Asymptotics of Schwarzschild black hole perturbations

Abstract

We study linear gravitational perturbations of Schwarzschild spacetime by solving numerically Regge-Wheeler-Zerilli equations in time domain using hyperboloidal surfaces and a compactifying radial coordinate. We stress the importance of including the asymptotic region in the computational domain in studies of gravitational radiation. The hyperboloidal approach should be helpful in a wide range of applications employing black hole perturbation theory.

9 pages, 8 figures; changed title, updated references, matches the published version

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Cited by in corpus (38)

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