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Applied Physics Letters

Heterodyne mixing with Nb tunnel junctions above the gap frequency

Gert J. de Lange, Cornelia E. Honingh, J. J. Kuipers, H. Schaeffer, R. A. Panhuyzen, T. M. Klapwijk, Herman van de Stadt, M. W. M. de Graauw

Published May 30, 1994• 38 citations
Publisher

Abstract

The noise and gain of a heterodyne waveguide mixer employing Nb/Al2O3/Nb superconducting tunnel junctions with an on-chip integrated tuning element are measured and analyzed at 680–750 GHz and at 840 GHz. The lowest receiver noise temperatures are 400 K (double side band) at 720 GHz and 1500 K (3000 K including the beam splitter loss) at 840 GHz. We compare data of the pumped I–V curves with the quantum theory of mixing and demonstrate good agreement at frequencies well above the gap frequency.

DOI
10.1063/1.111399

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•Jan 1, 1992•1 citation
The noise and gain of a heterodyne waveguide mixer employing Nb/Al2O3/Nb superconducting tunnel junctions with an on-chip integrated tuning element are measured and analyzed at 680–750 GHz and at 840 GHz. The lowest receiver noise temperatures are 400 K (double side band) at 720 GHz and 1500 K (3000 K including the beam splitter loss) at 840 GHz. We compare data of the pumped I–V curves with the quantum theory of mixing and demonstrate good agreement at frequencies well above the gap frequency.
The noise and gain of a heterodyne waveguide mixer employing Nb/A120JNb superconducting tunnel junc- tions is measured in the 400-500 GHz frequency range. Three different arrays of two junctions in series are analyzed. An array with integrated tuning stubs has lowest receiver noise temperatures of T, = 120 K DSB at 480 GHz, which is to our knowledge the lowest value reported in this frequency range. We compare data of the pumped I-V curves with the Wert- hamer-Tucker theory and demonstrate for the first time an excellent agreement at frequencies up to 500 GHz. For an array without integrated tuning stubs, a mixer noise tempe- rature T- = 90 f 30 K and a DSB mixer gain G-= -12.5 f 0.6 dB is measured. A comparison of the measured gain versus bias voltage with the quantum theory of mixing shows a good qualitative agreement, indicating the applicability of this theory, to Nb tunnel junctions up to 500 GHz. The noise temperature of an array with a lower gap voltage, is 220 K at 495 GHz. This frequency is 85 % of the reduced gap frequen- cy, indicating that Nb SIS mixers can be used up to at least the gap frequency of 680 GHz. I. INTRODUCTION
The noise and gain of a heterodyne waveguide mixer using Nb/Al/sub 2/O/sub 3//Nb superconducting tunnel junctions were measured in the 400-500-GHz frequency range. Three different arrays of two junctions in series are analyzed. The minimum receiver noise temperature is 120 K DSB at 480 GHz, measured with an array having integrated tuning stubs. The authors compare data of the pumped I-V curves with the Werthammer-Tucker theory and demonstrate an excellent agreement at frequencies up to 500 GHz. For an array without integrated tuning stubs. a mixer noise temperature of 90+or-30 K and a DSB mixer gain of -12.5+or-0.6 dB were measured. A comparison of the measured gain versus bias voltage with the quantum theory of mixing shows good qualitative agreement, indicating the applicability of this theory to Nb tunnel junctions up to 500 GHz. The noise temperature of an array with a lower gap voltage is 220 K at 495 GHz. This frequency is 85% of the reduced gap frequency, indicating that Nb superconductor insulator-superconductor (SIS) mixers can be used up at least the gap frequency of 680 GHz.>
We have built a waveguide SIS mixer with Nb-based parallel-connected twin junctions at 800 GHz which is above the gap frequency of Nb (690 GHz). Heterodyne mixing was performed at 810 GHz and a receiver noise temperature of 580 K (DSB), which includes noise contributions due to a vacuum window and a beam splitter, was achieved using Nb/AlO/sub x//Nb junctions with Nb striplines. The performance of this mixer is quite good and it is shown that efficient mixing in Nb-based SIS junctions is still possible above the gap frequency, SIS mixers with Al striplines have also been fabricated and good DC I-V characteristics have been observed. Heterodyne measurements of these mixers are now under preparation.
We report recent results on a 580-740 GHz SIS heterodyne receiver employing a tuned 0.50Am Nb/A10x/Nb SIS tunnel junction. The receiver has been successfully installed at the Caltech Submillimeter Observatory, Hawaii. Results of an untuned device in the same waveguide block were presented at the fifth International THz Conference. Since the mixer is meant to be operated near the superconducting gap frequency of niobium (2,L/h 690 GHz), special has been taken to minimize the absorption loss in the rf matching network. To this effect we propose the use of a RF matching network that constitutes a hybrid between the well know end-loaded stub and radial stub matching networks. We have measured uncorrected DSB receiver temperatures as low as 160K from 680to 702 Gliz, 200K at 725GHz and 120K from 585-640 GHz. The uncorrected mixer noise temperature at 702 Gliz is about 125K, of which 62K can be directly contributed to the front end optics loss. Mixer conversion loss at 702 GHz is 7dB, of which 0.9dB is due to the absorption loss in the Nb film. This results in a corrected mixer noise temperature of 63K, 1.7 times the quantum noise limit.
The authors have made a detailed study of the gain and noise of a SIS (superconductor-insulator-superconductor) heterodyne receiver at 345 GHz. An array of two Nb-Al/sub 2/O/sub 3/-Nb SIS junctions in series are used as the mixing element. The array is operated in a waveguide mount with a backshort and an E-plane tuner. The best receiver noise temperature achieved is 140 K DSB (double sideband). The embedding impedances were determined by fitting theory to the measured pumped curves. High-quality fits were obtained, providing the first detailed test of the Tucker-theory at frequencies above 300 GHz. The impedances found by this method are in very good agreement with impedances measured in a scale model at 3.3 GHz. From these embedding impedances, the gain and noise of the mixer were calculated over a full bias range using the Tucker theory in the three-port low-IF approximation. The measured dependence of mixer gain and noise on bias voltage, pump power and embedding impedance is in good agreement with theory. However the absolute values show discrepancies that appear to be independent of the bias parameters of the mixer.>
The measured gain and noise of a SIS waveguide mixer at 345 GHz have been compared with theoretical values, calculated from the quantum mixer theory using a three port model. As a mixing element, we use a series array of two Nb-Al2O3-Nb SIS junctions. The area of each junction is 0.8 sq microns and the normal state resistance is 52 omega. The embedding impedance of the mixer has been determined from the pumped DC-IV curves of the junction and is compared to results from scale model measurements (105 x). Good agreement was obtained. The measured mixer gain, however, is a factor of 0.45 plus or minus 0.5 lower than the theoretical predicted gain. The measured mixer noise temperature is a factor of 4-5 higher than the calculated one. These discrepancies are independent on pump power and are valid for a broad range of tuning conditions.