Dynamics of One or Two Black Holes in Galactic Nuclei

Mathematics – Logic

Scientific paper

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Scientific paper

The idealized theoretical background on the growth and dynamics of a single star-accreting black hole in galactic nuclei is reviewed. We then discuss how the standard picture changes in a modern cosmological view, where galaxies (and their nuclei with black holes) merge; as a model of such a merger product detailed self-consistent N-body models using a new hybrid direct and field code of nuclei containing binary black holes are presented. They follow the sinking of two massive black holes in a spherical stellar system under dynamical friction and, once a bound binary black hole has formed, under stochastic three-body interactions with the surrounding stellar system. The induced core motions of the nucleus are discussed.

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