Stellar Relaxation Processes Near the Galactic Massive Black Hole
arXiv:0708.0688
Abstract
The massive black hole (MBH) in the Galactic Center and the stars around it form a unique stellar dynamics laboratory for studying how relaxation processes affect the distribution of stars and compact remnants and lead to close interactions between them and the MBH. Recent theoretical studies suggest that processes beyond "minimal" two-body relaxation may operate and even dominate relaxation and its consequences in the Galactic Center. I describe loss-cone refilling by massive perturbers, strong mass segregation and resonant relaxation; review observational evidence that these processes play a role in the Galactic Center; and discuss some cosmic implications for the rates of gravitational wave emission events from compact remnants inspiraling into MBHs, and the coalescence timescales of binary MBHs.
Invited talk. To appear in "2007 STScI spring symposium: Black Holes", eds, M. Livio & A. M. Koekemoer, Cambridge University Press, in press. 25 pages, 13 figures
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Cited by in corpus (6)
- An Extremely Top-Heavy IMF in the Galactic Center Stellar Disks
- The spin-flip phenomenon in supermassive black hole binary mergers
- Observing white dwarfs orbiting massive black holes in the gravitational wave and electro-magnetic window
- HST Observations of the Stellar Distribution Near Sgr A*
- Extreme mass ratio inspirals: perspectives for their detection
- Massive Young Stars in the Galactic Center