Noise temperature and local oscillator power requirement of NbN phonon-cooled hot electron bolometric mixers at terahertz frequencies

被引:20
作者
Yagoubov, P [1 ]
Kroug, M
Merkel, H
Kollberg, E
Gol'tsman, G
Svechnikov, S
Gershenzon, E
机构
[1] Chalmers Univ Technol, S-41296 Gothenburg, Sweden
[2] Moscow State Pedag Univ, Moscow 119435, Russia
关键词
D O I
10.1063/1.122599
中图分类号
O59 [应用物理学];
学科分类号
摘要
In this letter, the noise performance of NbN-based phonon-cooled hot electron bolometric quasioptical mixers is investigated in the 0.55-1.1 THz frequency range. The best results of the double-sideband (DSB) noise temperature are: 500 K at 640 GHz, 600 K at 750 GHz, 850 K at 910 GHz, and 1250 K at 1.1 THz. The water vapor in the signal path causes significant contribution to the measured receiver noise temperature around 1.1 THz. The devices are made from 3-nm-thick NbN film on high-resistivity Si and integrated with a planar spiral antenna on the same substrate. The in-plane dimensions of the bolometer strip are typically 0.2x2 mu m. The amount of local oscillator power absorbed in the bolometer is less than 100 nW. (C) 1998 American Institute of Physics. [S0003-6951(98)03545-1].
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页码:2814 / 2816
页数:3
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