Taras Panamarev (Kazakhstan)
taras @ ari.uni-heidelberg.de
Dynamical interaction of Supermassive Black Holes with the surrounding stellar system
We examine the dynamical interaction of supermassive black hole and the surrounding stellar system. We start with implementing black hole potential and effects of stellar accretion in the high accuracy parallel code Nbody6++. The aim is to build the numerical model for the dynamical evolution of a galactic center performing star-by-star simulations and taking into account formation and evolution of binaries. As an application of the model we will study the dynamics of the central parsec region of the Milky Way galaxy. All the simulations will be performed on GPU computer clusters.
Supervisors: Andreas Just / Rainer Spurzem (ARI)