2005
DOI: 10.1088/0264-9381/22/15/001
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A time-domain fourth-order-convergent numerical algorithm to integrate black hole perturbations in the extreme-mass-ratio limit

Abstract: Abstract. We obtain a fourth order accurate numerical algorithm to integrate the Zerilli and Regge-Wheeler wave equations, describing perturbations of nonrotating black holes, with source terms due to an orbiting particle. Those source terms contain the Dirac's delta and its first derivative. We also re-derive the source of the Zerilli and Regge-Wheeler equations for more convenient definitions of the waveforms, that allow direct metric reconstruction (in the Regge-Wheeler gauge).

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Cited by 38 publications
(59 citation statements)
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“…2. Briefly, for second order global accuracy I use a standard diamond-cell integration scheme [16,33,34,37,55,56,84], while for fourth order global accuracy I use a modified version of the scheme described by Lousto [55] and Haas [38]. I describe the finite differencing schemes in detail in Appendix A.…”
Section: Unigrid Finite Differencingmentioning
confidence: 99%
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“…2. Briefly, for second order global accuracy I use a standard diamond-cell integration scheme [16,33,34,37,55,56,84], while for fourth order global accuracy I use a modified version of the scheme described by Lousto [55] and Haas [38]. I describe the finite differencing schemes in detail in Appendix A.…”
Section: Unigrid Finite Differencingmentioning
confidence: 99%
“…To discretize the wave equation (3) to fourth order global accuracy in the grid spacing , I use a scheme based on that of Haas [38] (see also [55]), but modified in its treatment of cells near the particle. The modification makes the scheme fully explicit, removing the need for an iterative computation at each cell intersecting the particle.…”
Section: A2 Fourth Order Global Accuracymentioning
confidence: 99%
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