A time-domain fourth-order-convergent numerical algorithm to integrate black hole perturbations in the extreme-mass-ratio limit
- 13 July 2005
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 22 (15) , S543-S568
- https://doi.org/10.1088/0264-9381/22/15/001
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- Coalescence remnant of spinning binary black holesPhysical Review D, 2004
- Computing the gravitational self-force on a compact object plunging into a Schwarzschild black holePhysical Review D, 2002
- Modeling gravitational radiation from coalescing binary black holesPhysical Review D, 2002
- Corotating and irrotational binary black holes in quasicircular orbitsPhysical Review D, 2002
- The Lazarus project: A pragmatic approach to binary black hole evolutionsPhysical Review D, 2002
- Plunge Waveforms from Inspiralling Binary Black HolesPhysical Review Letters, 2001
- Nonlinear and perturbative evolution of distorted black holes: Odd-parity modesPhysical Review D, 2000
- Gravitational waves from black hole collisions via an eclectic approachClassical and Quantum Gravity, 2000
- Second order gauge invariant gravitational perturbations of a Kerr black holePhysical Review D, 1999
- Imposition of Cauchy data to the Teukolsky equation. I. The nonrotating casePhysical Review D, 1998