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Squeezing in Gravitational Wave Detectors

Dwyer, Sheila E. and Mansell, Georgia L. and McCuller, Lee (2022) Squeezing in Gravitational Wave Detectors. Galaxies, 10 (2). Art. No. 46. ISSN 2075-4434. doi:10.3390/galaxies10020046. https://resolver.caltech.edu/CaltechAUTHORS:20220310-752347000

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Abstract

Injecting optical squeezed states of light, a technique known as squeezing, is now a tool for gravitational wave detection. Its ability to reduce quantum noise is helping to reveal more gravitational wave transients, expanding the catalog of observations in the last observing run. This review introduces squeezing and its history in the context of gravitational-wave detectors. It overviews the benefits, limitations and methods of incorporating squeezing into advanced interferometers, emphasizing the most relevant details for astrophysics instrumentation.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3390/galaxies10020046DOIArticle
ORCID:
AuthorORCID
Dwyer, Sheila E.0000-0002-2068-277X
Mansell, Georgia L.0000-0003-4736-6678
McCuller, Lee0000-0003-0851-0593
Additional Information:© 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Received: 11 January 2022 / Revised: 19 February 2022 / Accepted: 23 February 2022 / Published: 9 March 2022. (This article belongs to the Special Issue Present and Future of Gravitational Wave Astronomy) LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under Cooperative Agreement Grant No. PHY-1764464. Advanced LIGO was built under Grant No. PHY- 0823459. A+ LIGO is being constructed under Grant PHY-1834382. Institutional Review Board Statement: Not applicable. Informed Consent Statement: Not applicable. Data Availability Statement: Not applicable. The authors declare no conflict of interest.
Group:LIGO
Funders:
Funding AgencyGrant Number
NSFPHY-1764464
NSFPHY-0823459
NSFPHY-1834382
Subject Keywords:gravitational waves; squeezed states; quantum optics; interferometer; quantum noise
Issue or Number:2
DOI:10.3390/galaxies10020046
Record Number:CaltechAUTHORS:20220310-752347000
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220310-752347000
Official Citation:Dwyer SE, Mansell GL, McCuller L. Squeezing in Gravitational Wave Detectors. Galaxies. 2022; 10(2):46. https://doi.org/10.3390/galaxies10020046
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:113877
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:15 Mar 2022 16:07
Last Modified:15 Mar 2022 16:07

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