Modelling Gravitational Radiation from Binary Black Holes

Details Modelling Gravitational Radiation from Binary Black Holes Modelling Gravitational Radiation from Binary Black Holes

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.1204c&link_type=abstract

American Astronomical Society, HEAD meeting #9, #12.04; Bulletin of the American Astronomical Society, Vol. 38, p.366

Astronomy and Astrophysics

Astronomy

Scientific paper

The final merger and coalescence of binary black holes is a key source of strong gravitational waves for the LISA mission. Observing these systems will allow us to probe the formation of cosmic structure to high redshifts and test general relativity directly in the strong-field, dynamical regime.
Recently, major breakthroughs have been made in modeling black hole mergers using numerical relativity. This talk will survey these exciting developments, focusing on the gravitational waveforms and the recoil kicks produced from non-equal mass mergers.

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