1987
DOI: 10.1063/1.453602
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Rare gas clusters: Solids, liquids, slush, and magic numbers

Abstract: Simulations by constant energy molecular dynamics have been performed for numerous clusters in the size range N=7–33. Detailed investigations have been conducted on the portions of the caloric curves in which the transition between rigid and nonrigid behavior occurs, to study the N dependence of the solid–liquid phase change. Clusters of several sizes display a coexistence of forms, each with a characteristic mean temperature, over a well-defined energy range in the transition region, as had been observed for … Show more

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Cited by 328 publications
(143 citation statements)
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“…There has been some controversy concerning the dependence of the simulated thermodynamic properties on the ensemble until the work by Calvo and Labastie [17]. These authors [17] showed that if the sampling of the phase space is accurate enough (a large enough number of MC configurations and MD trajectories), the thermodynamic results are identical in both ensembles because the thermodynamics is determined by the configurational density of states [7,8,17,18].In this Letter, we show that the potential energy distribution of atoms in the clusters can consistently explain many of the important phenomena which occur during phase changes of small clusters, such as the nonmonotonic variation of melting temperature with the size of clusters [3,6,7], the dependence of melting, boiling, and sublimation temperatures on the interatomic potentials [12,13,19], the existence of a surface-melted phase [6,8,11,15,16], and the absence of a premelting peak in heat capacity curves [9,[14][15][16].We have studied the thermodynamic behavior of clusters of metals and nonmetals for the sizes of 12 # n # 34. For the interatomic interactions, we have employed the tight-binding potentials based on the second moment approximation [7,16] for metal clusters (M n , M Ni, Cu, Pd, Ag, Pt, Au, Al, and Pb) and pair potentials for nonmetal clusters.…”
mentioning
confidence: 66%
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“…There has been some controversy concerning the dependence of the simulated thermodynamic properties on the ensemble until the work by Calvo and Labastie [17]. These authors [17] showed that if the sampling of the phase space is accurate enough (a large enough number of MC configurations and MD trajectories), the thermodynamic results are identical in both ensembles because the thermodynamics is determined by the configurational density of states [7,8,17,18].In this Letter, we show that the potential energy distribution of atoms in the clusters can consistently explain many of the important phenomena which occur during phase changes of small clusters, such as the nonmonotonic variation of melting temperature with the size of clusters [3,6,7], the dependence of melting, boiling, and sublimation temperatures on the interatomic potentials [12,13,19], the existence of a surface-melted phase [6,8,11,15,16], and the absence of a premelting peak in heat capacity curves [9,[14][15][16].We have studied the thermodynamic behavior of clusters of metals and nonmetals for the sizes of 12 # n # 34. For the interatomic interactions, we have employed the tight-binding potentials based on the second moment approximation [7,16] for metal clusters (M n , M Ni, Cu, Pd, Ag, Pt, Au, Al, and Pb) and pair potentials for nonmetal clusters.…”
mentioning
confidence: 66%
“…As the cluster size decreases, the melting temperature monotonically decreases [4,5]. However, when the cluster size is small enough (# 200 atoms), the melting temperature does not vary monotonically with the size of cluster [3,6,7].…”
Section: (Received 28 July 2000)mentioning
confidence: 99%
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