The tail effect in gravitational radiation-reaction: time non-locality and renormalization group evolution
Chad R. Galley, Adam K. Leibovich, Rafael A. Porto, Andreas Ross

TL;DR
This paper employs effective field theory to analyze the tail effect in gravitational radiation reaction at 4PN order, revealing non-local time behavior, UV/IR singularities, and applying renormalization group techniques for resummation.
Contribution
It introduces a novel EFT-based calculation of the tail effect, demonstrating the cancellation of IR and UV divergences and deriving RG evolution for binary system parameters.
Findings
Tail contribution is non-local in time with dissipative and conservative parts.
UV divergence cancels with IR singularity from near zone, due to point-particle limit.
RG techniques successfully resum logarithmic corrections in gravitational dynamics.
Abstract
We use the effective field theory (EFT) framework to calculate the tail effect in gravitational radiation reaction, which enters at 4PN order in the dynamics of a binary system. The computation entails a subtle interplay between the near (or potential) and far (or radiation) zones. In particular, we find that the tail contribution to the effective action is non-local in time, and features both a dissipative and a `conservative' term. The latter includes a logarithmic ultraviolet (UV) divergence, which we show cancels against an infrared (IR) singularity found in the (conservative) near zone. The origin of this behavior in the long-distance EFT is due to the point-particle limit -shrinking the binary to a point- which transforms a would-be infrared singularity into an ultraviolet divergence. This is a common occurrence in an EFT approach, which furthermore allows us to use…
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