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Relaxation Processes and Black Holes in Star Clusters and Galactic Nuclei

We use high-precision direct N -body integration to study questions of the thermodynamic be- haviour of dense stellar systems and of the state of dense stellar systems interacting with binary black holes in galactic nuclei. Thermodynamical processes examined include mass segregation and equipartition processes and stellar orbits in galactic nuclei with thick accretion disks.