星团(航天器)
钽
成核
材料科学
分子动力学
结晶学
晶体结构
化学物理
构造形成
化学
物理
热力学
计算化学
冶金
银河系
量子力学
程序设计语言
计算机科学
作者
Aiqin Jiang,Trevor A. Tyson,Lisa Axe
标识
DOI:10.1088/0953-8984/17/39/001
摘要
The structure of small tantalum clusters is investigated by using molecular dynamics simulations. A structural evolution from polytetrahedral structures to layered Frank–Kasper-type structures is revealed as cluster size increases to N∼100 atoms. The lowest-energy structures have been located for clusters with N≤78. The bulk-like (bcc) structure becomes the most stable structure beyond N∼100. The stabilized structure strongly depends on the cooling rate. A structure similar to β-Ta, a σ-type Frank–Kasper structure, can be obtained by rapid cooling. The structural properties of small Ta clusters presented in the paper provide insight into the formation and origin of β-phase Ta. The growth of β-Ta films in practice may be due to the nucleation of Ta clusters with layered Frank–Kasper-type structure during the initial stage of film growth.
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