Binary black holes coalescence: transition from adiabatic inspiral to plunge

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dc.creatorBuonanno, Alessandra
dc.creatorDamour, Thibault
dc.date2000-11-14
dc.date.accessioned2026-07-07T03:25:24Z
dc.date.available2026-07-07T03:25:24Z
dc.descriptionUsing 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.
dc.description2 pages; contributed paper to the IX Marcel Grossmann Meeting in Rome, July 2000
dc.identifierhttps://arxiv.org/abs/gr-qc/0011052
dc.identifierhttp://arxiv.org/abs/gr-qc/0011052
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33696
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBinary black holes coalescence: transition from adiabatic inspiral to plunge
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