Project Details
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Co-Evolution of Supermassive Black Holes and Galactic Nuclei

Subject Area Astrophysics and Astronomy
Term from 2007 to 2012
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 42513392
 
Final Report Year 2012

Final Report Abstract

The objectives of the project are to study the dynamical interaction between Supper Massive Black Holes (SMBH) and the surrounding stellar dynamical component in galaxy cores, and outside the region of influence of the Black Hole, by using of realistic N-body techniques. We study the cusp formation, disruption rates and loss-cone theory in time scales of relaxation, which allows us to understand the past, present and possible future evolution of galactic nuclei harboring SMBHs.

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