1995
DOI: 10.1103/physrevlett.74.1908
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High Sensitivity Gravitational Wave Antenna with Parametric Transducer Readout

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Cited by 183 publications
(129 citation statements)
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“…Various resonant mass detectors are now operating [21][22][23][24][25]. In [38], the first experiment of cross-correlation…”
Section: A Gw Detectors and Bbn Boundmentioning
confidence: 99%
See 1 more Smart Citation
“…Various resonant mass detectors are now operating [21][22][23][24][25]. In [38], the first experiment of cross-correlation…”
Section: A Gw Detectors and Bbn Boundmentioning
confidence: 99%
“…The experimental efforts are converging towards the possibility of direct detection of stochastically distributed gravitational waves [19,20]. Various resonant mass detectors are now operating at a typical frequency of the order of kHz (Allegro [21], Auriga [22], Explorer [23], Nautilus [24], Niobe [25]) and four Michelson interferometers (GEO-600 [26],TAMA-400 [27], LIGO [29] and VIRGO [28]) will soon be operating in a wide frequency band from a few Hz up to 10 kHz. It is interesting, in the context of ABBN, to elaborate on the possibility that the additional relativistic species are of gravitational origin.…”
Section: Introductionmentioning
confidence: 99%
“…Two key requirements to enter this quantum regime are the capacities to efficiently quantum control the oscillator and to achieve zeropoint-motion-limited transduction sensitivity. Strong electrical actuation of mechanical oscillators, an enabling step for quantum control, has been achieved in nanoelectromechanical systems (NEMS) [10][11][12][13][14][15][16]. Furthermore, transduction sensitivities near the quantum limit have been reached with cavity optomechanical systems (COMS) [17,18].…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, optical heating via optical absorption of intracavity power severely constrains the possibility of operation in the quantum regime [18]. By contrast, electrical actuation of NEMS is inherently strong, much less prone to heating effects, and comparatively straightforward to implement [10,12,13,15,30].…”
Section: Introductionmentioning
confidence: 99%
“…Observation runs have already been performed in several interferometer (LIGO [1], VIRGO [2], GEO [3], TAMA [4], CLIO [5]) and resonator (ALLEGRO [6], EX-PLORER [7], NAUTILUS [8], AURIGA [9], NIOBE [10], MARIO SCHENBERG [11]) projects. In order of gravitational wave detection, the reduction of noise and fake triggers is crucial, since the gravitational wave amplitude and number of events are expected to be small and rare.…”
Section: Introductionmentioning
confidence: 99%