Four-band quantum well infrared photodetector array

被引:25
作者
Bandara, SV
Gunapala, SD
Liu, JK
Rafol, SB
Ting, DZ
Mumolo, JM
Chuang, RW
Trinh, TQ
Liu, JH
Choi, KK
Jhabvala, M
Fastenau, JM
Liu, WK
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] USA, Res Lab, Adelphi, MD 20783 USA
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] IQE Inc, Bethlehem, PA 18015 USA
关键词
D O I
10.1016/S1350-4495(03)00157-9
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
A four-band quantum well infrared photodetector (QWIP) focal plane array (FPA) has been demonstrated by stacking different multi-quantum well structures, which are sensitive in 4-5.5, 8.5-10, 10-12, and 13-15.5 mum infrared bands. This 640 x 514 format FPA consists of four 640 x 128 pixel areas which are capable of acquiring images in these infrared bands. In this application, instead of quarter wevelength groove depth grating reflectors, three-quarter wavelength groove depth reflectors were used to couple radiation to each QWIP layer. This technique allows us to optimize the light coupling to each QWIP stack at corresponding pixels while keeping the pixel (or mesa) height at the same level, which will be essential for indium bump-bonding with the multiplexer. In addition to light coupling, these gratings serve as a contact to the active stack while shorting the unwanted stacks. Flexible QWIP design parameters, such as well width, barrier thickness, doping density, and the number of periods, were cleverly exploited to optimize the performance of each detector while accommodating requirements set by the deep groove light coupling gratings. For imaging, detector array is operated at temperature T = 45 K, and each detector shows a very high D* > 1 x 10(11) cm rootHz/W for 300 K background with f/2 optics. This initial array gave excellent images with 99.9% of the pixels working, demonstrating the high yield of GaAs technology. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:369 / 375
页数:7
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