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Teukolsky evolution of particle orbits around Kerr black holes in the time domain: elliptic and inclined orbits
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Teukolsky evolution of particle orbits around Kerr black holes in the time domain: elliptic and inclined orbits
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We extend the treatment of the problem of the gravitational waves produced by a particle of negligible mass orbiting a Kerr black hole using black hole perturbation theory in the time domain, to elliptic and inclined orbits. We model the particle by smearing the singularities in the source term using narrow Gaussian distributions. We compare results (energy and angular momentum fluxes) for such orbits with those computed using the frequency domain formalism.
Forward citations
Cited by 2 Pith papers
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Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries
Adiabatic point-particle black hole perturbation theory reproduces numerical-relativity spin effects in comparable-mass inspirals to within ~1%, so only small spin-dependent post-adiabatic corrections are needed.
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