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3-mode detection for widening the bandwidth of resonant gravitational wave detectors
General Relativity and Quantum Cosmology · Submitted 24 Feb 2005
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The resulting 3-mode detection scheme widens significantly the bandwidth of the detector.
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The abstract, sentence by sentence
We have implemented a novel scheme of signal readout for resonant gravitational wave detectors. For the first time, a capacitive resonant transducer has been matched to the signal amplifier by means of a tuned high Q electrical resonator. The resulting 3-mode detection scheme widens significantly the bandwidth of the detector. We present here the results achieved by this signal readout equipped with a two-stage SQUID amplifier. Once installed on the AURIGA detector, the one-sided spectral sensitivity obtained with the detector operated at 4.5 K is better than 10^-20 Hz^-1/2 over 110 Hz and in good agreement with the expectations.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We have implemented a novel scheme of signal readout for resonant gravitational wave detectors. | contribution 0.99 | 0.95 | 0.06 | asserted 1.00 |
| s1 | For the first time, a capacitive resonant transducer has been matched to the signal amplifier by means of a tuned high Q electrical resonator. | method 0.51 | 0.89 | 0.06 | asserted 1.00 |
| s2 | The resulting 3-mode detection scheme widens significantly the bandwidth of the detector. | result 0.79 | 0.84 | 0.77 | asserted 1.00 |
| s3 | We present here the results achieved by this signal readout equipped with a two-stage SQUID amplifier. | contribution 0.64 | 0.90 | 0.07 | asserted 0.94 |
| s4 | Once installed on the AURIGA detector, the one-sided spectral sensitivity obtained with the detector operated at 4.5 K is better than 10^-20 Hz^-1/2 over 110 Hz and in good agreement with the expectations. | result 1.00 | 0.95 | 0.28 | asserted 1.00 |
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Original abstract
We have implemented a novel scheme of signal readout for resonant gravitational wave detectors. For the first time, a capacitive resonant transducer has been matched to the signal amplifier by means of a tuned high Q electrical resonator. The resulting 3-mode detection scheme widens significantly the bandwidth of the detector. We present here the results achieved by this signal readout equipped with a two-stage SQUID amplifier. Once installed on the AURIGA detector, the one-sided spectral sensitivity obtained with the detector operated at 4.5 K is better than 10^-20 Hz^-1/2 over 110 Hz and in good agreement with the expectations.
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