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Spin(1)spin(2) effects in the motion of inspiralling compact binaries at third order in the post-Newtonian expansion
Phys. Rev. D 78, 044012 – Published 7 August, 2008Errata Phys. Rev. D 81, 029904 (2010); Phys. Rev. D 81, 029905 (2010)
DOI: https://doi.org/10.1103/PhysRevD.78.044012
Abstract
We use effective field theory techniques to compute the potentials due to spin-spin and spin-orbit effects, from which the contribution to the motion of spinning compact binaries to third Post-Newtonian (PN) order follow. We use a formalism which allows us to impose the spin supplementary condition (SSC) in a canonical framework to all orders in the PN expansion. We explicitly show the equivalence with our previous results, obtained using the Newton-Wigner SSC at the level of the action for spin-spin and spin-orbit potentials reported in arXiv:gr-qc/0604099 and arXiv:0712.2032 , respectively.
Errata
Erratum: Spin(1)spin(2) effects in the motion of inspiralling compact binaries at third order in the post-Newtonian expansion [Phys. Rev. D 78, 044012 (2008)]
Erratum: Next to leading order spin(1)spin(1) effects in the motion of inspiralling compact binaries [Phys. Rev. D 78, 044013 (2008)]
Comments & Replies
Comment on two recent papers regarding next-to-leading order spin-spin effects in gravitational interaction
See Also
Next to leading order spin(1)spin(1) effects in the motion of inspiralling compact binaries
Article Text
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