Abstract
We study the melting of clusters and thin films as a mass-density-wave instability by generalizing recent density-functional methods of melting. We found that the freezing temperature is increased for thin films whereas for clusters it is decreased. For spherical boundaries, at melting the Debye-Waller factor as a function of the radial distance consists of a flat bulklike part close to the center and a decaying interface part at the surface. For small particles, the surface part dominates. This represents a type of generalized Lindemann criterion for small clusters. Our calculation also provides a detailed microscopic description of the density distribution and more physical insight about the system.

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