N-body simulations of IMBH Formation

Details N-body simulations of IMBH Formation N-body simulations of IMBH Formation

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...6e..12b&link_type=abstract

Neutron Stars and Black Holes in Star Clusters, 26th meeting of the IAU, Joint Discussion 6, 17-18 August 2006, Prague, Czech Re

Physics

Scientific paper

I will present results of N-body simulations of the dynamical evolution of young star clusters. Conditions under which run-away merging can lead to the growth of intermediate-mass black holes are illustrated for low and high mass clusters. I will then show how clusters containing intermediate-mass black holes evolve at later times. Special attention will be paid to the central density and velocity profile which arises as a result of the black hole and on the chances of observing IMBHs in galactic globular clusters.

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