Document Type

Article

Publication Date

1-1-2000

Abstract

We consider perturbations of a Schwarzschild black hole that can be of both even and odd parity, keeping terms up to second order in perturbation theory, for the 1 = 2 axisymmetric case. We develop explicit formulae for the evolution equations and radiated energies and waveforms using the Regge-Wheeler-Zerilli approach. This formulation is useful, for instance, for the treatment in the "close limit approximation" of the collision of counterrotating black holes. © 2000 Plenum Publishing Corporation.

Publication Source (Journal or Book title)

General Relativity and Gravitation

First Page

2021

Last Page

2042

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