Galaxy mergers and implications for massive black hole binary coalescence

Details Galaxy mergers and implications for massive black hole binary coalescence Galaxy mergers and implications for massive black hole binary coalescence

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cqgra..14.1431v&link_type=abstract

Classical and Quantum Gravity, Volume 14, Issue 6, pp. 1431-1437 (1997).

Physics

12

Scientific paper

Massive black hole binaries are one of the most interesting classes of sources that could be detectable by LISA, as they allow tests of general relativity in strong-field conditions and to probe into the very centre of galactic nuclei. We review our present knowledge about the scenario that leads to the formation of these systems and the event rate of detectable gravitational wave signals. We also discuss the use of a LISA-observation catalogue to gain information on the mass - redshift distribution of sources.

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