Design, Characterization and Modeling of GaN-based HEMTs for Low-Noise and Cryogenic Applications
Doctoral thesis, 2025

Radio astronomy relies on detecting extremely weak signals and requires robust and rugged technologies,capable of preventing and withstand radio frequency interference (RFI). Low-noise amplifiers (LNAs)operating at cryogenic temperatures are key components in radio astronomy instrumentation. WhileLNAs based on advanced semiconductor technologies with limited power-handling capabilities have beenwidely used, gallium nitride (GaN)-based high-electron-mobility transistors (HEMTs) offer a promisingalternative due to their high robusteness and excellent low-noise performance at room temperature.However, their low-noise behavior at cryogenic temperatures has remained largely unexplored.This thesis investigates the potential of GaN-based HEMTs for cryogenic low-noise operation. Theminimum noise temperature of GaN-HEMTs at 10 K was found to be in the range of 4–5 K (0.06–0.07 dBnoise figure), which is comparable to other advanced technologies in the field. This was achieved throughwell-established experimental and modeling techniques, allowing for the characterization of noisecontributions in GaN-HEMTs as a function of operating frequency, dissipated power, and total deviceperiphery. The findings provide a foundation for designing future GaN-based LNAs that meet therequirements of cryogenic applications.For the first time, GaN-HEMTs with superconducting niobium (Nb) gates were demonstrated. Acomparative study with conventional gold (Au)-gated GaN-HEMTs revealed that superconducting Nbgates suppress the gate resistance dependence on gate width and length below Nb critical temperature(Tc < 9.2 K). However, self-heating effects were found to prevent the maintenance of Nb superconductivityat optimal noise-bias conditions, highlighting the need for further optimization of the device's heatdissipation capabilities.GaN-based metal-insulator-semiconductor (MIS)-HEMTs with a silicon nitride (SiNx) gate dielectric werealso examined at 4 K, demonstrating a minimum noise temperature of 8 K—comparable to theirconventional HEMT counterparts under the same conditions. These results highlight the impact of thegate dielectric on the cryogenic small-signal and noise parameters of the device, suggesting that furtherreduction of gate leakage current through improved gate insulation could enable additional noisereduction.The incorporation of gate field plates (FPs) was shown to improve device reliability by mitigating high-fieldand trapping effects, which become more pronounced at cryogenic temperatures. However, noiseanalysis of devices with and without FPs at 4 K revealed an overall detrimental impact of FPs, leading toat least a 35% noise degradation. This was attributed to increased parasitic capacitances, which reducedthe cutoff frequency. Nonetheless, devices with FPs exhibited improved drain-source conductance,offering advantages for low-noise impedance matching.

high frequency

High Electron Mobility Transistor (HEMT)

RFI

Low Noise Amplifier (LNA)

Cryogenic temperatures

Gallium Nitride (GaN)

Radio-astronomy

Lecture hall EA, EDIT-huset

Author

Mohamed Aniss Mebarki

Chalmers, Space, Earth and Environment, Onsala Space Observatory

Low-noise amplifiers (LNAs) are essential components in highly sensitive electronic systems,enabling the amplification of weak signals with minimal added noise. In radio astronomy, theyplay a crucial role in detecting cosmic signals—faint traces of distant galaxies, pulsars, and othercelestial phenomena. To achieve the highest sensitivity, LNAs are cooled to cryogenictemperatures for ultimate noise reduction.Like most modern electronics, LNAs rely on semiconductor materials. While widely usedsemiconductor technologies have enabled significant advancements, they also come withlimitations: they are vulnerable to interference from unwanted radio signals and have limitedpower-handling capabilities, posing risks of failure and reliability issues in extreme environments.At room temperature, GaN-based LNAs are valued for their robustness and high survivability, buttheir performance at cryogenic temperatures remains largely unexplored.This research investigates the behavior of GaN-based high-electron-mobility transistors (HEMTs)at cryogenic temperatures and explores strategies to optimize them for ultra-low-noiseapplications. The impact of various design choices was analyzed, including the incorporation offield plates and insulation layers, revealing trade-offs between improved reliability and noiseperformance. Innovative solutions for noise reduction were also examined, such as theintegration of superconducting materials. These findings provide valuable insights into enhancingboth the reliability and low-noise performance in cryogenic environments using GaN-basedHEMTs.Beyond radio astronomy, this work contributes to the broader evolution of GaN-based HEMTstechnology. As the demand for ultra-low-noise electronics grows—particularly in fields such asquantum computing, where cryogenic conditions are essential—these advancements haveimplications not only for radio astronomy but also for next-generation computing andcommunication technologies.

Subject Categories (SSIF 2025)

Nano-technology

Electrical Engineering, Electronic Engineering, Information Engineering

ISBN

978-91-8103-215-4

Doktorsavhandlingar vid Chalmers tekniska högskola. Ny serie: 5673

Publisher

Chalmers

Lecture hall EA, EDIT-huset

Online

More information

Latest update

10/15/2025