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  Third post-Newtonian spin-orbit effect in the gravitational radiation flux of compact binaries

Blanchet, L., Buonanno, A., & Faye, G. (2012). Third post-Newtonian spin-orbit effect in the gravitational radiation flux of compact binaries. In Astronomical Society of the Pacific (Ed.), ASP Conference Series, Vol. 467 (pp. 215-220).

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1210.0764.pdf (Preprint), 60KB
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 Creators:
Blanchet, Luc, Author
Buonanno, A.1, 2, Author           
Faye, Guillaume, Author
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              
2Maryland Center for Fundamental Physics & Joint Space-Science Institute, ou_persistent22              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: Gravitational waves contain tail effects that are due to the backscattering of linear waves in the curved space-time geometry around the source. The knowledge as well as the accuracy of the two-body inspiraling post-Newtonian (PN) dynamics and of the gravitational-wave signal has been recently improved, notably by computing the spin-orbit (SO) terms induced by tail effects in the gravitational-wave energy flux at the 3PN order. Here we sketch this derivation, which yields the phasing formula including SO tail effects through the same 3PN order. Those results can be employed to improve the accuracy of analytical templates aimed at describing the whole process of inspiral, merger, and ringdown.

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 Dates: 2012-10-022012
 Publication Status: Issued
 Pages: 6 pages; proceeding of the 9th LISA Symposium, Paris
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 Identifiers: arXiv: 1210.0764
URI: http://arxiv.org/abs/1210.0764
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Title: 9th LISA Symposium, Paris
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Title: ASP Conference Series, Vol. 467
Source Genre: Proceedings
 Creator(s):
Astronomical Society of the Pacific, Editor              
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Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 215 - 220 Identifier: -