35/spl次/2英寸晶圆MOVPE系统用于电子和光电器件

T. Schmitt, M. Deufel, G. Strauch, D. Schmitz, M. Heuken, H. Juergensen
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引用次数: 0

摘要

将显示AIX 2600G3行星反应器(R)在35/spl次/2英寸配置下与气箔旋转(R)的结果。将展示包括一颗卫星的所有7个2英寸晶圆在内的测量结果。作为爱思强行星反应堆(R)系统AIX 2600G3在35倍2英寸配置下的进一步详细研究和调整,我们使用旋转和故意固定的卫星研究了沿着反应堆半径的耗尽行为。掺杂dbr结构通常用作AlGaInP LED有源区域下方的反射镜,以增加光输出。因此,选择AlAs/GaAs分布式Bragg反射器(DBR)来优化5颗6英寸卫星的厚度均匀性和镓效率。进一步,我们通过AlInP的x射线数据研究了反应器总压力对半导体层组成的影响。为了检查我们的反应器配置的调整,我们选择了关键和非常温度敏感的材料系统AlGaInP,以及AlGaInP- mqw结构。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
35/spl times/2 inch wafer MOVPE system for electronic and optoelectronic devices
Results of the AIX 2600G3 planetary reactor(R) in the 35/spl times/2 inch configuration with Gas Foil Rotation(R) will be shown. Measurements including all seven 2 inch wafers of one satellite will be presented. As a further detailed study and tuning of the AIXTRON Planetary Reactor(R) system AIX 2600G3 in the 35 times 2 inch configuration, we investigated the depletion behaviour along the reactor radius using rotating, as well as intentionally fixed satellites. Very often doped DBR-structures are used as a mirror below the active region of the AlGaInP LED to increase the light output. So AlAs/GaAs distributed Bragg reflectors (DBR) were chosen to optimise the thickness homogeneity and gallium efficiency across the five 6 inch satellites in dependence of the total flow. Further on, we examined the influence of the total reactor pressure on the semiconductor layer composition via X-ray data of AlInP. To check the adjustments of our reactor configuration we chose the critical and very temperature sensitive material system AlGaInP, as well as AlGaInP-MQW structures.
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