Modelling binary black-hole coalescence

Details Modelling binary black-hole coalescence Modelling binary black-hole coalescence

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cqgra..20s.201b&link_type=abstract

Classical and Quantum Gravity, Volume 20, Issue 10, pp. S201-S208 (2003).

Physics

3

Scientific paper

The final burst of radiation from the coalescence of two supermassive black holes produces extraordinary gravitational wave luminosity making these events visible to LISA even out to large redshift. Interpreting such observations will require detailed theoretical models, based on general relativity. The effort to construct these models is just beginning to produce results. I describe the Lazarus approach to modelling these radiation bursts, and present recent results which indicate that the system loses, in the last few wave cycles, about 3% of its mass-energy as strongly polarized gravitational radiation.

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