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We extend the treatment of the problem of the gravitational waves produced bya particle of negligible mass orbiting a Kerr black hole using black holeperturbation theory in the time domain, to elliptic and inclined orbits. Wemodel the particle by smearing the singularities in the source term usingnarrow Gaussian distributions. We compare results (energy and angular momentumfluxes) for such orbits with those computed using the frequency domainformalism.Comment: 6 pages, 3 figures; submitted to PR

Teukolsky evolution of particle orbits around Kerr black holes in the time domain: Elliptic and inclined orbits