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3-mode detection for widening the bandwidth of resonant gravitational wave detectors

L. Baggio·M. Bignotto·M. Bonaldi·M. Cerdonio·L. Conti·P. Falferi·N. Liguori·A. Marin·R. Mezzena·A. Ortolan·S. Poggi·G. A. Prodi·F. Salemi·G. Soranzo·L. Taffarello·G. Vedovato·A. Vinante·S. Vitale·J. P. Zendri
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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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L. Baggio, M. Bignotto, M. Bonaldi, M. Cerdonio, L. Conti, P. Falferi, N. Liguori, A. Marin, R. Mezzena, A. Ortolan, S. Poggi, G. A. Prodi, F. Salemi, G. Soranzo, L. Taffarello, G. Vedovato, A. Vinante, S. Vitale, J. P. Zendri. 2005-02-24. 3-mode detection for widening the bandwidth of resonant gravitational wave detectors. https://doi.org/10.1103/physrevlett.94.241101

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