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Numerical relativity simulations in the era of the Einstein Telescope

By Mark Hannam and Ian Hawke

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. <br/

Year: 2009
OAI identifier: oai:eprints.soton.ac.uk:155883
Provided by: e-Prints Soton

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