Biju K P, Subrahmanyam A, Jain Mahveer K
Department of Physics, IIT Madras, Chennai 600036, India.
J Nanosci Nanotechnol. 2009 Sep;9(9):5208-13. doi: 10.1166/jnn.2009.1123.
InN films are grown on silicon and glass substrates by radio frequency (rf) activated reactive evaporation. High purity indium (99.99) is evaporated by resistive heating in the presence of nitrogen plasma. X-ray diffraction shows that the film deposited at low rf plasma powers (< or =100 W) are indium rich and further increase in the rf power formation of InN take place. The average crystallite size was found varying from 8 nm to 20 nm as the power increases from 200 to 400 W. The diffraction pattern shows the polycrystalline nature of InN films. The band gap obtained from the transmission spectra show an increase in the band gap with the increase in rf power which can be attributed to variation of nitrogen: indium stoichiometry. The Raman spectra shows wurtzite nature of the film and the photoluminescence measurements show a weak peak around 1.81 eV for the film grown at 400 W. Plasma diagnostics has been carried out in order to understand the role of active species in the process. The large shift in the band gap is attributed to Moss-Burstein shift and presence of residual oxygen in the film.
通过射频(rf)激活反应蒸发在硅和玻璃衬底上生长氮化铟(InN)薄膜。在氮等离子体存在下,通过电阻加热蒸发高纯度铟(99.99)。X射线衍射表明,在低射频等离子体功率(≤100W)下沉积的薄膜富含铟,并且随着射频功率的进一步增加会形成氮化铟。随着功率从200W增加到400W,平均微晶尺寸从8nm变化到20nm。衍射图谱显示了InN薄膜的多晶性质。从透射光谱获得的带隙显示,随着射频功率的增加带隙增大,这可归因于氮:铟化学计量比的变化。拉曼光谱显示薄膜具有纤锌矿结构,光致发光测量表明,对于在400W下生长的薄膜,在1.81eV左右有一个弱峰。为了了解活性物种在该过程中的作用,进行了等离子体诊断。带隙的大幅移动归因于莫斯 - 伯斯坦位移和薄膜中残余氧的存在。