Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2002-06-03
Phys.Rev. D66 (2002) 064004
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
10 pages, 3 figures. Final version (to appear in PRD)
Scientific paper
10.1103/PhysRevD.66.064004
In this paper we consider the collision of black holes with parallel spins using first order perturbation theory of rotating black holes (Teukolsky formalism). The black holes are assumed to be close to each other, initially non boosted and spinning slowly. We estimate the properties of the gravitational radiation released from such an collision. The same problem was studied recently by Gleiser {\em et al.} in the context of the Zerilli perturbation formalism and our results for waveforms, energy and angular momentum radiated agree very well with the results presented in that work.
Khanna Gaurav
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