Higher-order spin effects in the dynamics of compact binaries I. Equations of motion

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dc.creatorFaye, Guillaume
dc.creatorBlanchet, Luc
dc.creatorBuonanno, Alessandra
dc.date2006-05-27
dc.date2007-01-18
dc.date.accessioned2026-07-07T07:41:27Z
dc.date.available2026-07-07T07:41:27Z
dc.descriptionWe derive the equations of motion of spinning compact binaries including the spin-orbit (SO) coupling terms one post-Newtonian (PN) order beyond the leading-order effect. For black holes maximally spinning this corresponds to 2.5PN order. Our result for the equations of motion essentially confirms the previous result by Tagoshi, Ohashi and Owen. We also compute the spin-orbit effects up to 2.5PN order in the conserved (Noetherian) integrals of motion, namely the energy, the total angular momentum, the linear momentum and the center-of-mass integral. We obtain the spin precession equations at 1PN order beyond the leading term, as well. Those results will be used in a future paper to derive the time evolution of the binary orbital phase, providing more accurate templates for LIGO-Virgo-LISA type interferometric detectors.
dc.descriptiontranscription error in Eqs. (2.17) corrected
dc.identifierhttps://arxiv.org/abs/gr-qc/0605139
dc.identifierhttp://arxiv.org/abs/gr-qc/0605139
dc.identifierPhysical Review D 74 (29/11/2006) 104033
dc.identifierdoi:10.1103/PhysRevD.74.104033
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/122116
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHigher-order spin effects in the dynamics of compact binaries I. Equations of motion
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