Self-heating of cryogenic high electron-mobility transistor amplifiers and the limits of microwave noise performance

Author:

Ardizzi Anthony J.1ORCID,Choi Alexander Y.1ORCID,Gabritchidze Bekari23ORCID,Kooi Jacob4ORCID,Cleary Kieran A.2ORCID,Readhead Anthony C.2ORCID,Minnich Austin J.1ORCID

Affiliation:

1. Division of Engineering and Applied Science, California Institute of Technology, Pasadena, California 91125, USA

2. Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, California 91125, USA

3. Department of Physics, University of Crete, GR-70 013 Heraklion, Greece

4. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA

Abstract

The fundamental limits of the microwave noise performance of high electron-mobility transistors (HEMTs) are of scientific and practical interest for applications in radio astronomy and quantum computing. Self-heating at cryogenic temperatures has been reported to be a limiting mechanism for the noise, but cryogenic cooling strategies to mitigate it, for instance, using liquid cryogens, have not been evaluated. Here, we report microwave noise measurements of a packaged two-stage amplifier with GaAs metamorphic HEMTs immersed in normal and superfluid [Formula: see text]He baths and in vacuum from 1.6 to 80 K. We find that these liquid cryogens are unable to mitigate the thermal noise associated with self-heating. Considering this finding, we examine the implications for the lower bounds of cryogenic noise performance in HEMTs. Our analysis supports the general design principle for cryogenic HEMTs of maximizing gain at the lowest possible power.

Funder

National Science Foundation

Jet Propulsion Laboratory

National Aeronautics and Space Administration

Publisher

AIP Publishing

Subject

General Physics and Astronomy

Reference48 articles.

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3. M. W. Pospieszalski, “Extremely low-noise cryogenic amplifiers for radio astronomy: Past, present and future,” in2018 22nd International Microwave and Radar Conference (MIKON)(IEEE, 2018), pp. 1–6.

4. Low-Noise Amplifier for Next-Generation Radio Astronomy Telescopes: Review of the State-of-the-Art Cryogenic LNAs in the Most Challenging Applications

5. J. Bautistaet al., “Cryogenic, X-band and Ka-band InP HEMT based LNAs for the deep space network,” in2001 IEEE Aerospace Conference Proceedings (Cat. No. 01TH8542)(IEEE, 2001), Vol. 2, pp. 2/829–2/842.

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