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Journal of Communications Technology and Electronics

Analysis of the possibility to amplify an RF signal with a superconducting quantum interference filter

A. Kalabukhov, M. L. Chukharkin, Anatoly A. Deleniv, Dag Winkler, Ivan A. Volkov, Oleg V. Snigirev

Published Aug 1, 2008• 13 citations
Publisher

Abstract

A laboratory prototype RF amplifier for the frequency range 1–10 GHz is designed, created, and tested. The device is based on high-temperature superconducting quantum interference filters (SQUIFs) and the technology of bicrystalline substrates. The main characteristics of the prototype SQUIF amplifier are numerically simulated and measured.

DOI
10.1134/s1064226908080111

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A laboratory prototype RF amplifier for the frequency range 1–10 GHz is designed, created, and tested. The device is based on high-temperature superconducting quantum interference filters (SQUIFs) and the technology of bicrystalline substrates. The main characteristics of the prototype SQUIF amplifier are numerically simulated and measured.
The superconducting quantum interference filter (SQIF) is a new type of superconducting device which has been recently proposed for highly sensitive magnetometers for absolute magnetic field measurements. It benefits of very high voltage-to-field response, which is, in contrast conventional dc SQUIDs, not periodical. The SQIF can also be used as a radiofrequency amplifier in a similar way as the dc SQUID that can operate in a gigahertz frequency range. We designed a series type of SQIF amplifier that is compatible to conventional YBa2Cu3O7(YBCO) technology on bicrystal substrates. We present analytical, numerical and scale modeling as well as first electrical measurements results at frequencies up to 10 GHz. The SQIF array consists of 50 loops with randomly distributed areas from 0.5 to 1.5 times of . We also compared it to the regular array of conventional SQUIDs with the same loop areas. We have additional dc contacts to each 5-th SQUIDs and the SQIFs for control and comparison. Devices are fabricated using Josephson junctions with 3 mum width formed in YBCO over 24/24 and 12/12 degrees grain boundaries in yttrium-stabilized zirconia (YSZ) bicrystal substrates.
Abstract Superconducting quantum interference filters (SQIF) are promising devices for radio frequency (RF) detection combining low noise, high sensitivity, large dynamic range and wide-band capabilities. Impressive progress has been made recently in the field, with SQIF based antennas and amplifiers showing interesting properties in the GHz range using the well-established Nb/AlO x technology. The possibility to extend these results to high temperature superconductors (HTS) is still open, and different techniques to fabricate HTS SQIFs compete to make RF devices. We report on the DC and RF response of a high temperature SQIF fabricated by the ion irradiation technique. It is made up of 1000 superconducting quantum interference devices in series, with loop areas randomly distributed between 6 and 60 μ m 2 . The DC transfer factor is ∼450 V T −1 at optimal bias and temperature, and the maximum voltage swing ∼2.5 mV. We show that such a SQIF detects RF signals up to 150 MHz. It presents linear characteristics for RF power spanning more than five decades, and non-linearities develop beyond P RF = −35 dBm in our set-up configuration. The second harmonic generation has been shown to be at a minimum at the functioning point in the whole range of frequencies. A model has been developed which captures the essential features of the SQIF RF response.
We designed, fabricated, and measured broadband low-noise amplifiers based on Superconducting Quantum Interference Filters (SQIFs) for variety of applications ranging from superconducting quantum bits readout to satellite communication receivers. Our microwave amplifiers (Microwave SQAs) are based on 1-, 5-, 10-, 20-cell serial biSQUID SQIF arrays. The RF input is applied via a 50 Ohm coplanar waveguide connected to a superconducting line coupled to each biSQUID cell and integrated with input/output planar capacitors to define and tune up signal frequency bandwidth. The RF output comes out from the central common line via a balanced output circuit matching to a 50 Ohm output coplanar waveguide. The same circuit is used for symmetrical dc biasing of an array. Microwave SQA samples were fabricated on 5 mm × 5 mm chips using standard HYPRES niobium 4.5 kA/cm2fabrication process. The results of experimental evaluation of our Microwave SQAs based on SQIF serial arrays with different number of biSQUID cells are compared. We have demonstrated a power gain up to 20 dB from 8 to 11 GHz.
We have studied superconducting quantum interference filters (SQIFs) based on bicrystal neodymium gallate substrates, which can be used in the microwave frequency range. The characteristics of a serial SQIF have been compared for the first time with those of a single superconducting quantum interference device (SQUID) and a chain of serially connected SQUIDs with equal areas of superconducting loops. The regime of SQIF operation with a voltage-flux ( V -Φ) characteristic determined by the magnetic-field dependence of the critical current in the Josephson junction has been analyzed. It is shown that the output noise of a SQIF measured with a cooled amplifier in the 1–2 GHz range is determined by the slope of the V -Φ characteristic. The influence of a spread in the parameters of Josephson junctions in the SQIF on the integral V -Φ characteristic of the whole structure is considered.
Superconducting quantum interference device (SQUID) is a sensitive detector of magnetic flux signals. Up to now, the main application of SQUIDs has been measurements of magnetic flux signals in the frequency range from near DC to several MHz. Recently, cryogenic low-noise radio-frequency (RF) amplifiers based on DC SQUID are under development aiming to detect RF signals with sensitivity approaching quantum limit. In this paper, we review the recent progress of cryogenic low-noise RF amplifiers based on SQUID technology.
Radio-frequency (RF) amplifiers based on direct current (DC) superconducting quantum interference device (SQUID) have low-noise performance for precision physics experiments. Gain curves of SQUID RF amplifiers depend on several parameters of the SQUID and operation conditions. We are developing SQUID RF amplifiers for application to measure very weak RF signals from ultra-low-temperature high-magnetic-field microwave cavity in axion search experiments. In this study, we designed, fabricated and characterized SQUID RF amplifiers with different SQUID parameters, such as number of input coil turn, shunt resistance value of the junction and coupling capacitance in the input coil, and compared the results.