A driven, shielded electromagnetic deflector can create propagating dark-matter millicharge and millicurrent waves that penetrate shields and are detectable with resonant LC circuits, extending direct-detection reach to sub-MeV masses.
3-mode detection for widening the bandwidth of resonant gravitational wave detectors
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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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hep-ph 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
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Direct Deflection of Particle Dark Matter
A driven, shielded electromagnetic deflector can create propagating dark-matter millicharge and millicurrent waves that penetrate shields and are detectable with resonant LC circuits, extending direct-detection reach to sub-MeV masses.