1.Institut für Laserphysik und Zentrum für Optische Quantentechnologien, Universität Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany
2.Theoretical Astrophysics 350-17, California Institute of Technology, Pasadena, CA 91125, USA
Mikhail Korobko (mkorobko@physnet.uni-hamburg.de)
纸质出版日期:2019,
网络出版日期:2019-12-11,
收稿日期:2019-04-15,
修回日期:2019-11-13,
录用日期:2019-11-28
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Quantum expander for gravitational-wave observatories[J]. LSA, 2019,8(6):1152-1159.
Korobko, K. et al. Quantum expander for gravitational-wave observatories. Light: Science & Applications, 8, 1152-1159 (2019).
Quantum expander for gravitational-wave observatories[J]. LSA, 2019,8(6):1152-1159. DOI: 10.1038/s41377-019-0230-2.
Korobko, K. et al. Quantum expander for gravitational-wave observatories. Light: Science & Applications, 8, 1152-1159 (2019). DOI: 10.1038/s41377-019-0230-2.
The quantum uncertainty of laser light limits the sensitivity of gravitational-wave observatories. Over the past 30 years
techniques for squeezing the quantum uncertainty
as well as for enhancing gravitational-wave signals with optical resonators have been invented. Resonators
however
have finite linewidths
and the high signal frequencies that are produced during the highly scientifically interesting ring-down of astrophysical compact-binary mergers still cannot be resolved. Here
we propose a purely optical approach for expanding the detection bandwidth. It uses quantum uncertainty squeezing inside one of the optical resonators
compensating for the finite resonators' linewidths while keeping the low-frequency sensitivity unchanged. This quantum expander is intended to enhance the sensitivity of future gravitational-wave detectors
and we suggest the use of this new tool in other cavity-enhanced metrological experiments.
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