Effective field theory approach to the gravitational two-body dynamics, at fourth post-Newtonian order and quintic in the Newton constant
Stefano Foffa, Pierpaolo Mastrolia, Riccardo Sturani, Christian Sturm
TL;DR
This work computes the missing $G_N^5$ contributions to the conservative two-body dynamics at $4$PN within an effective field theory (EFT) framework. By mapping each gravity amplitude at order $G_N^\\ell$ to a $(\ell-1)$-loop massless 2-point integral and applying integration-by-parts (IBP) with a basis of master integrals in dimensional regularization, the authors evaluate the 50 genuine $O(G_N^5)$ diagrams. The resulting complete 4PN Lagrangian is finite and matches existing results upon accounting for regularization and lower-order contributions, with explicit terms such as $\mathcal{L}_{49}=(32-3\pi^2)\frac{G_N^5 m_1^3 m_2^3}{r^5}$ and the total $\sum_a \mathcal{L}_a$ given by a specific combination of mass factors and powers of $r$. This EFT-based calculation provides a robust cross-check for the 4PN dynamics and demonstrates the feasibility of high-loop, classical-gravity calculations within the EFT paradigm.
Abstract
Working within the post-Newtonian (PN) approximation to General Relativity, we use the effective field theory (EFT) framework to study the conservative dynamics of the two-body motion at fourth PN order, at fifth order in the Newton constant. This is one of the missing pieces preventing the computation of the full Lagrangian at fourth PN order using EFT methods. We exploit the analogy between diagrams in the EFT gravitational theory and 2-point functions in massless gauge theory, to address the calculation of 4-loop amplitudes by means of standard multi-loop diagrammatic techniques. For those terms which can be directly compared, our result confirms the findings of previous studies, performed using different methods.
