The Heisenberg uncertainty principle states that the position of an object cannot be known with infinite precision, as the momentum of the object would then be totally uncertain. This momentum uncertainty then leads to position uncertainty in future measurements. When continuously measuring the position of an object, this quantum effect, known as back-action, limits the achievable precision1,2. In audio-band, interferometer-type gravitational-wave detectors, this back-action effect manifests as quantum radiation pressure noise (QRPN) and will ultimately (but does not yet) limit sensitivity3. Here, we present the use of a quantum engineered state of light to directly manipulate this quantum back-action in a system where it dominates the sensitivity in the 10–50 kHz range. We observe a reduction of 1.2 dB in the quantum back-action noise. This experiment is a crucial step in realizing QRPN reduction for future interferometric gravitational-wave detectors and improving their sensitivity.
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This research was supported by the Australian Research Council under the Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery grant no. CE170100004 and ARC Discovery Project DP160100760. J.C. and T.C. are supported by the National Science Foundation (NSF; grants nos. PHY-1150531 and PHY-1806634). The microresonator manufacturing was carried out at the University of California, Santa Barbara (UCSB) Nanofabrication Facility. M.J.Y. thanks D. Shaddock for initial discussions.
The authors declare no competing interests.
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Yap, M.J., Cripe, J., Mansell, G.L. et al. Broadband reduction of quantum radiation pressure noise via squeezed light injection. Nat. Photonics 14, 19–23 (2020). https://doi.org/10.1038/s41566-019-0527-y
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