nBn mid-wavelength infrared photodetectors based on bulk InGaAsSb absorbers

被引:0
|
作者
Cao, Peng [1 ,2 ]
Wei, Jiaqi [1 ,3 ]
Bentley, Matthew [4 ]
Davison, Nicholas [4 ]
Hu, Yidan [4 ]
You, Minghui [5 ]
Peng, Hongling [1 ,2 ]
Wang, Tiancai [6 ]
Zhuang, Qiandong [4 ]
Zheng, Wanhua [1 ,2 ,3 ,6 ]
机构
[1] Laboratory of Solid State Optoelectronics Information Technology, Institute of Semiconductors, CAS, Beijing,100083, China
[2] State Key Laboratory on Integrated Optoelectronics, Institute of Semiconductors, CAS, Beijing,100083, China
[3] College of Electronic and Communication Engineering, University of Chinese Academy of Sciences, Beijing,101408, China
[4] Physics Department, Lancaster University, Lancaster,LA1 4YB, United Kingdom
[5] College of Engineering and Technology, Jilin Agricultural University, 2888 Xincheng Street, Changchun,130118, China
[6] Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou,310024, China
关键词
Aluminum compounds - Gallium alloys - Indium alloys - Indium antimonides - Indium phosphide - Infrared detectors - Layered semiconductors - Semiconducting indium gallium arsenide - Semiconducting indium phosphide;
D O I
10.1364/OME.559184
中图分类号
学科分类号
摘要
In this paper, we demonstrate an nBn mid-wavelength infrared (MWIR) photodetector with a 100% cutoff wavelength over 4.0 µm based on a high-In composition InGaAsSb absorber on GaSb substrate. A thin AlGaAsSb layer is exploited as the barrier layer to suppress the generation-recombination (G-R) current. Both structural and optical properties of the grown InGaAsSb epilayer are investigated by high-resolution X-ray diffraction (HRXRD) and photoluminescence (PL) measurement. Low dark current density down to 9.9 × 10−5 A/cm2 and 6.5 × 10−2 A/cm2 are obtained at −500 mV under 77 K and 300 K, respectively. Moreover, respective peak responsivity of 0.64 A/W and 0.10 A/W at 2.67 µm are achieved at −500 mV under 77 K and 160 K. These correspond to a peak specific detectivity of 1.06 × 1011 cm·Hz1/2/W and 4.23 × 109 cm·Hz1/2/W, respectively. © 2025 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement.
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页码:717 / 723
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