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Published on: August 2, 2019
Quantum circuits with SINIS structures
Mikhail Tarasov1, Mikhail Fominskii1, Aleksandra Gunbina1
1V. Kotelnikov Institute of Radio Engineering and Electronics RAS, Moscow, Russia.
Superconductor-insulator-normal metal-insulator-superconductor (SINIS) tunnel junctions are key for cryogenic devices. Optimized SINIS arrays achieve high responsivity for detecting microwave radiation, crucial for radio astronomy applications.
Area of Science:
- Cryogenic devices
- Superconducting electronics
- Microwave detection
Background:
- Superconductor-insulator-normal metal-insulator-superconductor (SINIS) tunnel junctions are fundamental components in advanced cryogenic applications.
- These devices are utilized in microwave detectors, electron coolers, primary thermometers, and Aharonov-Bohm interferometers.
- Fabrication and measurement of SINIS devices have been performed at temperatures as low as 100 mK.
Purpose of the Study:
- To optimize SINIS tunnel junction structures for enhanced sensitivity and responsivity in cryogenic devices.
- To develop and test SINIS arrays specifically for detecting 90 GHz radiation for radio astronomy.
- To evaluate the performance of SINIS receivers in a cryostat at low temperatures.
Main Methods:
- Manufacturing of SINIS structures using Dolan-type and Manhattan-type shadow evaporation, and magnetron sputtering.
- Suspension of the absorber above the substrate to improve ultimate sensitivity.
- Testing of SINIS arrays with a black body radiation source, band-pass filters, and an IMPATT diode radiation source.
Main Results:
- Achieved responsivity up to 30 electrons per photon at 350 GHz (72000 A/W) and voltage responsivity up to 3.9 × 10^9 V/W.
- Designed SINIS arrays demonstrated noise equivalent power below 10^-16 W·Hz^-1/2 for 90 GHz radiation detection.
- Successful mounting and testing of a SINIS receiver in a 3He cryostat at 260 mK at the Nasmyth focus of the BTA telescope.
Conclusions:
- Optimized SINIS tunnel junctions offer significant improvements in sensitivity and responsivity for cryogenic applications.
- The developed SINIS arrays are suitable for detecting faint microwave signals, particularly for radio astronomy at 90 GHz.
- The experimental setup and testing at the BTA telescope confirm the potential of SINIS devices for astronomical observations.
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