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Journal Article

Gravitational waves from inspiraling binary black holes

MPS-Authors
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Buonanno,  Alessandra
Institut d'Astrophysique de Paris ;
Theoretical Astrophysics and Relativity Group, California Institute of Technology, Pasadena;
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Fulltext (public)

gr-qc_0203030.pdf
(Preprint), 219KB

CQG_19_7_305.pdf
(Any fulltext), 174KB

Supplementary Material (public)
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Citation

Buonanno, A. (2002). Gravitational waves from inspiraling binary black holes. Classical and Quantum Gravity, 19(7), 1267-1278. doi:10.1088/0264-9381/19/7/305.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0019-DC38-5
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.