蓝宝石衬底上GaN/AlxGa1-xN超晶格插入层对AlxGa1-xN外延薄膜应变及缺陷密度的影响

室温300K下,由于Al_xGa_1-xN的带隙宽度可以从GaN的3.42eV到AlN的6.2eV之间变化,所以Al_xGa_1-xN是紫外光探测器和深紫外LED所必需的外延材料.高质量高铝组分Al_xGa_1-xN材料生长的一大困难就是Al_xGa_1-xN与常用的蓝宝石衬底之间大的晶格失配和热失配.因而采用MOCVD在GaN/蓝宝石上生长的Al_xGa_1-xN薄膜由于受张应力作用非常容易发生龟裂.GaN/Al_xGa_1-xN超晶格插入层技术是释放应力和减少Al_xGa_1-xN薄膜中缺陷的有效方法.研究了GaN/Al_xGa_1-xN超晶格插入层对GaN/蓝宝石上Al_xGa_1-xN外延薄膜应变状态和缺陷密度的影响.通过拉曼散射探测声子频率从而得到材料中的残余应力是一种简便常用的方法,Al_xGa_1-xN外延薄膜的应变状态可通过拉曼光谱测量得到.Al_xGa_1-xN外延薄膜的缺陷密度通过测量X射线衍射得到.对于具有相同阱垒厚度的超晶格,例如4nm/4nm,5nm/5nm,8nm/8nm的GaN/Al_0.3Ga_0.7N超晶格,研究发现随着超晶格周期厚度的增加Al_xGa_1-xN外延薄膜缺陷密度降低,Al_xGa_1-xN外延薄膜处于张应变状态,且5nm/5nmGaN/Al_0.3Ga_0.7N超晶格插入层Al_xGa_1-xN外延薄膜的张应变最小.在保持5nm阱宽不变的情况下,将垒宽增大到8nm,即十个周期的5nm/8nmGaN/Al_0.3Ga_0.7N超晶格插入层使Al_xGa_1-xN外延层应变状态由张应变变为压应变.由X射线衍射结果计算了Al_xGa_1-xN外延薄膜的刃型位错和螺型位错密度,结果表明超晶格插入层对螺型位错和刃型位错都有一定的抑制效果.透射电镜图像表明超晶格插入层使位错发生合并、转向或是使位错终止,且5nm/8nmGaN/Al_0.3Ga_0.7N超晶格插入层导致Al_xGa_1-xN外延薄膜中的刃型位错倾斜30°左右,释放一部分压应变.     

晶格匹配InAs/AlSb超晶格材料的分子束外延生长研究

InAs/GaSb超晶格是量子级联激光器(quantum cascade lase,QCL)和带间级联激光器(interband cascade lasers,ICL)结构中重要的组成,特别是作为ICL的上下超晶格波导层是由大量的超薄外延层(纳米量级)交替生长而成,细微的晶格失配便会直接导致材料晶体质量变差,而且每层的厚度和组分变化会强烈影响材料结构性能.论文研究验证了InAs/GaSb超晶格材料生长的最佳温度约在420℃.通过在衬底旋转的情况下生长40周期短周期GaSb/AlSb和InAs/GaSb超晶格,并采用XRD测量拟合获得了GaSb和AlSb层厚分别为5.448 nm和3.921 nm,以及InAs和GaSb层厚分别为8.998 nm和13.77 nm,误差在10%以内,获得了InAs/AlSb超晶格的生长最优条件.在GaSb衬底上生长晶格匹配的40周期的InAs/AlSb超晶格波导层,充分考虑飘逸As注入对InAs/AlSb超晶格平均晶格常数的影响,在固定SOAK时间为3 s的条件下,通过变化As压为1.7×10^-6 mbar来调整个超晶格的平均晶格常...     

ZnSe-ZnS超晶格的通光蚀孔及列阵研究

用MOCVD方法在GaAs衬底上生长ZnSe-ZnS超晶格.用化学腐蚀方法在GaAs衬底上开一个通光窗口,使该窗口上仅剩有1～1.8μm厚的生长层.室温下测量了蚀孔后由于化学腐蚀造成生长层表面差异的ZnSe-ZnS超晶格的吸收光谱.研究了带有生长过渡层和无过渡层的超晶格质量对其吸收光谱性能的影响.发现过渡层的存在保护了超晶格激子吸收性能.在此基础上首次采用新工艺在3×3mm2面积上把GaAs衬底金部腐蚀掉,剩下均匀、光滑的ZnSe-ZnS超晶格层,在其上做出了300×300μm2的列阵,为在ZnSe-ZnS超晶格上实现光学双稳的集成化提供了必要条件.     

低压MOCVD生长参量对Ⅱ型InAs/GaSb超晶格材料表面形貌的影响

采用自制低压金属有机源化学气相沉积设备,在(100)面GaSb单晶衬底上生长了Ⅱ型InAs/GaSb超晶格材料.利用双晶X射线衍射、光学显微镜、原子力显微镜和光致发光谱等分析手段对材料特性进行了表征,获得了表面光亮的晶体质量较好的Ⅱ型InAs/GaSb超晶格材料,在77 K下得到光致发光谱峰值波长为3.25 μm.研究了生长温度、过渡层、界面层对其表面形貌的影响,得出生长温度在500 ℃～520 ℃,无过渡层,使用InAsSb界面层有利于改善材料的表面形貌.     

低压MOCVD生长参量对Ⅱ型InAs/GaSb超晶格材料表面形貌的影响

采用自制低压金属有机源化学气相沉积设备,在（100）面GaSb单晶衬底上生长了Ⅱ型InAs/GaSb超晶格材料.利用双晶X射线衍射、光学显微镜、原子力显微镜和光致发光谱等分析手段对材料特性进行了表征,获得了表面光亮的晶体质量较好的Ⅱ型InAs/GaSb超晶格材料,在77 K下得到光致发光谱峰值波长为3.25 μm.研究了生长温度、过渡层、界面层对其表面形貌的影响,得出生长温度在500 ℃~520 ℃,无过渡层,使用InAsSb界面层有利于改善材料的表面形貌.     

一维有限超晶格的电子态与透射问题的转移矩阵方法研究

采用转移矩阵方法,研究了一维有限超晶格的电子态与透射问题.计算了一维有限超晶格含单个缺陷层或少量缺陷层的透射谱和波函数,以及当电子被束缚在一维有限超晶格中电子的本征值和相应的定态本征函数.给出的方法对于研究电子通过任意排列的一维有限超晶格的输运具有普适性.     

SiO/SiO_2超晶格结构界面发光的研究

利用热蒸发技术在硅衬底上制备了层厚不同的SiO/SiO2超晶格样品.对其光致发光谱进行研究发现,随着SiO/SiO2超晶格中SiO层厚度的增加,发光峰在400～600 nm之间移动.研究表明,样品的发光中心来自于SiO/SiO2界面处的缺陷发光(界面态发光).即在样品沉积的过程中,在SiO/SiO2的界面处由于晶格的不连续性,会形成大量的Si-O悬挂键,这些悬挂键本身相互结合可以形成一定数量的缺陷,同时由于O原子容易脱离Si原子的束缚而产生扩散,因此,这些悬挂键可以与扩散的O原子结合,随着SiO层厚度的增加,在SiO/SiO2的界面处先后出现WOB(O3<≡Si-O-O·),NOV(O3≡Si-Si≡O3),E'中心(O≡Si·),NBOHC(O3≡Si-O·)等缺陷,这些缺陷在SiO层厚度增大的过程中对发光先后起到主导作用,从而使得发光峰产生红移.     

a-Si:H/a-SiNx:H超晶格的掺杂效应

采用带有可转动掩板的沉积系统,合成出一类新的a-Si:H/掺杂a-SiN_x:H超晶格。样品中各子层厚度及a-SiN_x:H子层中N/Si比固定,仅改变掺杂浓度。结果发现:此类超晶格中的费密能级可以通过a-SiN_x:H层中的掺杂来控制,即a-Si:H/a-SiN_x:H超晶格可以从n型转变为p型,依赖于a-SiN_x:H子层中B的掺杂比。然而,a-SiN_x:H子层中P的掺杂对a-Si:H/a-SiN_x:H超晶格传输特性影响并不大。 关键词：     

侧向铁磁/铁磁超晶格的推迟模式

用等效介质理论计算了半无限侧向铁磁/铁磁超晶格的推迟模式.且以Co/Ni体系超晶格为例具体计算了该超晶格的表面模式和体模式,展示出一些与磁性/非磁性超晶格不同的有趣性质.侧向磁性/磁性超晶格具有较复杂的推迟模式,这是一种具有高度一般性的体系,在改变构成超晶格的两种铁磁层的厚度的比值、外场时,可以调节两支表面模式的频率以及体模式的频带,这种调节作用是与两种铁磁层的饱和磁化值有关的.当饱和磁化值相差较大时,调制效果是很明显的.当第二种铁磁介质饱和磁化值趋于零时,该体系演变成熟知的磁性/非磁性超晶格.当取麦克斯 关键词： 铁磁/铁磁超晶格 推迟模式 等效介质理论 自旋波谱     

利用InAs/GaAs数字合金超晶格改进InAs量子点有源区的结构设计

利用分子束外延技术,通过InAs/GaAs数字合金超晶格代替传统的直接生长InGaAs层的方式,在GaAs(100)衬底上生长了InAs量子点结构并成功制备了1.3μm InAs量子点激光器.通过原子力显微镜和光致荧光谱测试手段,对传统生长模式和数字合金超晶格生长模式的两种样品进行了表征,研究发现采用32周期InAs/GaAs数字合金超晶格样品的量子点密度非常高,发光性能良好.通过与常规生长方式所制备激光器的性能对比,发现采用InAs/GaAs数字合金超晶格生长InAs量子点的有源区也可以得到高质量的激光器.利用该方式生长的InAs量子点激光器的阈值电流为24 mA,相应的阈值电流密度仅为75 A/cm2,最高工作温度达到120℃.InAs/GaAs数字合金超晶格既可以保证生长过程中源炉的温度保持不变,还可以对InGaAs层的组分实现灵活调控.不需要改变生长速度,通过改变InAs/GaAs数字合金超晶格的周期数以及InAs层和GaAs层的厚度,便可以获得任意组分的InGaAs,从而得到不同发光波长的激光器.这种生长方式对量子点有源区的结构设计和外延生长提供了新思路.     

Optical properties of core/multishell CdSe/Zn(S,Se) nanocrystals

CdSe nanocrystals are now known as highly efficient fluorescent light sources. Their efficiency is however strongly dependent on the quality of the passivation layers. We show here that using a ZnSe/ZnS bi-layer shell leads to a larger photoluminescence yield than both ZnSe and ZnS simple shells. The intermediate ZnSe layer acts as a lattice parameter adaptation layer to improve on the core/shell interface quality, while the ZnS outer shell maximizes the exciton confinement.     

Growth of high quality InSb thin films on GaAs substrates by molecular beam epitaxy method with AlInSb/GaSb as compound buffer layers

A series of In Sb thin films were grown on Ga As substrates by molecular beam epitaxy(MBE).Ga Sb/Al In Sb is used as a compound buffer layer to release the strain caused by the lattice mismatch between the substrate and the epitaxial layer,so as to reduce the system defects.At the same time,the influence of different interface structures of Al In Sb on the surface morphology of buffer layer is explored.The propagation mechanism of defects with the growth of buffer layer is compared and analyzed.The relationship between the quality of In Sb thin films and the structure of buffer layer is summarized.Finally,the growth of high quality In Sb thin films is realized.     

应变超晶格(ZnS)1/(ZnSe)1的光学性质

用linear mufin tin orbital能带方法，计算Si衬底上（ZnS）_n/（ZnSe）_n（001）超晶格的能带结构，计算中采用外加调整势进行带隙修正．在得到较准确的能带结构和波函数的基础上，计算该超晶格系统的光学介电函数虚部ε₂（ω）．结果表明，该超晶格系统的光学性质结合了ZnS和ZnSe体材料光学性质的特点，在相当宽的能量范围内有较好的光谱响应．并且该超晶格系统是直接带隙材料，在光电器件应用中有很大潜力． 关键词：     

Growth and electrical characterization of type II InAs/GaSb superlattices for midwave infrared detection

Herein, we report a type II InAs/GaSb superlattice structure (SLS) grown on GaSb(1 0 0) substrates by molecular beam epitaxy (MBE) and its electrical characterization for mid-wavelength infrared detection. A GaSb buffer layer was grown under optimized SLS growth conditions, which can decrease the occurrence of defects for similar pyramidal structures. The complications associated with these conditions include oxide desorption of the substrate, growth temperature of the SLS, the V/III ratio during superlattice growth and the shutter sequence. High-resolution X-ray diffraction (HRXRD) shows the sixth satellite peak, and the period of the SLS was 52.9 Å. The atomic force microscopy (AFM) images indicated that the roughness was less than 2.8 nm. High-resolution transmission electron microscopy (HRTEM) images indicated that the SLS contains few structural defects related to interface dislocations or strain relaxation during the growth of the superlattice layer. The photoresponse spectra indicated that the cutoff wavelength was 4.8 μm at 300 K. The SLS photodiode surface was passivated by a zinc sulfide (ZnS) coating after anodic sulfide.     

Zn1—xMnx／ZnSe应变超晶格分子束外延生长及光学特性研究

用分子束外延方法在ＧａＡｓ（１００）衬底上成功生长了高质量的Ｚｎ１－ｘＭｎｘＳｅ／ＺｎＳｅ（ｘ＝０．１６），超晶格结构，用Ｘ射线衍射和低温光致发光（ＰＬ）对其结构，应变分布以及光学性能进行了研究，结果表明，２Ｋ温度下，Ｚｎ１－ｘＭｎｘＳｅ／ＺｎＳｅ超晶格的光致发光中主发光峰对应于ＺｎＳｅ阱中基态电子和基态轻空穴之间的自由激子跃迁，而且其峰位相对于ＺｎＳｅ薄膜材料的自由激子峰有明显移动。其中，当超晶     

The influence of AlN/GaN superlattice intermediate layer on the properties of GaN grown on Si（111） substrates

AlN/GaN superlattice buffer is inserted between GaN epitaxial layer and Si substrate before epitaxial growth of GaN layer. High-quality and crack-free GaN epitaxial layers can be obtained by inserting AlN/GaN superlattice buffer layer. The influence of AlN/GaN superlattice buffer layer on the properties of GaN films are investigated in this paper. One of the important roles of the superlattice is to release tensile strain between Si substrate and epilayer. Raman spectra show a substantial decrease of in-plane tensile strain in GaN layers by using AlN/GaN superlattice buffer layer. Moreover, TEM cross-sectional images show that the densities of both screw and edge dislocations are significantly reduced. The GaN films grown on Si with the superlattice buffer also have better surface morphology and optical properties.     

SiC缓冲层对Si表面生长的 ZnO薄膜结构和光电性能的改善

用脉冲激光沉积(PLD)技术制备了ZnO/SiC/Si和 ZnO/Si薄膜并制成了紫外探测器。利用X射线衍射(XRD),光致发光(PL)谱,I-V曲线和光电响应谱对薄膜的结构和光电性能进行了研究。实验结果表明:SiC缓冲层改善了ZnO薄膜的结晶质量和光电性能,其原因可能是SiC作为柔性衬底能够减少ZnO与Si 之间大的晶格失配和热失配导致的界面缺陷和界面态。     

The role of a ZnO buffer layer in the growth of ZnO thin film on Al2O3 substrate

A ZnO buffer layer and ZnO thin film have been deposited by the pulsed laser deposition technique at the temperatures of 200 C and 400 C, respectively. Structural, electrical and optical properties of ZnO thin films grown on sapphire (Al₂O₃) substrate with 1, 5, and 9 nm thick ZnO buffer layers were investigated. A minute shift of the (101) peak was observed which indicates that the lattice parameter was changed by varying the thickness of the buffer layer. High resolution transmission electron microscopy (TEM) was used to investigate the thickness of the ZnO buffer layer and the interface involving a thin ZnO buffer between the film and substrate. Selected area electron diffraction (SAED) patterns show high quality hexagonal ZnO thin film with 30 in-plane rotation with respect to the sapphire substrate. The use of the buffer can reduce the lattice mismatch between the ZnO thin film and sapphire substrate; therefore, the lattice constant of ZnO thin film grown on sapphire substrate became similar to that of bulk ZnO with increasing thickness of the buffer layer.     

Surface preparation effect of GaAs(110) substrates on the ZnSe epitaxial layer grown by molecular beam epitaxy

The effect of the surface preparation of the GaAs(110) substrate on the ZnSe epitaxial layer grown by molecular beam epitaxy (MBE) was investigated by means of etch-pit density (EPD) measurements, surface morphology observation, and reflection high-energy electron diffraction (RHEED) analysis. The ZnSe epitaxial layer grown on a GaAs(110) surface prepared by cleaving the (001)-oriented wafer in ultrahigh vacuum (UHV) showed about 5×10⁴ cm^-2 of EPD. This value is much lower than that observed from both the samples grown on the mechanically polished surface with and without a GaAs buffer layer. Due to the non-stoichiometric surface after thermal evaporation of the surface oxide, three-dimensional growth can easily occur on the mechanically polished GaAs(110) substrate. These results suggest that the stoichiometric and atomically flat substrate surface is essential for the growth of low-defect ZnSe epitaxial layers on the GaAs(110) non-polar surface. Received: 21 August 1998 / Accepted: 19 October 1998 / Published online: 28 April 1999