Quantum Noise Engineering in Advanced LIGO

Abstract:Advanced LIGO is a gravitational-wave detector with extreme sensitivity, operating close to the quantum limits of optical measurement. The quantum noise in this system arises from vacuum fluctuations entering the interferometer readout port: phase-like fluctuations produce measurement imprecision, while amplitude-like fluctuations drive radiation-pressure back-action. In this review, we present an intuitive description in terms of complex fields and quadratures, and follow squeezed vacuum from its generation, through its interaction with the filter cavity and propagation through the interferometer, to the readout. We discuss how frequency-independent and frequency-dependent squeezing engineer quantum noise, and how correlations between optical quadratures map onto correlations between measurement imprecision and back-action. We conclude that LIGO is both a gravitational-wave observatory and a kilometre-scale platform for quantum measurement science.

Submitted to Contemporary Physics. Open source tools developed for this manuscript can be found in: this https URL

Quantum Physics (quant-ph); Instrumentation and Methods for Astrophysics (astro-ph.IM)

arXiv:2611.07074 [quant-ph]

(or arXiv:2611.07074v1 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2611.07074 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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