Physics and design of low noise avalanche photodiodes - LEOS distinguished lecture 2003-2004

J. David
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Abstract

Summary form only given. Avalanche photodiodes (APDs) are used in many applications when conventional unity gain photodiodes cannot provide enough sensitivity and the extra amplification provided by the impact ionization process gives it an advantage. Unfortunately this amplification or gain of the incoming optical signal is always accompanied by some 'excess noise' due to the stochastic nature of the ionization process and this sets a limit to the maximum useful gain. Early work by McIntyre showed that the excess noise depended on the ratio of hole ionization coefficient (/spl beta/) to electron ionization coefficient (/spl alpha/). /spl alpha/ and /spl beta/ are semiconductor material dependent and unfortunately most III-V materials have /spl alpha//spl ap//spl beta/, giving rise to relatively high excess noise. Since the ionization coefficients depend on the details of the band structure it is extremely difficult to modify, even using band-gap engineering techniques such as superlattices or MQWs. In recent years, work done at the University of Sheffield and the University of Texas (Austin) has shown that low excess noise can be obtained in homojunction structures simply by utilising thin avalanching regions. Experimental results show that contrary to conventional theory, the excess noise actually decreases as the avalanching width reduces. This behaviour has now been observed in virtually all semiconductor materials including GaAs, AlGaAs, InP, AlInAs and even silicon. The reason for this anomalous behaviour in thin devices is due to the 'dead space' (d), defined as the minimum distance a carrier has to travel before it is in equilibrium with the electric field. Conventional models of the ionization process ignored. This assumption is generally valid in devices with thick avalanching widths in which the dead space distance, d, is relatively small compared to the avalanching width, w. In thin avalanching width structures, d becomes a significant fraction of w and the ionizing process becomes more deterministic, reducing the stochastic variations that give rise to the excess noise. This talk will review these results and show that in addition to reducing the excess noise, thin avalanching widths offer APDs with other advantages such as lower operating voltages, better temperature stability and predicted enhanced speed of operation.
低噪音雪崩光电二极管的物理与设计- LEOS杰出讲座2003-2004
只提供摘要形式。当传统的单位增益光电二极管不能提供足够的灵敏度时,雪崩光电二极管(apd)被用于许多应用中,而冲击电离过程提供的额外放大使其具有优势。不幸的是,由于电离过程的随机性,输入光信号的放大或增益总是伴随着一些“过量噪声”,这就限制了最大有用增益。McIntyre的早期工作表明,多余噪声取决于空穴电离系数(/spl β /)与电子电离系数(/spl α /)的比值。/spl alpha/和/spl beta/依赖于半导体材料,不幸的是,大多数III-V材料具有/spl alpha//spl ap//spl beta/,从而产生相对较高的过量噪声。由于电离系数取决于带结构的细节,因此即使使用带隙工程技术(如超晶格或mqw)也很难修改。近年来,谢菲尔德大学和德克萨斯大学(奥斯汀)所做的工作表明,只需利用薄的雪崩区域,就可以在同质结结构中获得低过量噪声。实验结果表明,与传统理论相反,过量噪声实际上随着雪崩宽度的减小而减小。这种行为现在已经在几乎所有的半导体材料中被观察到,包括GaAs、AlGaAs、InP、AlInAs甚至硅。薄器件中这种异常行为的原因是由于“死区”(d),定义为载流子在与电场平衡之前必须行进的最小距离。传统的电离过程模型被忽略了。这种假设通常适用于具有较厚雪崩宽度的器件,其中死区距离d与雪崩宽度w相比相对较小。在较薄的雪崩宽度结构中,d成为w的重要部分,并且电离过程变得更加确定,减少了引起过量噪声的随机变化。本次演讲将回顾这些结果,并表明除了减少多余的噪声外,薄雪崩宽度还为apd提供了其他优势,例如更低的工作电压,更好的温度稳定性和预期的运行速度提高。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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