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SBIR/STTR

Design and fabrication of strain-balanced nBn dual-band LWIR/LWIR focal plane arrays based on InAsSb/InAsType-II superlattices, Phase I

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Project Introduction

The infrared spectral range is of particular interest for remote planetary sensing of gaseous molecules, such as H2O, CO2, CH4, N2O, CO, NH3, and many other compounds. Infrared thermography can also be used to accurate measure minute variations in surface temperatures. High performance infrared focal plane arrays (FPAs) allow rapid acquisition of a 2D surface maps--indispensable in planetary sciences. By using two different cut-off detectors integrated into a single FPA to simultaneously image a planet we can avoid atmospheric effect and much more accurately map minute variations in the surface temperature, or gain a clearer picture of the atmospheric composition. In recent years, Type-II InAs/GaSb superlattices have experienced significant development—we have played a pioneering role in the rapid development of that technology. However, the full potential of Type-II superlattice has not been fully explored and alternate superlattice architectures hold great promise; one of the most promising is gallium free InAsSb/InAs Type-II superlattices. In this project, we propose to study strain-balanced nBn InAs1-xSbx/InAs Type-II superlattice-based photodetectors and mini-arrays for LWIR/LWIR dual-band detection. Using this new superlattice structure, it is expected to achieve longer minority carrier lifetime. Longer minority carrier lifetime results in lower dark current, lower noise, higher operation temperature, and higher quantum efficiency. Applying this superlattice design to dual-band LWIR/LWIR FPAs, it is expected to achieve higher quantum efficiency, lower dark current, higher specific detectivity (D*) and reduced Noise Equivalent Temperature Difference (NETD). This work will form the basis of the Phase II work in which we will use this new superlattice structure to develop and deliver LWIR/LWIR dual-band FPAs for planetary sciences. More »

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