NNNLO gravitational quadratic-in-spin interactions at the quartic order in G
Michèle Levi, Andrew J. McLeod, Matthew von Hippel
TL;DR
This work computes the complete static $N^3$LO gravitational interactions quadratic in spin at order $G^4$ in the PN expansion for inspiraling binaries using the EFT of gravitating spinning objects. It extends the EFTofPNG framework to include quadratic-in-curvature couplings and spin-induced finite-size effects, and performs a worldline diagrammatic expansion with $163$ graphs, including $52$ three-loop topologies. A key result is the cancellation of divergences, logarithms, and $\\zeta(2)$ terms in the final sum, yielding a finite rational contribution at $5$PN for maximally spinning objects. The findings push the precision frontier of spinning PN gravity and provide a robust computational pipeline for completing the remaining sectors, with future work to incorporate higher-order spin-curvature operators and cross-check with amplitudes-based approaches.
Abstract
We compute the N$^3$LO gravitational quadratic-in-spin interactions at $G^4$ in the post-Newtonian (PN) expansion via the effective field theory (EFT) of gravitating spinning objects for the first time. This result contributes at the $5$PN order for maximally-spinning compact objects, adding the spinning case to the static sector at this PN accuracy. This sector requires extending the EFT of a spinning particle beyond linear order in the curvature to include higher-order operators quadratic in the curvature that are relevant at this PN order. We make use of a diagrammatic expansion in the worldline picture, and rely on our recent upgrade of the \texttt{EFTofPNG} code, which we further extend to handle this sector. Similar to the spin-orbit sector, we find that the contributing three-loop graphs give rise to divergences, logarithms, and transcendental numbers. However, in this sector all of these features conspire to cancel out from the final result, which contains only finite rational terms.
