Recently, stoichiometric II-VI nanoparticles with structures that are very different than the bulk crystalline structure of these materials have been identified by mass spectroscopy. The mass spectroscopy studies indicate that ultra-stable stoichiometric clusters containing 13, 33, or 34 atoms of each element can be formed. These are referred to as “magic-size clusters” (MSCs) and are believed to have a closed-cage structure that eliminates surface dangling bonds. Our objective is to analyze the relative stability of such II-VI clusters and to gain a fundamental understanding of the structure, energetics, and morphology of these intersting nanoparticles.
In this work, we focus on a detailed analysis of the stability, structure, and formation energetics of (ZnSe)n and (CdSe)n (n = 1-30) clusters. In our study, we have employed a variant of simulated annealing based on first-principles density functional theory (DFT) calculations for the corresponding energy computations. The simulated annealing variant uses a standard Metropolis Monte Carlo (MC) algorithm for geometry optimization in search of global energy minima. The DFT calculations are carried out within the generalized gradient approximation and employ plane-wave basis sets, ultra-soft pseudopotentials, and supercell models; our calculational scheme was thoroughly tested in computations of bulk ZnSe and CdSe structures.
Following this computational method, we have obtained the lowest-energy clusters for both (ZnSe)n and (CdSe)n nanostructures, with a size “n” varying over the range 1-30. Based on the formation energetics of these clusters, we have analyzed their relative stability and investigated the existence and exceptional stability of MSCs. Our calculations reveal that MSCs are cage-like structures, analogous to fullerenes, and that they correspond to the most stable (ZnSe)n and (CdSe)n nanostructures. Clusters of smaller sizes (n = 1-4) are found to have planar geometries and may serve as building blocks for larger-size clusters.
In addition to studying the stability of the MSCs, we have analyzed cluster-cluster interactions and cluster coalescence. Our theoretical analysis reveals that smaller clusters, owing to a large surface-to-volume ratio, can coalesce and form an MSC through an exothermic reaction. The energy released during the reaction is due to the minimization of the unsaturated surface bonds. A better understanding of the structure and stability of MSCs can allow the development of synthesis techniques for preparing these materials. A new class of cluster-based materials is also envisioned with II-VI MSCs as the bulding blocks. Such materials are expected to have unique optoelectronic and mechanical properties.