2021
DOI: 10.1119/10.0003534
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An interactive gravitational-wave detector model for museums and fairs

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Cited by 2 publications
(4 citation statements)
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“…The remaining deviation is not statistically significant, but may be due to weak correlations between successive shots, which violate the assumption of independence required for Eq. (11). Overall, the results are consistent with the expected scaling for a predominantly shot noise limited device in the presence of some technical noise.…”
Section: Shot Noise and The Measurement Of Gravitational Wavessupporting
confidence: 84%
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“…The remaining deviation is not statistically significant, but may be due to weak correlations between successive shots, which violate the assumption of independence required for Eq. (11). Overall, the results are consistent with the expected scaling for a predominantly shot noise limited device in the presence of some technical noise.…”
Section: Shot Noise and The Measurement Of Gravitational Wavessupporting
confidence: 84%
“…The resulting signals are so small that measurements in the frequency bands relevant to the final moments of black hole and neutron star mergers are limited by the inherent quantum shot noise of the laser used in the interferometer [13]. Thus there is value in incorporating quantum mechanics into the description of the interferometer, going beyond the classical framework [11] of understanding interferometers with electromagnetic waves. With only one qubit, a quantum circuit model can capture all the salient features of a classical model and demonstrate the effects of quantum projection noise.…”
Section: Ligo As a Quantum Circuitmentioning
confidence: 99%
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