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• W3100476074 startingPage "3259" @default.
• W3100476074 abstract "Treating the Teukolsky perturbation equation numerically as a 2+1 PDE and smearing the singularities in the particle source term by the use of narrow Gaussian distributions, we have been able to reproduce earlier results for equatorial circular orbits that were computed using the frequency domain formalism. A time domain prescription for a more general evolution of nearly geodesic orbits under the effects of radiation reaction is presented. This approach can be useful when tackling the more realistic problem of a stellar-mass black hole moving on a generic orbit around a supermassive black hole under the influence of radiation reaction forces." @default.
• W3100476074 created "2020-11-23" @default.
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• W3100476074 date "2003-07-01" @default.
• W3100476074 modified "2023-10-15" @default.
• W3100476074 title "Perturbative evolution of particle orbits around Kerr black holes: time-domain calculation" @default.
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• W3100476074 doi "https://doi.org/10.1088/0264-9381/20/14/320" @default.
• W3100476074 hasPublicationYear "2003" @default.
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