用MBE法在硅基光源上制备高拉伸应变锗量子点

Zhenpu Zhang, Yuxin Song, Qimiao Chen, Q. Gong, Shumin Wang
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引用次数: 0

摘要

理论上预测,高达1.4%的双轴拉伸应变可以弥补Ge[1]中Γ与L谷之间136mev的间隙,从而将Ge从间接带隙半导体转变为直接带隙半导体,可以有效地发射覆盖电信频段的光。两种载体的机动性同时显著提高。因此,拉伸应变锗在高速晶体管和硅光子学光源方面的潜力引起了人们的极大兴趣。我们提出并证明了InP上的拉伸应变Ge量子点(QD)是在Si上实现光源比薄膜更好的解决方案,因为它可以承受大的应变来转换带隙,同时对结构缺陷不敏感[2]。本文研究了厚度从亚单层(ML)到几层(ML)的GaSb(001)上的拉伸应变锗量子点的分子束外延。利用反射高能电子衍射(RHEED)研究了沉积的锗量子点的形成和演化,并用原子力显微镜(AFM)测量了表面形貌。图1显示,在1.7 ML的Ge沉积后,RHEED模式转变为点状模式,表明存在湿润层的Stranski-Krastanov (SK)生长模式。图2为不同锗厚度样品的AFM图像。可以发现,当厚度小于1 ML时,Ge原子在GaSb原子台阶上随机成核,形成亚ML岛。二维增长继续完全覆盖GaSb表面,达到1.7 ML。在1 ML之前可以发现一些量子点,可能是由于表面缺陷。这些亚ML岛和1 ML厚的Ge膜完全应变(拉伸应变为7.2%)。当厚度大于1.7 ML时,可以观察到清晰的量子点形成。量子点多为矩形,边缘沿(110)方向排列。从RHEED和AFM观察到的演变是一致的。随后,还生长了不同厚度的Ge样品,并加盖了GaSb。包括光学性质在内的进一步分析正在进行中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Highly tensile-strained Ge quantum dots on GaSb by MBE for light sources on Si
It is theoretically predicted that biaxial tensile strain as much as 1.4% can make up the 136 meV gap between the Γ and L valley in Ge [1], thereby converting Ge from an indirect-bandgap semiconductor into a direct-bandgap one that can emit light efficiently covering the telecom band. The mobility of both carriers is dramatically increased simultaneously. Therefore, tensile-strained Ge has drawn large interest in the potential for high speed transistors and light sources for Si photonics. We have proposed and demonstrated that tensile-strained Ge quantum dot (QD) on InP is a better solution for the realization of light sources on Si than thin films since it can hold large strain to convert the bandgap and insensitive to structural defects at the same time [2]. In this work, the molecular beam epitaxy (MBE) of tensile-strained Ge QDs on GaSb(001) with thickness ranging from sub-monolayer (ML) to a few MLs is studied. The formation and evolution of the deposited Ge QDs are investigated by the reflection high-energy electron diffraction (RHEED), and the surface morphology is measured by atomic force microscopy (AFM). In FIG. 1, it is shown that the RHEED pattern changed to a dotty one after 1.7 ML of the Ge deposition indicating a Stranski-Krastanov (SK) growth mode with the existence of a wetting layer. FIG. 2 are AFM images of the samples with different Ge thickness. It can be found that when the thickness is below one ML, the Ge atoms nucleate randomly on the GaSb atomic steps, forming sub-ML islands. The two dimensional growth continues to a full coverage of the GaSb surface and up to 1.7 ML. A few QDs can be found before 1 ML, probably due to surface defects. These sub-ML islands and the one ML thick Ge films are fully strained (7.2% tensile strain). When the thickness is larger than 1.7 ML, clear formation of QDs is observed. The QDs are mostly rectangular shape with the edges along the (110) directions. The evolution observed from RHEED and AFM is consistent. Later, samples of the Ge with different thicknesses capped by GaSb were also grown. Further analysis including optical properties are under implement.
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