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Averaged second-order energies

Before proceeding to applications, let us discuss another important aspect of averaged second-order energies Eqs. (15) and (17). Both formulae are of multipartitioning nature the zero-order operator varies with principal determinant AT). This affects not only the bi-orthogonal vector set, but also the zero-order excitation... [Pg.264]

Table 3.26. Relative energies AE and other properties of triaminomethylfluoride rotamers (cf. Fig. 3.68) showing C—F bond length Rce, frequency Wcf, NRTbond order bef, bond ioniciiy ice, fluoride charge qe, and average second-order stabilization energy for m 3-oriented iin-cfcf and iin-gcn interactions... Table 3.26. Relative energies AE and other properties of triaminomethylfluoride rotamers (cf. Fig. 3.68) showing C—F bond length Rce, frequency Wcf, NRTbond order bef, bond ioniciiy ice, fluoride charge qe, and average second-order stabilization energy for m 3-oriented iin-cfcf and iin-gcn interactions...
Figure 1. Experimental variations of 2p-core ionization energies (in eV) for atoms from A1(Z = 13) to Ba(Z = 56). Upper left. 2p /2 and 2p3/2 energies lower left, their weighted-average second-order discrete derivative, as functions of Z upper right spin-orbit splitting between the 2pi/2 and 2p3/2 levels lower right, its second derivative, as functions of Z. On the derivative diagrams shell effects appear about fully filled and half-filled shells and near filling irregularities of the transition elements. Figure 1. Experimental variations of 2p-core ionization energies (in eV) for atoms from A1(Z = 13) to Ba(Z = 56). Upper left. 2p /2 and 2p3/2 energies lower left, their weighted-average second-order discrete derivative, as functions of Z upper right spin-orbit splitting between the 2pi/2 and 2p3/2 levels lower right, its second derivative, as functions of Z. On the derivative diagrams shell effects appear about fully filled and half-filled shells and near filling irregularities of the transition elements.
The second-order energy obtained by averaging looks... [Pg.264]

These can be considered as a perturbation, the unperturbed problem being the harmonic oscillator. Since the average value of QkQiQm is zero in any state v, the first-order perturbation energy due to the cubic terms vanishes, but the second-order energy does not. The first-order energy from the quartic terms involves the mean value of hkbnnQkQiQ,aQn, which vanishes except for two classes of terms QIQ and QjJ. The mean values of terms of the first class arc given by (see Appendix III)... [Pg.303]

In the case at hand—the many-electron atom—we can justify the qualitative behavior of the first- and second-order energy corrections as follows. The first-order correction must be positive, because it is the average of the electron-electron repulsion. However, because that repulsion is averaged over the densities of non-interacting electrons (using the zero-order wavefunctions), it overestimates... [Pg.168]

A more balanced description requires MCSCF based methods where the orbitals are optimized for each particular state, or optimized for a suitable average of the desired states (state averaged MCSCF). It should be noted that such excited state MCSCF solutions correspond to saddle points in the parameter space for the wave function, and second-order optimization techniques are therefore almost mandatory. In order to obtain accurate excitation energies it is normally necessarily to also include dynamical Correlation, for example by using the CASPT2 method. [Pg.147]

The vast majority of the kinetic detail is presented in tabular form. Amassing of data in this way has revealed a number of errors, to which attention is drawn, and also demonstrated the need for the expression of the rate data in common units. Accordingly, all units of rate coefficients in this section have been converted to mole.l-1.sec-1 for zeroth-order coefficients (k0), sec-1 for first-order coefficients (kt), l.mole-1.sec-1 for second-order coefficients (k2), l2.mole-2.sec-1 for third-order coefficients (fc3), etc., and consequently no further reference to units is made. Likewise, energies and enthalpies of activation are all in kcal. mole-1, and entropies of activation are in cal.deg-1mole-1. Where these latter parameters have been obtained over a temperature range which precludes the accuracy favoured by the authors, attention has been drawn to this and also to a few papers, mainly early ones, in which the units of the rate coefficients (and even the reaction orders) cannot be ascertained. In cases where a number of measurements have been made under the same conditions by the same workers, the average values of the observed rate coefficients are quoted. In many reactions much of the kinetic data has been obtained under competitive conditions such that rate coefficients are not available in these cases the relative reactivities (usually relative to benzene) are quoted. [Pg.1]

Second-order and third-order results often bracket the true correction to pF - Three schemes that scale the third-order terms in various ways are known as the Outer Valence Green s Function (OVGF) [8], In OVGF calculations, one of these three recipes is chosen as the recommended one according to rules based on numerical criteria. These criteria involve quantities that are derived from ratios of various constituent terms of the self-energy matrix elements. Average absolute errors for closed-shell molecules are somewhat larger than for P3 [31]. [Pg.139]

So by measuring the second-order Doppler shift of the Mossbauer nuclei in a material it is possible to determine their average velocity and thus their average vibrational kinetic energy, /2, where the mass of the Mossbauer nucleus. The... [Pg.91]

The analysis of Eqs (29) and (30) shows that the self-consistent treatment of the averaged part of the energy tends to minimize the second-order terms [16]. Thus we arrive to the approximate form of the SET ... [Pg.59]

In Subsections 2.2 and 2.3 it was shown that Strutinsky s energy theorem can be formulated in two different forms, Eqs (13) and (29). The first form is relevant after the first step of the SCAP (the first averaging of the HFR results) is performed, whereas the second form comes in after the final step. Actual calculations in nuclear physics [16-22] have shown that the values obtained for E[p] and E[p] are rather close. The SCAP stationarity essentially leads to the gathering of all fluctuations of the total energy in the first-order term, 5, E(e, .), minimizing the sum of the second-order terms in Eqn (29). [Pg.62]

Figure 14.17 Reduction of chlorinated ethenes (for structures see Fig. 14.15) at a nickel electrode and by two zero-valent metals [Fe(0), Zn(0)]. Decadic logarithms of the relative overall reduction rates plotted (a) against / 0.059 V (analogous to Eq. 14-38 E H values from Arnold and Roberts, 1998), and (b) against the C-Cl bond energy (DR X) divided by 2.3 RT (Dr.x values from Perlinger et al., 2000). The absolute surface-normalized second-order rate constants for PCE are 3 x 10-3 L m 2 s I (Ni-electrode at -1.0 V Liu et al., 2000), 6 x 10-7 L-nr2 s 1 (Fe(0) average value reported by Scherer et al., 1998), and 8 x 10 5 L - nr2 s 1 (Zn(0) Arnold and Roberts, 1998). Figure 14.17 Reduction of chlorinated ethenes (for structures see Fig. 14.15) at a nickel electrode and by two zero-valent metals [Fe(0), Zn(0)]. Decadic logarithms of the relative overall reduction rates plotted (a) against / 0.059 V (analogous to Eq. 14-38 E H values from Arnold and Roberts, 1998), and (b) against the C-Cl bond energy (DR X) divided by 2.3 RT (Dr.x values from Perlinger et al., 2000). The absolute surface-normalized second-order rate constants for PCE are 3 x 10-3 L m 2 s I (Ni-electrode at -1.0 V Liu et al., 2000), 6 x 10-7 L-nr2 s 1 (Fe(0) average value reported by Scherer et al., 1998), and 8 x 10 5 L - nr2 s 1 (Zn(0) Arnold and Roberts, 1998).
Another important average over the spectral density of a perturbation is the second-order perturbation energy shift30... [Pg.91]

The usefulness of spectral densities in nonequilibrium statistical mechanics, spectroscopy, and quantum mechanics is indicated in Section I. In Section II we discuss a number of known properties of spectral densities, which follow from only the form of their definitions, the equations of motion, and equilibrium properties of the system of interest. These properties, particularly the moments of spectral density, do not require an actual solution to the equations of motion, in order to be evaluated. Section III introduces methods which allow one to determine optimum error bounds for certain well-defined averages over spectral densities using only the equilibrium properties discussed in Section II. These averages have certain physical interpretations, such as the response to a damped harmonic perturbation, and the second-order perturbation energy. Finally, Section IV discusses extrapolation methods for estimating spectral densities themselves, from the equilibrium properties, combined with qualitative estimates of the way the spectral densities fall off at high frequencies. [Pg.97]


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See also in sourсe #XX -- [ Pg.264 ]




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