We present measurements of quasiparticle generation-recombination noise in aluminium Microwave Kinetic Inductance Detectors, the fundamental noise source for these detectors. Both the quasiparticle lifetime and the number of quasiparticles can be determined from the noise spectra. The number of quasiparticles saturates to 10 μm−3 at temperatures below 160 mK, which is shown to limit the quasiparticle lifetime to 4 ms. These numbers lead to a generation-recombination noise limited noise equivalent power (NEP) of 1.5×10−19 W/Hz1/2. Since NEP∝Nqp, lowering the number of remnant quasiparticles will be crucial to improve the sensitivity of these detectors. We show that the readout power now limits the number of quasiparticles and thereby the sensitivity.
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Purple Mountain Observatory, Chinese Academy of Sciences
School of Astronomy & Space Science, University of Science and Technology of ChinaPurple Mountain Observatory, Chinese Academy of Sciences
Qing Shi
Jing Li
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Purple Mountain Observatory, Chinese Academy of SciencesPurple Mountain Observatory, Chinese Academy of Sciences
Jing Li
Qiang Zhi
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Purple Mountain Observatory, Chinese Academy of Sciences
School of Astronomy & Space Science, University of Science and Technology of ChinaPurple Mountain Observatory, Chinese Academy of Sciences
Qiang Zhi
Zheng Wang
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Purple Mountain Observatory, Chinese Academy of SciencesPurple Mountain Observatory, Chinese Academy of Sciences
Zheng Wang
Wei Miao
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Purple Mountain Observatory, Chinese Academy of SciencesPurple Mountain Observatory, Chinese Academy of Sciences
Wei Miao
Sheng-Cai Shi
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Purple Mountain Observatory, Chinese Academy of SciencesPurple Mountain Observatory, Chinese Academy of Sciences
机构:
Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Li, J.
Barry, P. S.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Barry, P. S.
Cecil, T.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Cecil, T.
Chang, C. L.
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Argonne Natl Lab, Argonne, IL 60439 USA
Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USAArgonne Natl Lab, Argonne, IL 60439 USA
Chang, C. L.
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Dibert, K.
Gualtieri, R.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Gualtieri, R.
Lisovenko, M.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Lisovenko, M.
Pan, Z.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Pan, Z.
Yefremenko, V.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Yefremenko, V.
Wang, G.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA
Wang, G.
Zhang, J.
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Argonne Natl Lab, Argonne, IL 60439 USAArgonne Natl Lab, Argonne, IL 60439 USA