and D. B. Boyd, VCH (1995)
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