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  Higher-order spin effects in the dynamics of compact binaries II. Radiation field

Blanchet, L., Buonanno, A., & Faye, G. (2006). Higher-order spin effects in the dynamics of compact binaries II. Radiation field. Physical Review D, 74: 104034. doi:10.1103/PhysRevD.74.104034.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0018-D7D1-A Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0018-D7DE-0
Genre: Journal Article

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 Creators:
Blanchet, Luc, Author
Buonanno, Alessandra1, 2, 3, 4, Author              
Faye, Guillaume, Author
Affiliations:
1Department of Physics, University of Maryland, escidoc:persistent22              
2AstroParticule et Cosmologie (APC), UMR 7164-CNR, escidoc:persistent22              
3GReCO, Institut d’Astrophysique de Paris, escidoc:persistent22              
4Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:1933290              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: Motivated by the search for gravitational waves emitted by binary black holes, we investigate the gravitational radiation field of point particles with spins within the framework of the multipolar-post-Newtonian wave generation formalism. We compute: (i) the spin-orbit (SO) coupling effects in the binary's mass and current quadrupole moments one post-Newtonian (1PN) order beyond the dominant effect, (ii) the SO contributions in the gravitational-wave energy flux and (iii) the secular evolution of the binary's orbital phase up to 2.5PN order. Crucial ingredients for obtaining the 2.5PN contribution in the orbital phase are the binary's energy and the spin precession equations, derived in paper I of this series. These results provide more accurate gravitational-wave templates to be used in the data analysis of rapidly rotating Kerr-type black-hole binaries with the ground-based detectors LIGO, Virgo, GEO 600 and TAMA300, and the space-based detector LISA. Erratum-ibid.D75:049903,2007; Erratum-ibid.D81:089901,2010

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 Dates: 2006-05-272010-03-052006
 Publication Status: Published in print
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 Identifiers: arXiv: gr-qc/0605140
DOI: 10.1103/PhysRevD.74.104034
URI: http://arxiv.org/abs/gr-qc/0605140
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Title: Physical Review D
  Other : Phys. Rev. D.
Source Genre: Journal
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Publ. Info: Lancaster, Pa. : American Physical Society
Pages: - Volume / Issue: 74 Sequence Number: 104034 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111088197762258