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Quantum correlation measurements in interferometric gravitational-wave detectors

Martynov, D. V. and Abbott, B. P. and Abbott, R. and Adhikari, R. X. and Anderson, S. B. and Ananyeva, A. and Appert, S. and Arai, K. and Billingsley, G. and Biscans, S and Bork, R. and Brooks, A. F. and Coyne, D. C. and Etzel, T. and Gushwa, K. E. and Gustafson, E. K. and Hall, E. D. and Heptonstall, A. W. and Korth, W. Z. and Maros, E. and Matichard, F. and McIntyre, G. and McIver, J. and Quintero, E. A. and Reitze, D. H. and Robertson, N. A. and Rollins, J. G. and Sanchez, E. J. and Taylor, R. and Torrie, C. I. and Vajente, G. and Wipf, C. C. and Yamamoto, H. and Zhang, L. and Zucker, M. E. and Zweizig, J. (2017) Quantum correlation measurements in interferometric gravitational-wave detectors. Physical Review A, 95 (4). Art. No. 043831. ISSN 2469-9926. http://resolver.caltech.edu/CaltechAUTHORS:20170421-132510454

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Abstract

Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitivity of modern optical instruments. The sensitivity of the interferometric gravitational-wave detectors, such as the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO), is limited by quantum shot noise, quantum radiation pressure noise, and a set of classical noises. We show how the quantum properties of light can be used to distinguish these noises using correlation techniques. Particularly, in the first part of the paper we show estimations of the coating thermal noise and gas phase noise, hidden below the quantum shot noise in the Advanced LIGO sensitivity curve. We also make projections on the observatory sensitivity during the next science runs. In the second part of the paper we discuss the correlation technique that reveals the quantum radiation pressure noise from the background of classical noises and shot noise. We apply this technique to the Advanced LIGO data, collected during the first science run, and experimentally estimate the quantum correlations and quantum radiation pressure noise in the interferometer.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevA.95.043831DOIArticle
https://journals.aps.org/pra/abstract/10.1103/PhysRevA.95.043831PublisherArticle
https://arxiv.org/abs/1702.03329arXivDiscussion Paper
ORCID:
AuthorORCID
Adhikari, R. X.0000-0002-5731-5076
Billingsley, G.0000-0002-4141-2744
Korth, W. Z.0000-0003-3527-1348
Zucker, M. E.0000-0002-2544-1596
Zweizig, J.0000-0002-1521-3397
Additional Information:© 2017 American Physical Society. Received 14 February 2017; published 21 April 2017. The authors gratefully acknowledge the support of the United States National Science Foundation (NSF). D.V.M. would like to thank the Kavli Foundation for the support provided by a Kavli fellowship. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the NSF and operates under Cooperative Agreement No. PHY-0757058. The Advanced LIGO was built under Award No. PHY-0823459.
Group:LIGO
Funders:
Funding AgencyGrant Number
Kavli FoundationUNSPECIFIED
NSFPHY-0757058
NSFPHY-0823459
Record Number:CaltechAUTHORS:20170421-132510454
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170421-132510454
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:76820
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Apr 2017 20:43
Last Modified:16 Nov 2017 23:05

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