TY - JOUR
T1 - Four-band quantum well infrared photodetector array
AU - Bandara, S. V.
AU - Gunapala, S. D.
AU - Liu, J. K.
AU - Rafol, S. B.
AU - Ting, D. Z.
AU - Mumolo, J. M.
AU - Chuang, R. W.
AU - Trinh, T. Q.
AU - Liu, J. H.
AU - Choi, K. K.
AU - Jhabvala, M.
AU - Fastenau, J. M.
AU - Liu, W. K.
N1 - Funding Information:
The research described here was performed at the Center for Space Microelectronics Technology, Jet Propulsion Laboratory, California Institute of Technology, and was jointly sponsored by the National Aeronautics and Space Administration-Office of Space Science, the Ballistic Missile Defense Organization/Innovative Science & Technology Office, and the Air Force Research Lab.
PY - 2003
Y1 - 2003
N2 - 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 μm infrared bands. This 640 × 514 format FPA consists of four 640 × 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 × 1011 cm √Hz/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.
AB - 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 μm infrared bands. This 640 × 514 format FPA consists of four 640 × 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 × 1011 cm √Hz/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.
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U2 - 10.1016/S1350-4495(03)00157-9
DO - 10.1016/S1350-4495(03)00157-9
M3 - Article
AN - SCOPUS:0141904584
SN - 1350-4495
VL - 44
SP - 369
EP - 375
JO - Infrared Physics and Technology
JF - Infrared Physics and Technology
IS - 5-6
ER -