插入生长AlGaAs薄膜对InAs量子点探测器性能的影响

利用分子束外延生长获得的两个InAs量子点样品制备了n型的量子点红外探测器.对于其中一个器件,在InAs量子点有源区的底部和顶部分别插入生长了AlGaAs势垒层.利用透射电阻显微技术研究了两个样品的结构特性;利用光致发光光谱和光电流谱研究了两个器件的光电性质.实验结果表明,AlGaAs层的插入对器件的探测性质有显著的影响.利用有三维效质量近似模型的计算结果,指认了带内光电流谱中峰结构的起源. 关键词： InAs 量子点 AlGaAs薄膜 光致发光光谱 有效质量近似模型     

纤锌矿GaN薄膜光学性质的研究

在测试大量纤锌矿GaN外延薄膜透射光谱基础上,通过对有代表性的四个样品的透射光谱进行拟合,获取了GaN外延薄膜的光学常量并计算了薄膜厚度.结果表明:GaN外延薄膜的折射率差异较小,但在370～800 nm波长范围内消光系数差异很大,GaN薄膜的消光系数差异在一定程度上可用以评价外延薄膜的质量.     

B+注入HgCdTe外延材料的红外透射光谱分析

运用多层模型和膜系传递矩阵以及非线性二乘法，模拟了B+注入碲镉汞外延材料的红外透射光谱，结果表明B+注入碲镉汞外延材料的红外透射光谱能够很好地理论再现，并由此获得了结区的自由载流子浓度分布、迁移率、面自由载流子浓度以及折射率和消光系数等相关参量，所得结果与微分Hall法测试的结果是一致的.计算结果也表明B+注入HgCdTe导致红外透射率变化的根本原因是注入层的高载流子浓度的等离子效应改变了该层的折射率和消光系数.     

利用紫外透射光谱研究透射式GaN光电阴极的材料结构及光学特性

GaN紫外光电阴极是近年发展起来的一种高性能真空紫外探测器件,其中透射式结构作为光电阴极实际应用的工作模式,其多层结构参数及光学特性对阴极的最终光电发射性能有着重要的影响.测试了透射式GaN阴极材料的紫外透射光谱,通过建立透射式GaN阴极样品的透射模型,得到了GaN阴极样品的薄膜厚度、光学吸收系数与透射谱之间的函数关系.计算得到的GaN外延材料的厚度与实际值误差小,吸收系数与已发表数据一致,表明紫外透射光谱法能够准确地实现透射式GaN阴极材料结构及光学特性的评估.     

红外光谱法研究射频功率对微晶硅薄膜微结构的影响

采用射频等离子体增强化学气相沉积(RF-PECVD)技术,在硅衬底上以不同的射频功率生长微晶硅(μc-Si:H)薄膜,利用傅里叶变换红外透射光谱技术对薄膜进行测试.通过对红外透射光谱的高斯拟合分析,结果表明薄膜中的氢含量和硅氢键合模式跟射频功率密切相关;当射频率从30W增加到110W时,薄膜中的氢含量先减少后慢慢增加,而结构因子逐渐增加后再减小,并且硅氢键合模式由以SiH为主转变为以SiH2为主.并讨论了这些参量随射频功率变化的机理.     

GaN及AlGaN薄膜透射光谱的研究

利用透射光谱矩阵光学原理,对三种GaN或AlGaN外延薄膜的透射光谱进行了分析.在传统的透射光谱拟合方法的基础上,添加了表征材料表面粗糙度、膜内散射情况的拟合参量,拟合曲线与实验曲线达到了准确的吻合.结果表明:外延薄膜透射光谱的拟合可以准确提取出材料的消光系数、表面状况、散射情况、折射率及厚度,从而对样品质量作出详细的分析.     

截止波长12 μm的p型-InAs0.04Sb0.96材料的熔体外延生长

为了获得p-型的长波长InAsSb材料并研究掺杂剂Ge对材料特性的影响,用熔体外延法生长了掺Ge的波长为12 μm的p型-InAsSb 外延层.用傅里叶红外光谱仪、Van der Pauw 法和电子探针微分析研究了材料的透射光谱、电学性质以及组分的分布.结果表明,两性杂质Ge在熔体外延生长的InAs0.04Sb0.96材料中起受主杂质作用.当外延层的组分相同时,材料的截止波长不随掺Ge浓度的变化而变化,但是随着外延层中掺Ge量的增加,外延层的透射率下降.掺杂原子Ge在外延层的表面及生长方向的分布都是相当均匀的.77 K下测得,载流子浓度为9.18×1016 cm-3的掺Ge的p型-InAs0.04Sb0.96样品,其空穴迁移率达到1 120 cm2·Vs-1.     

高速850 nm垂直腔面发射激光器的优化设计与外延生长

利用传输矩阵理论和TFCalc薄膜设计软件分析了分布布拉格反射镜和垂直腔面发射激光器(VCSEL)的反射率谱特性,对比了从谐振腔入射与从表面入射时反射率谱的差异,为白光反射谱表征VCSEL外延片提供了依据.利用Crosslight软件模拟了InGaAs/AlGaAs应变量子阱的增益谱随温度的变化特性及VCSEL器件内部温度分布,设计了增益-腔模调谐的VCSEL.采用金属有机物化学气相淀积设备外延生长了顶发射VCSEL,制作了氧化孔径为7.5μm的氧化限制型VCSEL器件,测试了器件的直流特性、光谱特性和眼图特性;6 mA,2.5 V偏置条件下输出光功率达5 mW,4级脉冲幅度调制传输速率达50 Gbit/s.     

在a-平面蓝宝石衬底上分子束外延生长的ZnO和ZnMgO材料结构和光学性质(英文)

氧化锌材料是新一代宽禁带光电子半导体材料,我们通过等离子体分子束外延设备,在a plane的蓝宝石衬底生长了高质量的氧化锌外延材料。在生长过程中用反射高能电子束衍射仪(RHEED),在位地研究了生长时材料薄膜的表面形貌。通过调节ZnMgO材料镁的组份,生长了禁带宽度可调的宽禁带材料。用紫外-可见透射光谱研究了ZnO,Zn0.89Mg0.11O和Zn0.80Mg0.20O薄膜材料的透射和吸收光谱性质,观察到Zn0.89Mg0.11O,Zn0.80Mg0.20O材料的吸收边的蓝移现象等。以上说明了我们用分子束外延生长 收稿日期:2003 07 22·09·　　第1期StructuralandOpticalCharacterizationofZnOandZnMgOFilmsona-planesapphiresbyMolecularBeamEpitaxy2004年设备成功的生长了高质量的氧化锌和组份渐变的ZnMgO薄膜材料。     

GaAs/Al_xGa_(1-x)As多量子阱外延结构及其LP-MOCVD生长工艺研究

在低压金属有机化学气相沉积生长工艺中,对用于制作850nm垂直腔面发射激光器件的GaAs/Al_xGa_(1-x)As多量子阱外延结构的生长温度、反应室压力、总载气流量以及生长速度等主要工艺参量进行优化,并进行了完整外延结构的生长.实验结果表明:在700℃条件下,得到多种组分的GaAs/Al_xGa_(1-x)As多量子阱结构,通过光致发光谱对比测试得到的最佳组分x为0.24,同时得到良好的表面形貌,最终确定的最佳生长速度为0.34~0.511nm/s.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...