Numerical relativity simulations in the era of the Einstein Telescope
Numerical relativity simulations in the era of the Einstein Telescope
Numerical-relativity (NR) simulations of compact binaries are expected to be an invaluable tool in gravitational-wave (GW) astronomy. The sensitivity of future detectors such as the Einstein Telescope (ET) will place much higher demands on NR simulations than first- and second-generation ground-based detectors. We discuss the issues facing compact-object simulations over the next decade, with an emphasis on estimating where the accuracy and parameter space coverage will be sufficient for ET and where significant work is needed.
465-483
Hannam, Mark
fdf732dc-e968-4b09-8262-7f4a0cb8f08e
Hawke, Ian
fc964672-c794-4260-a972-eaf818e7c9f4
21 August 2009
Hannam, Mark
fdf732dc-e968-4b09-8262-7f4a0cb8f08e
Hawke, Ian
fc964672-c794-4260-a972-eaf818e7c9f4
Hannam, Mark and Hawke, Ian
(2009)
Numerical relativity simulations in the era of the Einstein Telescope.
General Relativity and Gravitation, 43 (2), .
(doi:10.1007/s10714-010-1008-2).
Abstract
Numerical-relativity (NR) simulations of compact binaries are expected to be an invaluable tool in gravitational-wave (GW) astronomy. The sensitivity of future detectors such as the Einstein Telescope (ET) will place much higher demands on NR simulations than first- and second-generation ground-based detectors. We discuss the issues facing compact-object simulations over the next decade, with an emphasis on estimating where the accuracy and parameter space coverage will be sufficient for ET and where significant work is needed.
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Published date: 21 August 2009
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Imported from arXiv
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Local EPrints ID: 155883
URI: http://eprints.soton.ac.uk/id/eprint/155883
ISSN: 0001-7701
PURE UUID: 041f149b-3227-4eee-aad3-34b500292ee0
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Date deposited: 28 May 2010 15:50
Last modified: 14 Mar 2024 02:50
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Author:
Mark Hannam
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