In this paper, an inverter-based optical receiver is proposed to support gigabit-per-second optical wireless communication (OWC). The proposed optical receiver mainly consists of inverter-based amplifiers. In particular, a low-noise shunt-feedback transimpedance amplifier (TIA) is employed based on the three-stage inverter structure with pseudo-differential output. By decreasing the power supply, the noise performance is improved significantly, while the power consumption of the receiver is reduced. In addition, a two-stage limiting amplifier (LA) is adopted to further amplify signal swing. To prevent the saturation of the receiver under strong incident ambient light, a DC photocurrent cancellation (DPC) block is employed. The proposed receiver is designed with a 180 nm standard CMOS process. Simulation results indicated that the receiver achieves a data rate of up to 2 Gb/s with a bandwidth of 1.36 GHz, a gain of 110 dB Ω, and an input-referred noise (IRN) of 0.16 μ A <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">rms</inf> . Due to its simple inverter-based structure, the proposed receiver is promising to be implemented through digital synthesis in the future.
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Zhu et al. (2024) studied this question.
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