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 |
|---|---|
| Date Type: | Publication |
| Status: | Published |
| Schools: | 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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