Strong-lensing of gravitational waves by galaxy clusters

Smith, G. P. et al. (2019) Strong-lensing of gravitational waves by galaxy clusters. Proceedings of the International Astronomical Union, 13(S338), pp. 98-102. (doi: 10.1017/S1743921318003757)

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Abstract

Discovery of strongly-lensed gravitational wave (GW) sources will unveil binary compact objects at higher redshifts and lower intrinsic luminosities than is possible without lensing. Such systems will yield unprecedented constraints on the mass distribution in galaxy clusters, measurements of the polarization of GWs, tests of General Relativity, and constraints on the Hubble parameter. Excited by these prospects, and intrigued by the presence of so-called "heavy black holes" in the early detections by LIGO-Virgo, we commenced a search for strongly-lensed GWs and possible electromagnetic counterparts in the latter stages of the second LIGO observing run (O2). Here, we summarise our calculation of the detection rate of strongly-lensed GWs, describe our review of BBH detections from O1, outline our observing strategy in O2, summarize our follow-up observations of GW170814, and discuss the future prospects of detection.

Item Type:Articles
Additional Information:IAU Symposium 16-19 October 2017, Baton Rouge, United States
Status:Published
Refereed:No
Glasgow Author(s) Enlighten ID:Veitch, Dr John and Berry, Dr Christopher
Authors: Smith, G. P., Berry, C., Bianconi, M., Farr, W. M., Jauzac, M., Massey, R., Richard, J., Robertson, A., Sharon, K., Vecchio, A., and Veitch, J.
Subjects:Q Science > QB Astronomy
Q Science > QC Physics
College/School:College of Science and Engineering > School of Physics and Astronomy
Research Group:Institute for Gravitational Research
Journal Name:Proceedings of the International Astronomical Union
Publisher:Cambridge University Press
ISSN:1743-9213
ISSN (Online):1743-9221
Copyright Holders:Copyright © 2019 International Astronomical Union
First Published:First published in Proceedings of the International Astronomical Union 13(S338):98-102
Publisher Policy:Reproduced in accordance with the copyright policy of the publisher
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