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Radiation Reaction for Non-Spinning Bodies at 4.5PN in the Effective Field Theory Approach
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We calculate the 2 post-Newtonian correction to the radiation reaction acceleration for non-spinning binary systems, which amounts to the 4.5 post-Newtonian correction to Newtonian acceleration. The calculation is carried out completely using the effective field theory approach. The center-of-mass corrections to the results are complicated and are discussed in detail. Non-trivial consistency checks are performed and we compare with corresponding results in the literature. Analytic results are supplied in the supplementary materials.
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Cited by 2 Pith papers
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Gravitational radiation reaction for compact binary systems at the fourth-and-a-half post-Newtonian order in harmonic coordinates
The 4.5PN radiation-reaction acceleration of nonspinning compact binaries is derived in harmonic coordinates, including a dimensional-regularization pole, and is shown to satisfy flux-balance laws and Lorentz invariance.
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Radiation-reaction driven dynamics at the third-and-a-half post-Newtonian order in different gauges
A method is given for obtaining the 3.5PN radiation-reaction force and orbit correction in any Hamiltonian coordinate system by transforming from harmonic coordinates.
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