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.
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BibTeX
@misc{kabagoz2026quantum,
title = {{Quantum Noise Engineering in Advanced LIGO}},
author = {Begüm Kabagöz},
howpublished = {arXiv},
year = {2026},
month = nov,
doi = {10.48550/arxiv.2611.07074},
eprint = {2611.07074},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2611.07074},
note = {CC BY-NC-ND 4.0},
}
RIS
TY - UNPB
TI - Quantum Noise Engineering in Advanced LIGO
AU - Begüm Kabagöz
PY - 2026
DA - 2026/11/04
PB - arXiv
DO - 10.48550/arxiv.2611.07074
UR - https://arxiv.org/abs/2611.07074
AB - 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.
ER -