Differential BroadBand (1¿16 GHz) MMIC GaAs mHEMT Low-Noise Amplifier for Radio Astronomy Applications and Sensing Articles uri icon

authors

  • Jimenez Martin, Jose Luis
  • GONZALEZ POSADAS, VICENTE
  • Parra Cerrada, Angel
  • Espinosa Adams, David
  • SEGOVIA VARGAS, DANIEL
  • Hernandez, Wilmar

publication date

  • May 2024

issue

  • 10

volume

  • 24

Electronic International Standard Serial Number (EISSN)

  • 1424-8220

abstract

  • A broadband differential-MMIC low-noise amplifier (DLNA) using metamorphic high-electron-mobility transistors of 70 nm in Gallium Arsenide (70 nm GaAs mHEMT technology) is presented. The design and results of the performance measurements of the DLNA in the frequency band from 1 to 16 GHz are shown, with a high dynamic range, and a noise figure ((Formula presented.)) below 1.3 dB is obtained. In this work, two low-noise amplifiers (LNAs) were designed and manufactured in the OMMIC foundry: a dual LNA, which we call balanced, and a differential LNA, which we call DLNA. However, the paper focuses primarily on DLNA because of its differential architecture. Both use a 70 nm GaAs mHEMT space-qualified technology with a cutoff frequency of 300 GHz. With a low power bias (Formula presented.) (5 V/40.5 mA), (Formula presented.) less than 1.07 dB 'on wafer' was achieved, from 2 to 16 GHz; while with the measurements made 'on jig', (Formula presented.) = 1.1 dB, from 1 to 10 GHz. Furthermore, it was obtained that (Formula presented.) less than 1.5 dB, from 1 to 16 GHz, with a figure of merit equal to 145.5 GHz/mW. Finally, with the proposed topology, several LNAs were designed and manufactured, both in the OMMIC process and in other foundries with other processes, such as UMS. The experimental results showed that the (Formula presented.) of the DLNA MMIC with multioctave bandwidth that was built in the frequency range of the L-, S-, C-, and X-bands was satisfactory.

keywords

  • broadband gallium arsenide; differential low-noise amplifier; figure of merit; monolithic microwave integrated circuit; noise figure; radio astronomy; stability analysis