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Low noise millimeter wave amplifiers for space science and technology: a study of hot electron noise

Completed TRL 2 (started at 2, targeting 3)

Description

The objective of this project is to identify the physical origin of drain noise in high electron mobility transistors (HEMTs) and thereby establish a pathway towards millimeter-wave amplifiers with a quantum-limited noise figure. Low noise amplifiers based on HEMTs are ubiquitous in space science and technology. While the noise mechanisms in these devices have been studied since their original development in the late 1980s, the origin of the noise associated with the hot electron gas in the channel remains a topic of debate. I will address this long-standing challenge using a novel technical approach that permits a parameter-free microscopic description of the fluctuations of hot electrons. With the knowledge gained from this approach, predictions regarding device optimization can be tested to create the next generation of low noise microwave amplifiers operating near the quantum noise limit.

Benefits

With the knowledge gained from this approach, predictions regarding device optimization can be tested to create the next generation of low noise microwave amplifiers operating near the quantum noise limit.

Details

Technology areaSensors and Instruments > Remote Sensing Instruments and Sensors > Microwave, Millimeter Waves, and Submillimeter Waves
ProgramSpace Technology Research Grants (STRG)
Lead organizationCalifornia Institute of Technology, Pasadena, CA
Start date2021-08-02
End date2024-08-30

Project contacts

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How to get involved

This is early/mid-stage (TRL 2) — the most realistic path in is NASA SBIR/STTR, which funds small businesses and research institutions to develop technology aligned with NASA's needs (equity-free, phased funding). Check whether a current SBIR/STTR solicitation topic overlaps with this project's technology area, or contact the project directly (above) to ask.

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