光学
量子级联激光器
激光器
自由空间光通信
探测器
级联
波长
远红外激光器
光电子学
材料科学
红外线的
物理
色谱法
化学
作者
Robert A. Marsland,Steven A. Jacobs,C. L. Canedy,Chase T. Ellis,Chul Soo Kim,Eric M. Jackson,I. Vurgaftman,B. Kolasa,Vijaysekhar Jayaraman,Morgan Turville-Heitz,T. Earles,Steven Ruder,B. Knipfer,Jaemin Ryu,J. R. Meyer,D. Botez,L. J. Mawst
出处
期刊:Optics Express
[Optica Publishing Group]
日期:2024-05-22
卷期号:32 (13): 22479-22479
被引量:7
摘要
Research has shown that free-space laser communication systems may experience fewer outages due to atmospheric impairments such as haze, fog, clouds, and turbulence by operating at a longer wavelength in the mid-wave or long-wave infrared, if disadvantages such as lower-performance transceiver components may be overcome. Here we report a resonant cavity infrared detector (RCID) with 4.6-µm resonance wavelength that enables 20-dB larger link budget than has been reported previously for ∼ 5 Gb/s operation. The device combines high responsivity, 1.97 A/W, with a low noise equivalent power (NEP) of 0.7 pW/ H z at room temperature, and a high bandwidth of 6.7 GHz at 3-dB. The relatively large surface-normal-incidence device with 30-µm diameter simplifies the coupling relative to intra-subband quantum cascade detectors. Although the RCID NEP is expected to increase with frequency to ∼ 1.5 pW/ H z , we estimate that the total equivalent noise power in a 2.5-GHz bandwidth is less than 200 nW. When combined with a relatively high power (∼100-mW) distributed-feedback quantum cascade laser, the difference of > 50 dB between modulated laser power and RCID noise significantly outpaces that of existing devices.
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