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Exploring the sensitivity of next generation gravitational wave detectors

Abbott, B. P. and Abbott, R. and Adhikari, R. X. and Anderson, S. B. and Arai, K. and Araya, M. C. and Barayoga, J. C. and Barish, B. C. and Berger, B. K. and Billingsley, G. and Blackburn, J. K. and Bork, R. and Brooks, A. F. and Brunett, S. and Cahillane, C. and Callister, T. and Cepeda, C. B. and Chen, Y. and Couvares, P. and Coyne, D. C. and Dergachev, V. and Drever, R. W. P. and Ehrens, P. and Eichholz, J. and Engels, W. and Etzel, T. and Gossan, S. E. and Gushwa, K. E. and Gustafson, E. K. and Hall, E. D. and Heptonstall, A. W. and Isi, M. and Kanner, J. B. and Kells, W. and Kondrashov, V. and Korth, W. Z. and Kozak, D. B. and Lazzarini, A. and Lewis, J. B. and Maros, E. and McIntyre, G. and McIver, J. and Meshkov, S. and Pedraza, M. and Perreca, A. and Price , L. R. and Quintero, E. A. and Reitze, D. H. and Robertson, N. A. and Rollins, J. G. and Sachdev, S. and Sanchez, E. J. and Schmidt, P. and Singer, A. and Smith, N. D. and Smith, R. J. E. and Taylor, R. and Thirugnanasambandam, M. P. and Torrie, C. I. and Vajente, G. and Vass, S. and Wallace, L. and Weinstein, A. J. and Williams, R. D. and Wipf, C. C. and Yamamoto, H. and Zhang, L. and Zucker, M. E. and Zweizig, J. (2017) Exploring the sensitivity of next generation gravitational wave detectors. Classical and Quantum Gravity, 34 (4). Art. No. 044001. ISSN 0264-9381. https://resolver.caltech.edu/CaltechAUTHORS:20170130-122117784

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Abstract

The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/1361-6382/aa51f4DOIArticle
http://iopscience.iop.org/article/10.1088/1361-6382/aa51f4PublisherArticle
https://arxiv.org/abs/1607.08697arXivDiscussion Paper
ORCID:
AuthorORCID
Adhikari, R. X.0000-0002-5731-5076
Billingsley, G.0000-0002-4141-2744
Callister, T.0000-0001-9892-177X
Isi, M.0000-0001-8830-8672
Kanner, J. B.0000-0001-8115-0577
Korth, W. Z.0000-0003-3527-1348
Kozak, D. B.0000-0003-3118-8950
Weinstein, A. J.0000-0002-0928-6784
Williams, R. D.0000-0002-9145-8580
Zucker, M. E.0000-0002-2544-1596
Zweizig, J.0000-0002-1521-3397
Additional Information:© 2017 IOP Publishing. Received 26 September 2016; revised 29 November 2016; accepted for publication 6 December 2016; published 24 January 2017. The authors would like to acknowledge the invaluable wisdom derived from interactions with members of the Virgo and Kagra collaborations without which this work would not have been possible. 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 PHY-0757058. Advanced LIGO was built under award PHY-0823459. This paper carries LIGO Document Number LIGO-P1600143.
Group:LIGO
Funders:
Funding AgencyGrant Number
NSFPHY-0757058
NSFPHY-0823459
Subject Keywords:Gravitational Waves; Cosmic Explorer; LIGO
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentLIGO-P1600143
Issue or Number:4
Record Number:CaltechAUTHORS:20170130-122117784
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170130-122117784
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:73820
Collection:CaltechAUTHORS
Deposited By: Melissa Ray
Deposited On:31 Jan 2017 18:27
Last Modified:03 Oct 2019 16:31

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