Waveform propagation in black hole spacetimes: evaluating the quality of numerical solutions

Details Waveform propagation in black hole spacetimes: evaluating the quality of numerical solutions Waveform propagation in black hole spacetimes: evaluating the quality of numerical solutions

1997-12-08

arxiv.org/abs/gr-qc/9712037v1

Phys.Rev. D57 (1998) 1084-1091

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, RevTeX, to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.57.1084

We compute the propagation and scattering of linear gravitational waves off a Schwarzschild black hole using a numerical code which solves a generalization of the Zerilli equation to a three dimensional cartesian coordinate system. Since the solution to this problem is well understood it represents a very good testbed for evaluating our ability to perform three dimensional computations of gravitational waves in spacetimes in which a black hole event horizon is present.

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