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Transition from inspiral to plunge in binary black hole coalescences
Open accessAbstract
Combining recent techniques giving nonperturbative resummed estimates of the damping and conservative parts of the two-body dynamics, we describe the transition between the adiabatic phase and the plunge, in coalescing binary black holes with comparable masses moving on quasicircular orbits. We give initial dynamical data for numerical relativity investigations, with a fraction of an orbit left, and provide, for data analysis purposes, an estimate of the gravitational waveform emitted throughout the inspiral, plunge and coalescence phases.
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Cited by
Quasinormal modes of black holes and black branes
Berti, E., Cardoso, V., & Starinets, A. O. (2009) · Classical and Quantum Gravity · doi:10.1088/0264-9381/26/16/163001 · Cited by 2,095
Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
Blanchet, L. (2006) · Living Reviews in Relativity · doi:10.12942/lrr-2006-4 · Cited by 686
Shankar, F., Bernardi, M., Sheth, R. K., Ferrarese, L., Graham, A. W., Savorgnan, G., Allevato, V., Marconi, A., Läsker, R., & Lapi, A. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw678 · Cited by 263
Ould El Hadj, M. (2025) · Physical Review D · doi:10.1103/physrevd.111.044055 · Cited by 9
Metadata
- Authors
- Buonanno, A., & Damour, T.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2000-08-10
- Volume
- 62
- Issue
- 6
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2116108818
- Cited by
- 847
- References
- 0
- FWCI
- 8.64
- Type
- journal article
- Language
- en
- Open access
- green
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