基于lnxGa1−xSb的红外光学探测器工作在1.7- 3µm范围内,用于环境气体传感

F. Mansoor, S. Haywood, P. Stavrinou, N. Mason, R. Nicholas, P. Walker, G. Hill
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引用次数: 0

摘要

在2-5微米范围内工作的设备对于环境传感应用具有潜在的重要性。大气污染物如CO, SOx和NOx在2-5µm范围内显示吸收带,并且在光源和检测器之间通过任何这些吸收带都会显示检测器信号的变化。在松弛的GaxIn1_xSb缓冲层上生长的2-3 μ m区域,正在研究应变平衡的GaSb/GaxIn1−xSb量子阱结构。这些提供了低应变结构,同时设计带隙以实现感兴趣的波长。本文主要讨论的是探测器的结构,而不是有源区的设计。因此,在一些设计用于确定从谐振结构实现的效率和灵敏度提高的器件中,大块GaSb被用作有源区域。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Infrared optical detectors operating in the 1.7- to 3-µm range based on lnxGa1−xSb for environmental gas-sensing
Devices operating in the 2-5 µm region are of potential importance for use in environmental sensing applications. Atmospheric pollutants such as CO, SOx, and NOx show absorption bands in the 2-5 µm range and passing any of these between a light source and detector will show a change in the detector signal. Strain-balanced GaSb/GaxIn1−xSb quantum well structures are being investigated to cover the 2-3 µm region grown on relaxed GaxIn1_xSb buffer layers. These provide low-strain structures while engineering the bandgap to realise the wavelength of interest. This paper is concerned mainly with the detector structure rather than the design of the active region. Hence bulk GaSb is used as the active region in some of the devices designed to ascertain the efficiency and sensitivity enhancement achievable from resonant structures.
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