Development of an SIS mixer-based amplifier for large-scale multipixel heterodyne receivers
This paper introduces a potential low-power-consumption and low-noise microwave amplifier operated at cryogenic temperature, essential for large-scale multi-pixel heterodyne receivers and fault-tolerant quantum computers. The amplifier employs two millimeter-wave superconductor-insulator-superconductor (SIS) mixers as amplifying elements and a millimeter-wave Josephson array oscillator as the local oscillator source. A proof-of-concept experiment utilizing waveguide SIS mixer modules demonstrated an average gain of approximately 7.5 dB and a noise temperature of around 10 K at microwave frequencies. Additionally, a waveguide Josephson array oscillator module, developed to validate the design, exhibited an output power of roughly 52 nW, estimated from the response of a waveguide SIS detector connected to the oscillator module. These findings indicate the feasibility of realizing a monolithically integrated amplifier chip incorporating SIS mixers and a Josephson array oscillator.
Authors
- Yoshinori Uzawa (ORCID: https://orcid.org/0000-0002-5483-7688)
- Wenlei Shan (ORCID: https://orcid.org/0000-0001-9270-0802)
- Kazumasa Makise (ORCID: https://orcid.org/0000-0002-2429-319X)
- Akira Kawakami (ORCID: https://orcid.org/0000-0001-9105-6349)
- Takafumi Kojima (ORCID: https://orcid.org/0000-0001-7949-6528)
- Sho Masui (ORCID: https://orcid.org/0000-0002-6264-6507)
- Akihira Miyachi (ORCID: https://orcid.org/0009-0002-6497-1001)
- Yosuke Murayama (ORCID: https://orcid.org/0009-0002-8315-4728)
Institutions
- National Astronomical Observatory of Japan (JP)
- National Institute of Information and Communications Technology (JP)
Publication Details
- Published
- 2024-08-16
- DOI
- https://doi.org/10.1117/12.3020000
- Primary Topic
- Advanced Electrical Measurement Techniques
- Type
- article
- Field-Weighted Citation Impact
- 0.00