Department of Applied Physics, National Defense Academy, Yokosuka 239-8686, Japan.
J Phys Condens Matter. 2010 Oct 13;22(40):404204. doi: 10.1088/0953-8984/22/40/404204. Epub 2010 Sep 22.
The structures of phase-change In(0.21)Sb(0.79) thin film in the amorphous phase were modeled using the reverse Monte Carlo (RMC) method, making simultaneous use of measured x-ray diffraction and x-ray absorption fine structure data. The experimental data that we used do not contain the crystalline phase, which can be observed in the diffraction pattern. Three kinds of initial configurations--a simple cubic lattice, a rhombohedral A7 structure and a dense randomly packed hard sphere form--were used in attempts to reproduce the measured data. The former configuration is thought to be the most probable structure for the crystalline In(0.21)Sb(0.79) thin film. For the latter configuration we could not reproduce the structure of the amorphous In(0.21)Sb(0.79) thin film under the present RMC conditions. We obtained probable structure models for the amorphous In(0.21)Sb(0.79) thin film. We found that the models obtained possess some traces of crystallinity.
采用反蒙特卡罗(RMC)方法,利用测量的 X 射线衍射和 X 射线吸收精细结构数据,对非晶相中的相变 In(0.21)Sb(0.79) 薄膜的结构进行了建模。我们使用的实验数据不含晶相,而晶相可在衍射图中观察到。尝试使用了三种初始构型——简单立方晶格、三方 A7 结构和密堆积硬球形式——来重现测量数据。前一种构型被认为是晶态 In(0.21)Sb(0.79) 薄膜最可能的结构。对于后一种构型,我们无法在当前的 RMC 条件下重现非晶态 In(0.21)Sb(0.79) 薄膜的结构。我们得到了非晶态 In(0.21)Sb(0.79) 薄膜的可能结构模型。我们发现,得到的模型具有一些结晶的痕迹。