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Gravitational waves from inspiraling binary black holes

Alessandra Buonanno

gr-qcarXiv:gr-qc/0203030

Abstract

Binary black holes are the most promising candidate sources for the first generation of earth-based interferometric gravitational-wave detectors. We summarize and discuss the state-of-the-art analytic techniques developed during the last years to better describe the late dynamical evolution of binary black holes of comparable masses.

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