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  Gravitational waves from inspiraling binary black holes

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.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0019-DC38-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0019-DC39-3
Genre: Journal Article

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 Creators:
Buonanno, Alessandra1, 2, 3, Author              
Affiliations:
1Institut d'Astrophysique de Paris , ou_persistent22              
2Theoretical Astrophysics and Relativity Group, California Institute of Technology, Pasadena, ou_persistent22              
3Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 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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 Dates: 2002-03-092002-03-252002
 Publication Status: Published in print
 Pages: References added and updated; few typos corrected
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 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: gr-qc/0203030
DOI: 10.1088/0264-9381/19/7/305
URI: http://arxiv.org/abs/gr-qc/0203030
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Title: Classical and Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 19 (7) Sequence Number: - Start / End Page: 1267 - 1278 Identifier: -