Binary Black Holes Coalescence:. Transition from Adiabatic Inspiral to Plunge

Physics

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Scientific paper

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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