Resonant Cavity Enhanced Photodetectors for the Mid-Wave Infrared

被引:0
|
作者
Craig, A. P. [1 ]
Golding, T. [2 ,3 ]
Savich, G. R. [3 ]
Wicks, G. W. [3 ,4 ]
Marshall, A. R. [1 ]
机构
[1] Univ Lancaster, Phys Dept, Lancaster LA1 4YB, England
[2] Amethyst Res Ltd, Kelvin Campus,West Scotland Sci Pk, Glasgow G20 0SP, Lanark, Scotland
[3] Amethyst Res Inc, 123 Case Circle, Ardmore, OK 73401 USA
[4] Univ Rochester, Inst Opt, Rochester, NY 14627 USA
关键词
resonant cavity; antimonides; photodetector; BLIP limit; methane; CO2; toxic gasses;
D O I
10.1117/12.2536900
中图分类号
TP7 [遥感技术];
学科分类号
081102 ; 0816 ; 081602 ; 083002 ; 1404 ;
摘要
We present III-Sb resonant cavity-enhanced (RCE) photodetectors suitable for gas detection in the mid-wave infrared. AlAsSb/GaSb DBRs and absorbers of bulk InAsSb or a type-II InAsSb-InAs SLS were grown on GaSb, allowing for operation at 3.72 mu m or 4.52 mu m, with linewidth Delta lambda < 50 nm and Delta lambda < 70 nm, respectively. A barrier diode structure was used, and the absorber thickness was limited to 96 nm for InAsSb - or 192 nm for the SLS - in order to limit the dark currents. High quantum efficiency was obtained through the resonant optical field, while the remainder of the cavity was grown using wide-gap AlAsSb spacer layers not contributing to the dark current. By carefully compensation doping the AlAsSb layers, the 3.72 mu m device was bandgap-engineered for a flat Fermi level in the thin absorber, and hence dark currents which scale with the absorber thickness. This can equate to a >20x reduction in noise compared with a conventional nBn detector with full thickness absorber. At 3.72 mu m, performance above the BLIP limit imposed on broadband photodetectors was found by calculating for the specific detectivity.
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页数:6
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