Higher-order spin effects in the dynamics of compact binaries. II. Radiation field
By L. Blanchet, A. Buonanno, G. Faye. 2006
165 citations recorded by the source corpus.
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.
View Paper: https://www.semanticscholar.org/paper/4a0c2e4fc6f70f6470b4af295fcae54f71924ac0
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
- T. Damour
- J. Steinhoff
- M. Levi
- P. Jaranowski
- G. Schāfer
- L. S. Collaboration
- Texas Tech University
- Grond
Citations in the corpus
- Multi-messenger observations of a binary neutron star merger (2017, methodology): “This analysis uses post-Newtonian waveform models(Blanchet et al. 1995, 2004, 2006; Bohé et al. 2013) to construct a matchedfilter search(Sathyaprakash & Dhurandhar 1991; Cutler et al. 1993; Allen et al. 2012) for gravitational waves from the coalescence of compact-object binary systems in the…”
- Spinning gravitating objects in the effective field theory in the post-Newtonian scheme (2015, methodology): “To verify equivalence with the ADM Hamiltonian result, which was first obtained in [59], after the corresponding EOM were obtained in [56, 68], we resolve the difference between the result in [59], and the result here, using canonical transformations, see e.”
- Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling (2008, methodology): “[15] has considered, instead of the Taylor-Hamiltonian LSO, the minimum of the Taylor-expanded function e(Ω̂) (or “ICO”).”