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Transition ensemble size

In this section, we move from the elucidation of molecular and atomic adsorption to the fundamental features that control smface reactivity. We start by initially describing dissociative adsorption processes. We focus on elucidating surface chemistry as well as the understanding of how the metal substrate influences the intrinsic surface reactivity. We will also pay attention to geometric ensemble-size related requirements. The Brpnsted-Evans Polanyi relationship between transition-state energy and reaction energy discussed in Chapter 2 is particularly useful in understanding differences in reactivity between different metal surfaces. [Pg.119]

In this section we review several studies of phase transitions in adsorbed layers. Phase transitions in adsorbed (2D) fluids and in adsorbed layers of molecules are studied with a combination of path integral Monte Carlo, Gibbs ensemble Monte Carlo (GEMC), and finite size scaling techniques. Phase diagrams of fluids with internal quantum states are analyzed. Adsorbed layers of H2 molecules at a full monolayer coverage in the /3 X /3 structure have a higher transition temperature to the disordered phase compared to the system with the heavier D2 molecules this effect is... [Pg.97]

The simulation of a first-order phase transition, especially one where the two phases have a significant difference in molecular area, can be difficult in the context of a molecular dynamics simulation some of the works already described are examples of this problem. In a molecular dynamics simulation it can be hard to see coexistence of phases, especially when the molecules are fairly complicated so that a relatively small system size is necessary. One approach to this problem, described by Siepmann et al. [369] to model the LE-G transition, is to perform Monte Carlo simulations in the Gibbs ensemble. In this approach, the two phases are simulated in two separate but coupled boxes. One of the possible MC moves is to move a molecule from one box to the other in this manner two coexisting phases may be simulated without an interface. Siepmann et al. used the chain and interface potentials described in the Karaborni et al. works [362-365] for a 15-carbon carboxylic acid (i.e. pen-tadecanoic acid) on water. They found reasonable coexistence conditions from their simulations, implying, among other things, the existence of a stable LE state in the Karaborni model, though the LE phase is substantially denser than that seen experimentally. The re-... [Pg.125]

Fig. 7.18 The radiative recombination time r as a function of the blue shift of the photon energy AE from the bulk silicon band edge zero-phonon transitions (dots) TO phonon-assisted transitions (line). This scatter plot shows the radiative time for each member of an ensemble uniformly distributed around a cubic geometry. The top scale indicates the equivalent cube size. Redrawn from [Hy2],... Fig. 7.18 The radiative recombination time r as a function of the blue shift of the photon energy AE from the bulk silicon band edge zero-phonon transitions (dots) TO phonon-assisted transitions (line). This scatter plot shows the radiative time for each member of an ensemble uniformly distributed around a cubic geometry. The top scale indicates the equivalent cube size. Redrawn from [Hy2],...
It is worth noticing that although the double-steeped isotherm may be indicative of the second-order phase transitions (as speculated in Ref. 15 for Kr in AlP04-5), they may be not for an adsorbate whose size is comparable to the nanotube diameter that behaves as a one dimensional confined fluid. MC simulations in the grand canonical ensemble (shown in full circles) fully agree with the predictions from Eq. (6). [Pg.659]

Figure 35 shows the transition temperature T and the domain size r (= 2n/q ) as a function of Ts for different N. Note that both T and r are averaged over the ensemble of generated sequences ( 106). If Ts is too high, the sequences tend to become random. In contrast, when Ts is too low, the evolutionary algorithm leads to the trivial diblock sequence. In this case, one observes a typical mean-field behavior T ex N and r oc N1/2 (for long... [Pg.68]

Canonical ensemble density functional theory (CEDFT) has been employed for predicting hysteretic adsorption/desorption isotherms in nanopores of different geometries in the wide range of pore sizes (1 - 12 nm). It is shown that the CEDFT model qualitatively describes equilibrium and spinodal transitions and is in a reasonable quantitative agreement with experiments on well-characterized MCM-41 samples. A DFT-based method for calculating pore size distributions from the adsorption and desorption branches of nitrogen adsorption isotherms has been elaborated and tested against literature data on capillary condensation in MCM-41 samples with pores from 5 to 10 nm. [Pg.51]

Abstract Transition metal carbides and phosphides have shown tremendons potential as highly active catalysts. At a microscopic level, it is not well understood how these new catalysts work. Their high activity is usually attributed to ligand or/and ensemble effects. Here, we review recent studies that examine the chemical activity of metal carbides and phosphides as a function of size, from clusters to extended surfaces, and metal/carbon or metal/phosphorous ratio. These studies reveal that the C and P sites in these compounds cannot be considered as simple spectators. They moderate the reactivity of the metal centers and provide bonding sites for adsorbates. [Pg.117]

It has been implied that the surface of the nanocrystal acts as a perturbation of the total nanocrystal free energy. The assumption has been that, from a thermodynamics viewpoint, the nanocrystal behaves merely as a fragment of the extended solid. However, evidence suggests that structure throughout a nanoparticle in very small particle size may be perturbed relative to the bulk (see chapters by Banfield and Zhang and Waychunas, this volume). Although the thermodynamic properties of the nanocrystal ensemble are well defined, structural phase transitions are rigorously defined only in an infinite medium. A lower limit must exist for the number of atoms required for the crystal in... [Pg.62]

The simulation of frustrated systems suffers from a similar tunneling problem as the simulation of first order phase transitions local minima in energy space are separated by barriers that grow with system size. While the multicanonical or optimized ensembles do not help with the NP-hard problems faced by spin glasses, they are efEcient in speeding up simulations of frustrated magnets without disorder. [Pg.608]


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Ensemble size

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