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Binding energies, calculations

From the binding energies calculated for the different cluster compositions, we determined abundance mass spectra for heated CggLi clusters from a simple Monte Carlo simulation. Figure 11 shows the simulated mass spectra resulting from these calculations, including the Li and Cgo isotope distributions. The peaks at A = 12 and at x = 6 + n (where n is the cluster charge) observed in the experiment (Fig. 9) are well reproduced. For more details, see ref. [12]. [Pg.176]

Table of Relativistically Corrected Core Electron Binding Energies Calculated Using the AE s(PW86 - PW91) + Qei Method. [Pg.295]

J. Shen and J. Wendoloski, Electrostatic binding energy calculation using the finite... [Pg.222]

Figure 9.14 Correlation between binding energy calculated using MMFFsl b] and measured Ki for a diverse set of ligands in P3 pocket. Figure 9.14 Correlation between binding energy calculated using MMFFsl b] and measured Ki for a diverse set of ligands in P3 pocket.
The calculated gain of energy equivalent to the loss of mass is called the binding energy of the atom (or nucleus, if it is being considered independently of the electrons in the shells). When the binding energy calculations are... [Pg.362]

Figure 8-7. A. Binding energy (AEMP2, circles, and AEel, squares) as a function of inhibitory activity for the model comprising LAP active site residues. Numbers of particular points correspond to inhibitors designation introduced in right panel. B. Structures of LAP inhibitors included into binding energy calculations presented in left panel... Figure 8-7. A. Binding energy (AEMP2, circles, and AEel, squares) as a function of inhibitory activity for the model comprising LAP active site residues. Numbers of particular points correspond to inhibitors designation introduced in right panel. B. Structures of LAP inhibitors included into binding energy calculations presented in left panel...
A linear correlation was found288 between experimental proton affinities and inner-shell Is electron binding energies calculated by the semi-empirical CNDO/2 method289 within a homologous series of amines. [Pg.54]

Table 3.5. Comparison of metal-water bond lengths and binding energies calculated using (SCF) Hartree-Fock-Roothaan methods with... Table 3.5. Comparison of metal-water bond lengths and binding energies calculated using (SCF) Hartree-Fock-Roothaan methods with...
The selection of additives can be guided by molecular visualizations of the crystal structure based on geometric fits ° or binding energy calculations. ... [Pg.849]

Margrave and Sthapitanonda (1 ) report estimated dissociation energies in the range 111-178 kcal mol" based on approximate ionic binding energies calculated from ionic radii for N" in the range 0.70 to 1.08 A. [Pg.1435]

To further speed up this approach, one can replace the expensive explicit-solvent simulations with implicit ones. Statistical mechanical theory gives the Helmholtz free energy A, apart from the scaling constant of the classical partition function that cancels out in binding energy calculations, as... [Pg.37]

Fig. 5.7. Binding energies, calculated by DFT-GGA, for oxygen at Ru(OOOl). Coverages with < 1 ML correspond to pure on-surface adsorption (hep or fee site). For > IML an 0(1 x 1) arrangement is always present at the surface, cf. Fig. 5.5, while the remaining O is located in either of the three interstitial sites between the first and second substrate layer. From the six possible structures at each coverage, the three with on-surface O in hep (fee) sites are drawn with thicker (thinner) lines (from [22])... Fig. 5.7. Binding energies, calculated by DFT-GGA, for oxygen at Ru(OOOl). Coverages with < 1 ML correspond to pure on-surface adsorption (hep or fee site). For > IML an 0(1 x 1) arrangement is always present at the surface, cf. Fig. 5.5, while the remaining O is located in either of the three interstitial sites between the first and second substrate layer. From the six possible structures at each coverage, the three with on-surface O in hep (fee) sites are drawn with thicker (thinner) lines (from [22])...

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