Application of energy and angular momentum balance to gravitational radiation reaction for binary systems with spin-orbit coupling

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dc.creatorZeng, Jing
dc.creatorWill, Clifford M.
dc.date2007-04-20
dc.date.accessioned2026-07-07T10:59:41Z
dc.date.available2026-07-07T10:59:41Z
dc.descriptionWe study gravitational radiation reaction in the equations of motion for binary systems with spin-orbit coupling, at order (v/c)^7 beyond Newtonian gravity, or O(v/c)^2 beyond the leading radiation reaction effects for non-spinning bodies. We use expressions for the energy and angular momentum flux at infinity that include spin-orbit corrections, together with an assumption of energy and angular momentum balance, to derive equations of motion that are valid for general orbits and for a class of coordinate gauges. We show that the equations of motion are compatible with those derived earlier by a direct calculation.
dc.description12 pages, submitted to General Relativity and Gravitation
dc.identifierhttps://arxiv.org/abs/0704.2720
dc.identifierhttp://arxiv.org/abs/0704.2720
dc.identifierGen.Rel.Grav.39:1661-1673,2007
dc.identifierdoi:10.1007/s10714-007-0475-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187488
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleApplication of energy and angular momentum balance to gravitational radiation reaction for binary systems with spin-orbit coupling
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