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  Binary black holes coalescence: transition from adiabatic inspiral to plunge

Buonanno, A., & Damour, T. (2002). Binary black holes coalescence: transition from adiabatic inspiral to plunge. In Proceedings of the Ninth Marcel Grossmann Meeting on General Relativity (pp. 1637-1638).

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gr-qc_0011052.pdf (Preprint), 71KB
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Buonanno, Alessandra1, 2, Author           
Damour, Thibault, Author
Affiliations:
1Theoretical Astrophysics and Relativity Group California Institute of Technology, Pasadena, ou_persistent22              
2Astrophysical 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: 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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 Dates: 2000-11-142002
 Publication Status: Issued
 Pages: 2 pages; contributed paper to the IX Marcel Grossmann Meeting in Rome, July 2000
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 Identifiers: arXiv: gr-qc/0011052
DOI: 10.1142/9789812777386_0335
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Title: Ninth Marcel Grossmann Meeting
Place of Event: Roma, Italy
Start-/End Date: 2000-07-02 - 2000-07-08

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Title: Proceedings of the Ninth Marcel Grossmann Meeting on General Relativity
Source Genre: Proceedings
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Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 1637 - 1638 Identifier: -