NbN hot electron bolometric mixers at frequencies between 0.7 and 3.1 THz

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Published under licence by IOP Publishing Ltd
, , Citation Pavel Yagoubov et al 1999 Supercond. Sci. Technol. 12 989 DOI 10.1088/0953-2048/12/11/387

0953-2048/12/11/989

Abstract

The performance of NbN-based phonon-cooled hot electron bolometric (HEB) quasioptical mixers is investigated in the 0.7-3.1 THz frequency range. The devices are made from a 3.5-4 nm thick NbN film on high resistivity Si and integrated with a planar spiral antenna on the same substrate. The length of the bolometer microbridge is 0.1-0.2 µm; the width is 1-2 µm. The best results of the DSB receiver noise temperature measured at 1.5 GHz intermediate frequency are: 800 K at 0.7 THz, 1100 K at 1.6 THz, 2000 K at 2.5 THz and 4200 K at 3.1 THz. The measurements were performed with a far infrared laser as the local oscillator (LO) source. The estimated LO power requirement is less than 500 nW at the receiver input. First results on spiral antenna polarization measurements are reported.

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10.1088/0953-2048/12/11/387