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Binary black holes coalescence: transition from adiabatic inspiral to plunge

Alessandra Buonanno·Thibault Damour
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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.

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Alessandra Buonanno, Thibault Damour. 2000-11-14. Binary black holes coalescence: transition from adiabatic inspiral to plunge. https://arxiv.org/abs/gr-qc/0011052

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