2006
DOI: 10.1063/1.2168252
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27 ℏ SQUID amplifier operating with high-Q resonant input load

Abstract: We have extended to ultracryogenic temperatures the complete noise characterization of a low-noise two-stage superconducting quantum interference device (SQUID) amplifier developed for resonant gravitational wave detectors. The additive current noise is evaluated from open input measurements. To evaluate the back action voltage noise, the SQUID is strongly coupled to a high-Q macroscopic electrical resonator operating at 11.7 kHz. From these measurements, we estimate a minimum noise temperature of 15μK, corres… Show more

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Cited by 17 publications
(23 citation statements)
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“…5.12 of about ≈ 0.3 K. This suggests that a coupled energy resolution of about 50h is possible. This is close to the optimum performance achieved for the original design [156].…”
Section: Discussionsupporting
confidence: 65%
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“…5.12 of about ≈ 0.3 K. This suggests that a coupled energy resolution of about 50h is possible. This is close to the optimum performance achieved for the original design [156].…”
Section: Discussionsupporting
confidence: 65%
“…The minimum equivalent input noise temperature is not needed for MiniGRAIL. The achievable values in the kHz frequency regime are in the order of µK [156], which is several orders of magnitude below the intended operation temperature of 20 mK. The more interesting properties for MiniGRAIL are the bandwidth and the stability.…”
Section: Design and Characterization Of Dc-squid Amplifiersmentioning
confidence: 99%
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