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Hartree-Fock approximation length

Calculations show that cross-sections obtained in the Hartree-Fock approximation utilizing length and velocity forms of the appropriate operator, may essentially differ from each other for transitions between neighbouring outer shells, particularly with the same n. However, they are usually close to each other in the case of photoionization or excitation from an inner shell whose wave function is almost orthogonal with the relevant function of the outer open shell. In dipole approximation an electron from a shell lN may be excited to V = l + 1, but the channel /— / + prevails. For configurations ni/f1 n2l 2 an important role is... [Pg.396]

One reason for interest in more accurate calculations on HF has been the measured dissociation energy Z)o(HF), which can be obtained from photoionization or photoelectron spectra. Since HF+ dissociates correctly within the Hartree-Fock approximation to H+ and F(2P) in both the X2Tl and 2S+ states, PE curves were calculated by Julienne et a/.,203 and later by Bondybey et a/.,187 both of whom obtained values of Do in good agreement with experiment for the SCF calculation. The bond length in HF+ of 1.000 bohr is less than the experimental result, which the authors call into question. Julienne et al. give a detailed discussion of the adiabatic dissociation process. HF+ was also considered in the calculations of ref. 198. Richards and co-workers have reported several calculations of the PE curves of HF+, including the A2E+ state, which is correctly predicted to be bound.204... [Pg.107]

Consider, as an example, polyethylene if the chains are packed as in the crystal (Fig. 1), there are 5.5 x 10 per m in the plane perpendicular to their length. Hence the tensile fracture stress would be 33 GPa. Variants of this approach, using simple Morse potentials, provide values ranging from about 19 to 36 GPa. Other calculations using Hartree-Fock self-consistent field methods yield values of 66 GPa at 0 K (Crist et al., 1979). This last value seems a bit high and may be due to inaccuracies of the Hartree-Fock approximation at large atomic separations. [Pg.31]

The Hartree-Fock approximation, which is equivalent to the molecular orbital approximation, is central to chemistry. The simple picture, that chemists carry around in their heads, of electrons occupying orbitals is in reality an approximation, sometimes a very good one but, nevertheless, an approximation—the Hartree-Fock approximation. In this chapter we describe, in detail, Hartree-Fock theory and the principles of ab initio Hartree-Fock calculations. The length of this chapter testifies to the important role Hartree-Fock theory plays in quantum chemistry. The Hartree-Fock approximation s important not only for its own sake but as a starting point for more accurate approximations, which include the effects of electron correlation. A few of the computational methods of quantum chemistry bypass the Hartree-Fock approximation, but most do not, and all the methods described in the subsequent chapters of this book use the Hartree-Fock approximation as a starting point. Chapters 1 and 2 introduced the basic concepts and mathematical tools important for an indepth understanding of the structure of many-electron theory. We are now in a position to tackle and understand the formalism and computational procedures associated with the Hartree-Fock approximation, at other than a superficial level. [Pg.108]

In this subsection, we describe restricted closed-shell calculations on the ground state of H2. As we will see, there is a very basic deficiency in such calculations at long bond lengths. Later in this chapter, when we describe unrestricted open-shell calculations, we will return to minimal basis H2 and partially correct this deficiency. Some of the results obtained here will also be used in later chapters when we use the minimal basis H2 model to illustrate procedures that go beyond the Hartree-Fock approximation. [Pg.159]

TABLE 2.3. Optimized Single-Double Bond Length Difference AR, Total Energy per Unit Cell, and the Fundamental Gap in trans-FA in the Hartree-Fock Approximation Using Different Basis Sets ... [Pg.67]

Fig. 9 Total energy per carbon atom contours for C4 +2H4 +2 planar all-cis rings as a function of the two consecutive bond lengths, according to the Hartree-Fock approximation. The number of carbon atoms ( c = 4ra + 2) increases from 6 to 14 in steps of four atoms... Fig. 9 Total energy per carbon atom contours for C4 +2H4 +2 planar all-cis rings as a function of the two consecutive bond lengths, according to the Hartree-Fock approximation. The number of carbon atoms ( c = 4ra + 2) increases from 6 to 14 in steps of four atoms...
The Hartree-Fock equilibrium bond distance of the hydrogen molecule is 1.387oo. just. % shorter than the FCI value of 1.402ao- In Section 15.3, we shall see that this excellent behaviour with respect to bond distances is often observed for the Hartree-Fock approximation and that Hartree-Fock bond lengths are typically 2-3 pm too short. [Pg.172]

Table 8.7 The equilibrium bond length Re and the dissociation energy De of BH in the electronic ground state calculated in the Hartree-Fock approximation and using FCI wave functions with and without core correlation. The experimental bond length is 2.3289oo [18]. The experimental dissociation energy of 131.0 m is in doubt -see [18] and Exercise 15.1... Table 8.7 The equilibrium bond length Re and the dissociation energy De of BH in the electronic ground state calculated in the Hartree-Fock approximation and using FCI wave functions with and without core correlation. The experimental bond length is 2.3289oo [18]. The experimental dissociation energy of 131.0 m is in doubt -see [18] and Exercise 15.1...
In this paper we present the first application of the ZORA (Zeroth Order Regular Approximation of the Dirac Fock equation) formalism in Ab Initio electronic structure calculations. The ZORA method, which has been tested previously in the context of Density Functional Theory, has been implemented in the GAMESS-UK package. As was shown earlier we can split off a scalar part from the two component ZORA Hamiltonian. In the present work only the one component part is considered. We introduce a separate internal basis to represent the extra matrix elements, needed for the ZORA corrections. This leads to different options for the computation of the Coulomb matrix in this internal basis. The performance of this Hamiltonian and the effect of the different Coulomb matrix alternatives is tested in calculations on the radon en xenon atoms and the AuH molecule. In the atomic cases we compare with numerical Dirac Fock and numerical ZORA methods and with non relativistic and full Dirac basis set calculations. It is shown that ZORA recovers the bulk of the relativistic effect and that ZORA and Dirac Fock perform equally well in medium size basis set calculations. For AuH we have calculated the equilibrium bond length with the non relativistic Hartree Fock and ZORA methods and compare with the Dirac Fock result and the experimental value. Again the ZORA and Dirac Fock errors are of the same order of magnitude. [Pg.251]

Table 3.7. Calculated equilibrium structural properties of H,0 and NHj [bond lengths, / (0-H) and 7 (N-H) in A, bond angles Table 3.7. Calculated equilibrium structural properties of H,0 and NHj [bond lengths, / (0-H) and 7 (N-H) in A, bond angles <H-0-H and <H-N-H in degrees] obtained using density-functional theory (local-density approximation, LCAO-Aa method) and Hartree-Fock-Roothaan theory, compared with experimental data...

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