The Dynamical Evolution of Dense Clusters of Compact Stars
Abstract
Results of Fokker-Planck calculations of the dynamical evolution of a dense cluster of compact stars (neutron stars or black holes) are presented. The dominant physical process is the dissipative formation of binaries through gravitational radiation emission and their subsequent merger, which results in the runaway buildup of a massive 'seed' black hole. The binary systems that form are promising sources of gravitational radiation for detection by ground-based laser interferometers. The ultimate fate of the cluster is discussed.
- Publication:
-
Dynamics of Dense Stellar Systems
- Pub Date:
- 1989
- Bibcode:
- 1989ddse.work..113Q
- Keywords:
-
- Black Holes (Astronomy);
- Fokker-Planck Equation;
- Neutron Stars;
- Star Clusters;
- Stellar Evolution;
- Stellar Motions;
- Active Galactic Nuclei;
- Binary Stars;
- Computerized Simulation;
- Gravitational Collapse;
- Laser Interferometry;
- Red Shift;
- Astrophysics