2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/33696Using 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.2 pages; contributed paper to the IX Marcel Grossmann Meeting in Rome, July 2000General Relativity and Quantum CosmologyBinary black holes coalescence: transition from adiabatic inspiral to plungetext