Teukolsky evolution of particle orbits around Kerr black holes in the time domain: elliptic and inclined orbits

Details Teukolsky evolution of particle orbits around Kerr black holes in the time domain: elliptic and inclined orbits Teukolsky evolution of particle orbits around Kerr black holes in the time domain: elliptic and inclined orbits

2003-09-22

arxiv.org/abs/gr-qc/0309107v1

Phys.Rev. D69 (2004) 024016

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, 3 figures; submitted to PRD

Scientific paper

10.1103/PhysRevD.69.024016

We extend the treatment of the problem of the gravitational waves produced by a particle of negligible mass orbiting a Kerr black hole using black hole perturbation theory in the time domain, to elliptic and inclined orbits. We model the particle by smearing the singularities in the source term using narrow Gaussian distributions. We compare results (energy and angular momentum fluxes) for such orbits with those computed using the frequency domain formalism.

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