Physics
Scientific paper
Mar 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..apr.q8008s&link_type=abstract
American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #Q8.008
Physics
Scientific paper
The Caltech-Cornell-CITA Spectral Einstein Code has, in the past years, matured to the point where the simulation of the full binary black hole problem (inspiral, merger, ringdown) ceases to require a significant amount of human interaction. This, combined with the low CPU-hour cost of these runs, allows SpEC to enter ``mass-production mode.'' I will discuss some of the technicalities involved in obtaining a robust algorithm. I will present measures of code accuracy in this mass-production context, as seen in the black hole physical characteristics as well as the wave-forms.
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