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Conference Paper

Binary black holes coalescence: transition from adiabatic inspiral to plunge

MPS-Authors
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Buonanno,  Alessandra
Theoretical Astrophysics and Relativity Group California Institute of Technology, Pasadena;
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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gr-qc_0011052.pdf
(Preprint), 71KB

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Citation

Buonanno, A., & Damour, T. (2002). Binary black holes coalescence: transition from adiabatic inspiral to plunge. In Proceedings of the Ninth Marcel Grossmann Meeting on General Relativity (pp. 1637-1638).


Cite as: https://hdl.handle.net/11858/00-001M-0000-0019-E2F3-3
Abstract
Using two recent techniques giving non-perturbative re-summed estimates of the damping and of the conservative part of the dynamics of two-body systems, we describe the transition between adiabatic inspiral and plunge in binary non-spinning black holes moving along quasi-circular orbits.