...
首页> 外文期刊>Journal of Crystal Growth >Visible emissions near 1.9-2.2 eV from hexagonal InN films grown by electron cyclotron resonance plasma-assisted molecular-beam epitaxy
【24h】

Visible emissions near 1.9-2.2 eV from hexagonal InN films grown by electron cyclotron resonance plasma-assisted molecular-beam epitaxy

机译:电子回旋共振等离子体辅助分子束外延生长的六方InN薄膜的可见发射接近1.9-2.2 eV

获取原文
获取原文并翻译 | 示例
           

摘要

We have investigated the influence of residual oxygen (O) atoms and In2O3 grains included in 200-nm-thick hexagonal (alpha)-InN crystalline films grown on Si (1 1 1) substrates. (1 1 1)-oriented cubic (beta)-In2O3 crystal grains were formed from O atoms in In droplets adhering to the film surface, and from residual O atoms in the film when the samples were annealed at 500degreesC in a N-2 atmosphere after growth. The samples exhibited relatively strong and uniform orange photoluminescence (PL) emissions on the whole surface when using a 325nm He-Cd laser excitation. The emission consisted of two broad bands at approximately 1.9 and 2.0 eV, however no PL emissions were observed when using a 514.5 nm Ar+ ion laser. beta-In2O3, formed from residual O atoms in the film, was also detected following post-growth annealing after In droplets were removed by HCl etching. It is shown that the residual O concentration in the as-grown film can be qualitatively estimated from the orange peaks in the PL spectra. It is suggested that the origin of the localized yellow emissions observed at 2.2 eV under a 514.5 nm Ar+ ion laser excitation for as-grown InN films, as reported previously [Phys. Stat. Sol. B 228 (2001) 21; Appl. Phys. Lett. 80 (2002) 968], is not beta-In2O3 crystal grains although it is closely related to the residual O concentration. (C) 2004 Elsevier B.V. All rights reserved.
机译:我们已经研究了在Si(1 1 1)衬底上生长的200 nm厚的六边形(alpha)-InN晶体膜中包括的残余氧(O)原子和In2O3晶粒的影响。当样品在N-2气氛中于500°C退火时,由In液滴中的O原子和薄膜中的残留O原子形成(1 1 1)取向的立方β-In2O3晶粒。成长之后。当使用325nm He-Cd激光激发时,样品在整个表面上表现出相对较强且均匀的橙色光致发光(PL)发射。发射光由大约1.9和2.0 eV的两个宽带组成,但是当使用514.5 nm Ar +离子激光器时,未观察到PL发射光。在通过HCl蚀刻去除In小滴后,在生长后退火之后,还检测到了由膜中残留O原子形成的β-In2O3。结果表明,可以从PL光谱中的橙色峰定性地估计成膜后的残留O浓度。如先前所报道,建议在生长的InN膜上,在514.5 nm Ar +离子激光激发下,在2.2 eV处观察到的局部黄色发射的起源[Phys。统计索尔B 228(2001)21;应用物理来吧80(2002)968]不是β-In2 O 3晶粒,尽管它与残余的O浓度密切相关。 (C)2004 Elsevier B.V.保留所有权利。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号