中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Quantum noise in a terahertz hot electron bolometer mixer

文献类型:期刊论文

作者Zhang, W.1,2; Khosropanah, P.1; Gao, J. R.1,3; Kollberg, E. L.4; Yngvesson, K. S.5; Bansal, T.1,3; Barends, R.3; Klapwijk, T. M.3
刊名APPLIED PHYSICS LETTERS
出版日期2010-03-15
卷号96期号:11页码:111113
关键词bolometers millimetre wave mixers quantum noise
ISSN号0003-6951
英文摘要We have measured the noise temperature of a single, sensitive superconducting NbN hot electron bolometer (HEB) mixer in a frequency range from 1.6 to 5.3 THz, using a setup with all the key components in vacuum. By analyzing the measured receiver noise temperature using a quantum noise (QN) model for HEB mixers, we confirm the effect of QN. The QN is found to be responsible for about half of the receiver noise at the highest frequency in our measurements. The beta-factor (the quantum efficiency of the HEB) obtained experimentally agrees reasonably well with the calculated value.
WOS标题词Science & Technology ; Physical Sciences
学科主题Physics
类目[WOS]Physics, Applied
研究领域[WOS]Physics
收录类别SCI
语种英语
WOS记录号WOS:000275825200013
公开日期2011-11-23
源URL[http://159.226.72.40/handle/332002/997]  
专题紫金山天文台_毫米波和亚毫米波技术实验室
作者单位1.Univ Groningen, SRON Netherlands Inst Space Res, NL-9747 AD Groningen, Netherlands
2.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
3.Delft Univ Technol, Kavli Inst Nanosci, NL-2628 CJ Delft, Netherlands
4.Chalmers, Dept Microelect & Nanosci, SE-41296 Gothenburg, Sweden
5.Univ Massachusetts, Dept Elect & Comp Engn, Amherst, MA 01003 USA
推荐引用方式
GB/T 7714
Zhang, W.,Khosropanah, P.,Gao, J. R.,et al. Quantum noise in a terahertz hot electron bolometer mixer[J]. APPLIED PHYSICS LETTERS,2010,96(11):111113.
APA Zhang, W..,Khosropanah, P..,Gao, J. R..,Kollberg, E. L..,Yngvesson, K. S..,...&Klapwijk, T. M..(2010).Quantum noise in a terahertz hot electron bolometer mixer.APPLIED PHYSICS LETTERS,96(11),111113.
MLA Zhang, W.,et al."Quantum noise in a terahertz hot electron bolometer mixer".APPLIED PHYSICS LETTERS 96.11(2010):111113.

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来源:紫金山天文台

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