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Third-order equations particles

In Fig. 4(a) we show a typical diagram in the expansion of A3 that cannot be incorporated into any ladder-type diagram because it involves simultaneous correlation between three particles [69]. As it appears in CSE(2) and ICSE(2), however, A3 is always traced over coordinate X3, and in Fig. 4(b) we show the effect of tT3 on the diagram in Fig. 4(a). Diagram 4(b) is included in the partial trace of a third-order ladder-type diagram, namely, the one shown in Fig. 4(c). Thus the presence of tr3 in the two-particle equations allows one to incorporate three- and higher-body effects that would not otherwise be present in a ladder approximation for the three- and four-electron cumulants. [Pg.289]

In a series of works [126,132,246,247] a set of approximate solutions for the contact reactions was suggested. These solutions are based on a hierarchical system of diffusional equations for /(-particle probabilities. The truncation of this system at the second order has led to the so-called multiparticle kernel 3 (MPK3) approximation [126] the third order has given MPK2 theory [132,247], but well before the effort was mounted to truncate this system at the fourth order [246], This earliest attempt, known as MPK1, turned out to be the best for the reversible dissociation/association reaction. It correctly reduces to the limits available for strict investigation ... [Pg.372]

Obviously, those are the same considerations as we went through in order to obtain Eqs (90) and (91) and the electron propagator method and the ADC are thus equivalent methods. Using n = 2 in Eq. (93) we determine and n — 3 gives The U matrix in Eq. (93) corresponds to the transition matrix (cf. Eq. (75)). Both and only contain C and D terms (see Eqs (87), (88), (90) and (91), i.e. hj = hj alone. From Eq. (63) we see that we may classify the operators in hj as 2p-lh (two-particle, one-hole) and 2h-lp operators, and the n = 3 ADC approach, corresponding to the third-order electron propagator method, is therefore referred to as the extended 2p-lh Tamm-Dancoff approximation (TDA) (Walter and Schirmer, 1981). A fourth-order approximation to the ADC equations has also been described (Schirmer et ai, 1983) but not yet tested in actual applications. [Pg.218]

The two-particle nature of Coulomb interaction in equation (10.27) is the reason that among the third-order contributions to the transition amplitude, in addition to one particle effective operators (as in the standard J-O approach), two particle objects are also present. However, the numerical analysis based on ab initio calculations performed for all lanthanide ions, applying the radial integrals evaluated for complete radial basis sets (due to perturbed function approach), demonstrated that the contributions due to two-particle effective operators are relatively negligible [11,44-58]. This is why here they are not presented in an explicit tensorial form (see for example Chapter 17 in [13]). At the same time it should be pointed out that two-particle effective operators, as the only non-vanishing terms, play an important role in determining the amplitude of transitions that are forbidden by the selection rules of second- and the third-order approaches. This is the only possibility, at least within the non-relativistic model, to describe the so-called special transitions like, 0 <—> 0 in Eu +, for example, as discussed above. [Pg.259]

Note that Equation (9) implies that the square of the standard deviation a2 is the second moment of d relative to the mean d. Higher order moments can be used to represent additional information about the shape of a distribution. For example, the third moment is a measure of the skewness or lopsidedness of a distribution. It equals zero for symmetrical distributions and is positive or negative, depending on whether a distribution contains a higher proportion of particles larger or smaller, respectively, than the mean. The fourth moment (called kurtosis) purportedly measures peakedness, but this quantity is of questionable value. [Pg.633]

Second-Order Moment. The linearity of y U /2L vs. l/t/B2 is shown in Figure 4. From the slope of the straight line, the axial dispersion coefficient D can be calculated. With the assumption that kR = Z)Ab, Da and Di can be calculated from the second and third terms in the bracket of the right-hand side of Equation 6 by varying the particle size. The results are given in Table II. As expected, both inter- and intracrystalline diffusion coefficients increase with temperature. The values obtained for Di in Na mordenite are somewhat smaller than those obtained by Satterfield and Frabetti (7) and Satterfield and Margetts (8) which were obtained at a lower temperature. However, Frabetti reported that diffusion co-... [Pg.399]

To obtain the temporal evolution of this virtual distribution (defined by the left hand side of this equation) we must analyse in which way it can be created and annihilated. The first term on the right hand site describes the creation due to an A-adsorption event. It can be annihilated by a direct (second term) and by indirect reaction events (third and fourth terms). The factor of 2/4 in the second term on the right hand side of the equation written above comes from the fact that here there are two possibilities to annihilate the A particle. The events written on the right hand side are all possibilities to create or annihilate this virtual distribution. Now we list all other virtual distributions which affect the temporal evolution of the AB pairs (equation (9.1.51)). With the help of all the virtual distributions we are able to express all virtual distributions through normal ones in equation (9.1.51). To this end we list all virtual distributions which affect the evolution of ab and solve it as a set of linear equations for the virtual distributions. The solution will be inserted in equation (9.1.51) in order to obtain an exact and handable equation. First, we study other virtual distributions with an A particle in the center and B particles in the neighbourhood. They are formed by A-adsorption in an appropriate configuration of B particles. In the last equation the A particle has two B particles as its neighbours. Now we write... [Pg.532]


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See also in sourсe #XX -- [ Pg.454 , Pg.455 , Pg.456 ]




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