Statistics – Computation
Scientific paper
Apr 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..apr.m1102p&link_type=abstract
American Physical Society, APS/AAPT Joint April Meeting, April 18-21, 1998 Columbus, Ohio, abstract #M11.02
Statistics
Computation
Scientific paper
The strong field late stage inspiral of a pair of comparable mass black holes provides one of the most interesting possible source of detectable gravitational waves. How important such systems will be to observations depends not only on the astrophysical question of how common black hole binaries are, but also on the answers to some very open questions about the physics of the coalescence of the holes. A discussion will be given of the relationship of the questions of detectability and coalescence details, and of the relationship of two approaches to finding answers: numerical relativity and semi-analytical computations. Recent results will be reported on higher order perturbation theory, and on progress with initially moving and rotating holes.
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