Hannam, Mark ORCID: https://orcid.org/0000-0001-5571-325X and Hawke, Ian 2011. Numerical relativity simulations in the era of the Einstein Telescope. General Relativity and Gravitation 43 (2) , pp. 465-483. 10.1007/s10714-010-1008-2 |
Official URL: http://dx.doi.org/10.1007/s10714-010-1008-2
Abstract
Numerical-relativity (NR) simulations of compact binaries are expected to be an invaluable tool in gravitational-wave 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.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | Numerical relativity; Black holes; Neutron stars; Einstein Telescope |
Publisher: | Springer Verlag |
ISSN: | 0001-7701 |
Last Modified: | 20 Oct 2022 07:55 |
URI: | https://orca.cardiff.ac.uk/id/eprint/26920 |
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