Analysis of the auger recombination rate in P+N−n−N−N HgCdTe detectors for HOT applications

J. Schuster, W. Tennant, E. Bellotti, P. Wijewarnasuriya
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引用次数: 8

Abstract

Infrared (IR) photon detectors must be cryogenically cooled to provide the highest possible performance, usually to temperatures at or below ~ 150K. Such low operating temperatures (Top) impose very stringent requirements on cryogenic coolers. As such, there is a constant push in the industry to engineer new detector architectures that operate at higher temperatures, so called higher operating temperature (HOT) detectors. The ultimate goal for HOT detectors is room temperature operation. While this is not currently possibly for photon detectors, significant increases in Top are nonetheless beneficial in terms of reduced size, weight, power and cost (SWAP-C). The most common HgCdTe IR detector architecture is the P+n heterostructure photodiode (where a capital letter indicates a wide band gap relative to the active layer or “AL”). A variant of this architecture, the P+N−n−N−N heterostructure photodiode, should have a near identical photo-response to the P+n heterostructure, but with significantly lower dark diffusion current. The P+N−n−N−N heterostructure utilizes a very low doped AL, surrounded on both sides by wide-gap layers. The low doping in the AL, allows the AL to be fully depleted, which drastically reduces the Auger recombination rate in that layer. Minimizing the Auger recombination rate reduces the intrinsic dark diffusion current, thereby increasing Top. Note when we use the term “recombination rate” for photodiodes, we are actually referring to the net generation and recombination of minority carriers (and corresponding dark currents) by the Auger process. For these benefits to be realized, these devices must be intrinsically limited and well passivated. The focus of this proceeding is on studying the fundamental physics of the intrinsic dark currents in ideal P+N−n−N−N heterostructures, namely Auger recombination. Due to the complexity of these devices, specifically the presence of multiple heterojunctions, numerical device modeling techniques must be utilized to predict and understand the device operation, as analytical models do not exist for heterojunction devices.
热应用中P+N−N−N HgCdTe探测器的螺旋复合率分析
红外(IR)光子探测器必须低温冷却以提供尽可能高的性能,通常温度在~ 150K或以下。如此低的工作温度(Top)对低温冷却器提出了非常严格的要求。因此,业界不断推动设计在更高温度下工作的新型探测器架构,即所谓的高工作温度(HOT)探测器。热探测器的最终目标是在室温下工作。虽然目前还不可能用于光子探测器,但Top的显著增加在减小尺寸、重量、功率和成本(SWAP-C)方面仍然是有益的。最常见的HgCdTe红外探测器结构是P+n异质结构光电二极管(其中大写字母表示相对于有源层或“AL”的宽带隙)。这种结构的一种变体,P+N−N−N−N异质结构光电二极管,应该具有与P+N异质结构几乎相同的光响应,但具有明显更低的暗扩散电流。P+N−N−N−N异质结构利用掺量极低的AL,两侧被宽间隙层包围。AL中的低掺杂使AL完全耗尽,从而大大降低了该层中的俄歇复合率。使俄歇复合率最小化可降低本禀暗扩散电流,从而增加Top。注意,当我们对光电二极管使用术语“重组率”时,我们实际上指的是通过俄歇过程产生的少数载流子(以及相应的暗电流)的净产生和重组。为了实现这些好处,这些器件必须具有内在的限制和良好的钝化。本研究的重点是研究理想P+N−N−N异质结构(即俄歇复合)中本征暗电流的基本物理性质。由于这些器件的复杂性,特别是多个异质结的存在,必须利用数值器件建模技术来预测和理解器件的操作,因为异质结器件不存在解析模型。
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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