Defect characterization of InSb1−xNx grown using radio frequency nitrogen plasma-assisted molecular beam epitaxy

Defect characterization of InSb1−xNx grown using radio frequency nitrogen plasma-assisted molecular beam epitaxy
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DOI:
10.1088/0022-3727/41/16/165301
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发表时间:
2008-08
期刊:
Journal of Physics D: Applied Physics
影响因子:
--
通讯作者:
K. P. Lim;S. F. Yoon;H. T. Pham;S. Tripathy
K. P. Lim;S. F. Yoon;H. T. Pham;S. Tripathy
中科院分区:
其他
文献类型:
--
作者:
K. P. Lim;S. F. Yoon;H. T. Pham;S. Tripathy

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我们报道了用射频氮等离子体辅助分子束外延生长InSb 1 −xNx,并用可见波长拉曼散射和X射线衍射对其进行表征。研究了生长温度(330-420 °C)和等离子体功率(200-500 W)对N诱导缺陷的影响。Sb反位缺陷从A1 gSb模式被证明是占主导地位的,在高的生长温度和低的等离子体功率。另一方面,高的生长温度和高的等离子体功率诱导间隙Sb-N缺陷的形成。在最低衬底温度(330 °C)和等离子体功率(200 W)下观察到Sb相关缺陷的减少。根据实验结果,提出了一种可能的缺陷形成机制。
We report the growth of InSb1−xNx using radio frequency nitrogen plasma-assisted molecular beam epitaxy and its characterization using visible wavelength Raman scattering and x-ray diffraction. The effects of the growth temperature (330–420 °C) and the plasma power (200–500 W) on the N-induced defects were studied. Sb antisite defects from the A1gSb mode are shown to be dominant at a high growth temperature and a low plasma power. On the other hand, the high growth temperature and high plasma power induce the formation of interstitial Sb–N defects. A reduction in Sb related defects is observed at the lowest substrate temperature (330 °C) and plasma power (200 W). Based on the experimental results, a possible mechanism of defect formation is suggested.