Electronic structure Hartree-Fock theory

Recently, a third class of electronic structure methods have come into wide use density functional methods. These DFT methods are similar to ab initio methods in many ways. DFT calculations require about the same amount of computation resources as Hartree-Fock theory, the least expensive ab initio method. 

Hartree-Fock theory is very useful for providing initial, first-level predictions for many systems. It is also reasonably good at computing the structures and vibrational frequencies of stable molecules and some transition states. As such, it is a good base-level theory. However, its neglect of electron correlation makes it unsuitable for some purposes. For example, it is insufficient for accurate modeling of the energetics of reactions and bond dissociation. 

The DFT and MP2 calculations produce very similar structures, although the BLYP bond length is again longer than those of the other functionals. Hartree-Fock theory predicts a bond length which is significantly shorter than the methods including electron correlation. 

The value of 3 and its dispersion can be theoretically calculated from equation 6, provided a complete set of electron states of the system is known. Such quantum mechanical calculations have been developed based on molecular Hartree-Fock theory including configuration interactions( 1 3). A detailed theoretical analysis of 3 and contributing 1T -electron states has been presented for several important molecular structures. 

Most of the commonly used electronic-structure methods are based upon Hartree-Fock theory, with electron correlation sometimes included in various ways (Slater, 1974). Typically one begins with a many-electron wave function comprised of one or several Slater determinants and takes the one-electron wave functions to be molecular orbitals (MO s) in the form of linear combinations of atomic orbitals (LCAO s) (An alternative approach, the generalized valence-bond method (see, for example, Schultz and Messmer, 1986), has been used in a few cases but has not been widely applied to defect problems.)... 

We have presented a practical Hartree-Fock theory of atomic and molecular electronic structure for individual electronically excited states that does not involve the use of off-diagonal Lagrange multipliers. An easily implemented method for taking the orthogonality constraints into account (tocia) has been used to impose the orthogonality of the Hartree-Fock excited state wave function of interest to states of lower energy. 

Hartree-Fock theory is a rigorous ab initio theory of electronic structure and has a vast array of successes to its credit. Equilibrium structures of most molecules are calculated almost to experimental accuracy, and reasonably accurate properties (e.g., dipole moments and IR and Raman intensities) can be calculated from HF wave functions. Rela-... 

Orbital interaction theory forms a comprehensive model for examining the structures and kinetic and thermodynamic stabilities of molecules. It is not intended to be, nor can it be, a quantitative model. However, it can function effectively in aiding understanding of the fundamental processes in chemistry, and it can be applied in most instances without the use of a computer. The variation known as perturbative molecular orbital (PMO) theory was originally developed from the point of view of weak interactions [4, 5]. However, the interaction of orbitals is more transparently developed, and the relationship to quantitative MO theories is more easily seen by straightforward solution of the Hiickel (independent electron) equations. From this point of view, the theoretical foundations lie in Hartree-Fock theory, described verbally and pictorially in Chapter 2 [57] and more rigorously in Appendix A. 

When discussing the electronic structure of molecules and solids, one-electron descriptions, such as the molecular orbitals of Equation 8.1, are quite intuitive. It is common to talk about individual electrons occupying particular states. For example, reactions often occur by the mixing of the highest occupied molecular orbital (HOMO) of one species and the lowest unoccupied molecular orbital (LUMO) of another. In such a reaction the electrons in the HOMO state move into the new mixed orbital, lowering their energy. The HOMO and LUMO states are each pairs of one-electron molecular orbitals, since in the simplest case an orbital giving the spahal distribution for a spin up electron has an identical partner for spin down. Mulh-electron wavefunctions that describe the whole electronic structure in this picture are constructed from the one-electron states. So, for example, in a four-electron system in which all the electronic states are doubly occupied (spin up and spin down), based on Hartree-Fock theory we can write ... 

In 2002, Nakai [24] presented a non-Bom-Oppenheimer theory of molecular structure in which molecular orbitals (MO) are used to describe the motion of individual electrons and nuclear orbitals (NO) are introduced each of which describes the motion of single nuclei. Nakai presents an ab initio Hartree-Fock theory, which is designated NO+MO/HF theory , which builds on the earlier work of Tachikawa et al. [25]. In subsequent work published in 2003, Nakai and Sodeyama [26] apply MBPT to the problem of simultaneously describing both the nuclear and electronic components of a molecular system. Their approach will be considered in some detail in this paper as a first step in the development of a literate quantum chemistry program for the simultaneous description of electronic and nuclear motion. 

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