4.7-THz Superconducting Hot Electron Bolometer Waveguide Mixer

We present the first superconducting hot electron bolometer (HEB) waveguide mixer operating at 4.7 THz. The 5.5-nm-thick, 300-nm-long, and 3600-nm-wide NbN HEB microbridge is integrated into a normal metal (Au) planar circuit on a 2 μm thick silicon substrate. This circuit is integrated in a 24 μm ×...

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Veröffentlicht in:IEEE transactions on terahertz science and technology 2015-03, Vol.5 (2), p.207-214
Hauptverfasser: Buchel, Denis, Putz, Patrick, Jacobs, Karl, Schultz, Michael, Graf, Urs U., Risacher, Christophe, Richter, Heiko, Ricken, Oliver, Hubers, Heinz-Wilhelm, Gusten, Rolf, Honingh, Cornelia E., Stutzki, Jurgen
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Sprache:eng
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Zusammenfassung:We present the first superconducting hot electron bolometer (HEB) waveguide mixer operating at 4.7 THz. The 5.5-nm-thick, 300-nm-long, and 3600-nm-wide NbN HEB microbridge is integrated into a normal metal (Au) planar circuit on a 2 μm thick silicon substrate. This circuit is integrated in a 24 μm × 48 μm × 21 μm waveguide cavity and a 14 μm × 7 μm × 200 μm substrate channel, which is directly machined into a CuTe alloy block. The power spectrum of the HEB mixer, measured with a Fourier transform spectrometer, is in good agreement with the results of 3-D EM circuit simulation. Measured mixer performance shows a state-of-the-art double sideband noise temperature of 1100 K, averaged over the IF bandwidth of 0.2-3.5 GHz. The 3-dB noise roll-off is 3.5 GHz. This mixer is used in the German REceiver for Astronomy at Terahertz frequencies (GREAT) at the airborne Stratospheric Observatory for Far Infrared Astronomy (SOFIA).
ISSN:2156-342X
2156-3446
DOI:10.1109/TTHZ.2014.2382434