Energy and angular momentum radiated for non head-on binary black hole collisions
arXiv:gr-qc/0205027 · doi:10.1103/PhysRevD.66.104017
Abstract
We investigate the possible total radiated energy produced by a binary black hole system containing non-vanishing total angular momentum. For the scenearios considered we find that the total radiated energy does not exceed 1%. Additionally we explore the gravitational radiation field and the variation of angular momentum in the process.
9 pages, 2 figures
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Cited by in corpus (5)
- Black-hole horizons as probes of black-hole dynamics I: post-merger recoil in head-on collisions
- Numerical evolution of general Robinson-Trautman spacetimes: code tests, wave forms and the efficiency of the gravitational wave extraction
- Gravitational wave recoil in Robinson-Trautman spacetimes
- Perturbations with angular momentum of Robinson-Trautman spacetimes
- Symmetries of the Robinson-Trautman equation