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Clusters empty

FIG. 13 Snapshot configuration of the catalyst surface obtained for the ZGB model with local reconstructions using lattices and patches of side L = 129 and Lp = 3, respectively, and taking 7 = 0.331 and = 0. B species , A species. Empty sites are left white. Notice the formation of clusters of both species surrounded by empty sites. [Pg.411]

Parts of the tank were projected to distances up to 360 m (1200 ft). Twenty-two pieces of the tank were recovered, constituting approximately 80% of the original tank. Debris was found clustered in two separate areas, namely, within the radii of 5° to 20° and 65° to 95° from the car s direction of movement. Three empty tank cars located up to a distance of three railroad tracks from the exploded car were blown from the rails. The undercarriage of the car was bent into a V-shape (see Figure 2.1). One person was killed in the explosion. Analysis of a recovered piece of the tank car showed that failure was due to brittle fracture. [Pg.27]

Figure 2.14. The molecular orbitals of gas phase carbon monoxide, (a) Energy diagram indicating how the molecular orbitals arise from the combination of atomic orbitals of carbon (C) and oxygen (O). Conventional arrows are used to indicate the spin orientations of electrons in the occupied orbitals. Asterisks denote antibonding molecular orbitals, (b) Spatial distributions of key orbitals involved in the chemisorption of carbon monoxide. Barring indicates empty orbitals.5 (c) Electronic configurations of CO and NO in vacuum as compared to the density of states of a Pt(lll) cluster.11 Reprinted from ref. 11 with permission from Elsevier Science. Figure 2.14. The molecular orbitals of gas phase carbon monoxide, (a) Energy diagram indicating how the molecular orbitals arise from the combination of atomic orbitals of carbon (C) and oxygen (O). Conventional arrows are used to indicate the spin orientations of electrons in the occupied orbitals. Asterisks denote antibonding molecular orbitals, (b) Spatial distributions of key orbitals involved in the chemisorption of carbon monoxide. Barring indicates empty orbitals.5 (c) Electronic configurations of CO and NO in vacuum as compared to the density of states of a Pt(lll) cluster.11 Reprinted from ref. 11 with permission from Elsevier Science.
Fig 28. Vanadium borophosphates with the composition [(VO)2BP20io] n form cage-like cluster anions, which may be empty (107, n = 4) or centered by a cation (109, n = 6). For clarity only half of the vanadium and phosphorus atoms of the cluster anions are shown... [Pg.31]

Accepting that the electronic structure of the metal clusters is in between the discreet electronic levels of the isolated atoms and the band structure of the metals, it is expectable that under a certain size the particle becomes nonmetallic. Indeed, theoretical estimations [102,105] suggest that the gap between the filled and empty electron states becomes comparable with the energy of the thermal excitations in clusters smaller than 50-100 atoms or 1 nm in size, where the particles start to behave as insulators. A... [Pg.89]

Figure 4. Cross-sectional bright-field TEM views of Au-implanted silica samples at 3 x lO Au /cm, 190 keV, aimealed for 1 h at (a) 400 °C in air, (b) 700 °C in air, (c) 900 °C in air, and (d) 900 °C in Ar, respectively (e) the histograms of the size distribution of the samples annealed 1 h in air at different temperatures (f) Arrhenius plot of the squared average cluster radius after 1 h annealing in air (filled circles) or argon (empty triangles). Solid lines are linear fit to the experimental data. Figure 4. Cross-sectional bright-field TEM views of Au-implanted silica samples at 3 x lO Au /cm, 190 keV, aimealed for 1 h at (a) 400 °C in air, (b) 700 °C in air, (c) 900 °C in air, and (d) 900 °C in Ar, respectively (e) the histograms of the size distribution of the samples annealed 1 h in air at different temperatures (f) Arrhenius plot of the squared average cluster radius after 1 h annealing in air (filled circles) or argon (empty triangles). Solid lines are linear fit to the experimental data.
Figure 7. Optical absorption spectra of Au-implanted silica samples atmealed in air (a) or Ar (b) for 1 h at different temperatures, (c) Nonlinear fit (empty circles) to the optical absorption spectrum of the sample annealed at 900 °C in air, from which the average cluster diameter is obtained and compared to the TEM measured one, (d) Evolution of the optical spectra of Au-... Figure 7. Optical absorption spectra of Au-implanted silica samples atmealed in air (a) or Ar (b) for 1 h at different temperatures, (c) Nonlinear fit (empty circles) to the optical absorption spectrum of the sample annealed at 900 °C in air, from which the average cluster diameter is obtained and compared to the TEM measured one, (d) Evolution of the optical spectra of Au-...
Geometrically illustrated, clusters are continuous regions of a highdimensional space, each of them containing a relatively high density of points (e.g., objects), separated from each other by regions that are relatively empty (low density of points). The belonging of points (objects) to... [Pg.256]

Cu atoms at each of the four empty tetrahedral positions. A comer from each of these clusters form the comers of a central tetrahedron. Thus the Cu atoms form a cluster of clusters as in Figure 8.2b. [Pg.106]

Fig. 32. Hydrogen (empty circle) adsorption on Ni clusters, (1) (111) surface (2) (100) surface (5) (110) surface (4) (111) surface hole (5) (100) surface hole. Fig. 32. Hydrogen (empty circle) adsorption on Ni clusters, (1) (111) surface (2) (100) surface (5) (110) surface (4) (111) surface hole (5) (100) surface hole.
Fig. 1. Plot of Ca, Mg and Na ratios over Fe in Fornax GC (filled symbols) and Fornax field (empty squares) [2] stars. We show data for individual stars in cluster 1 (triangles), cluster 2 (circles) and cluster 3 (diamonds). The other points comes from 2 review papers, the small dots are galactic stars from [3] and the small open circles are Galactic GCs, from [4]. The asterisk are M15 stars, our reference cluster. Fig. 1. Plot of Ca, Mg and Na ratios over Fe in Fornax GC (filled symbols) and Fornax field (empty squares) [2] stars. We show data for individual stars in cluster 1 (triangles), cluster 2 (circles) and cluster 3 (diamonds). The other points comes from 2 review papers, the small dots are galactic stars from [3] and the small open circles are Galactic GCs, from [4]. The asterisk are M15 stars, our reference cluster.
The most stable cluster consists of an aggregation of four cation vacancies in a tetrahedral geometry surrounding an Fe3+ ion, called a 4 1 cluster. Cations in the sodium chloride structure normally occupy octahedral sites in which each metal is coordinated to six nonmetal atoms. The central Fe3+ ion in the 4 1 cluster is displaced into a normally unoccupied tetrahedral site in which the cation is coordinated to four oxygen ions. Because tetrahedral sites in the sodium chloride structure are normally empty, the Fe3+ is in an interstitial site. Equation (4.1) can now be written correctly as... [Pg.150]

Figure 4.8 Structure of a Willis 2 2 2 structure (a) an empty Og cube (b) the stacking of four Og cubes in the UO2 structure (c) an Og cube containing a < 111 > interstitial oxygen ion (1d) an Og cube containing a < 110> interstitial oxygen ion and (e) the 2 2 2 cluster. Figure 4.8 Structure of a Willis 2 2 2 structure (a) an empty Og cube (b) the stacking of four Og cubes in the UO2 structure (c) an Og cube containing a < 111 > interstitial oxygen ion (1d) an Og cube containing a < 110> interstitial oxygen ion and (e) the 2 2 2 cluster.

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Condensed Empty Clusters

Emptiness

Empty

Halides empty clusters

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