Physics
Scientific paper
Mar 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..apr.q8007m&link_type=abstract
American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #Q8.007
Physics
Scientific paper
Numerical simulations of black hole binaries (BH-BH) have matured at an astonishing rate over the last years. Nevertheless, there is a pronounced dearth of accurate simulations covering many inspiral orbits for precessing BH-BH binaries. This talk reports on an effort to significantly increase the number of high-quality BH-BH waveforms using the Spectral Einstein code (black-holes.ord/SpEC). We will describe our approach to efficiently compute low-eccentricity orbital parameters, detail our current set of simulations, and present first scientific results from these simulations, focusing on the inspiral phase of the BH-BH.
Mroue Abdul
Pfeiffer Harald
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