Abstract

An ultralow-power <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">$K$ </tex-math></inline-formula> -band low-noise amplifier (LNA) for next generation radio astronomical receivers fabricated in 65-nm CMOS technology is presented in this letter. A gate–source transformer feedback is utilized for the simultaneous noise and impedance matching. In order to achieve high gain with limited dc power consumption ( <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">$P_{\mathrm {dc}}$ </tex-math></inline-formula> ), a single-ended neutralization technique is applied to the circuit. According to measurement, the proposed <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">$K$ </tex-math></inline-formula> -band LNA achieves a 19.1-dB small signal gain with 2.8-GHz 3-dB bandwidth (21.2–24 GHz) and noise figure of 3.6 dB with only 0.99 mW <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">$P_{\mathrm {dc}}$ </tex-math></inline-formula> . To the best of author’s knowledge, this LNA shows the highest figure of merit (FoM), which is 7071 1/W, among published <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">$K$ </tex-math></inline-formula> -band low-power LNAs.

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