The Ratio Law of the Structure Evolution and Stability for TinOm (n=3-18, m=1-2n) Clusters

Abstract

Most theoretical investigations about titanium oxide clusters focus on (TiO2)n. However, many TinOm clusters with m≠ 2n are produced experimentally. In this work, first-principles calculations are performed to probe the evolution of TinOm clusters. Our investigations show that for n=3-11, there exist one relatively stable specie; while for n=12-18, there are two relatively stable species: Ti-rich and O-rich species. HOMO-LOMO calculations show that the gap can be tuned by changing the size and configurations of TinOm clusters. Our investigation provides insights into the evolution of cluster-to-bulk process in titanium oxide.

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