Authors: Mark Hannam, Ian Hawke
Date: 21 Aug 2009
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.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis