The gravitational Compton amplitude at third post-Minkowskian order
N. Emil J. Bjerrum-Bohr, Gang Chen, Carl Jordan Eriksen, Nabha Shah
TL;DR
This work computes the classical gravitational Compton amplitude for a graviton scattering off a non-spinning massive body up to $3$PM using curved-space worldline effective field theory. The method expands around a Schwarzschild–Tangherlini background, builds the $3$PM integrand from recoil and metric-insertion diagrams, and solves master integrals via a canonical differential-equation framework to obtain the IR-exponentiated and finite parts. The authors verify infrared factorization, check against known results, and compare with black hole perturbation theory, finding exact agreement with BHPT at $2$PM and only partial agreement at $3$PM due to subtleties in mapping between frameworks. The results demonstrate the computational power of curved-space worldline EFT for classical gravity amplitudes and illuminate how amplitude methods connect to BH perturbation theory, with implications for scattering-based analyses of massive binaries. Future work will aim to resolve the $3$PM BHPT mismatch and to extend the formalism to higher orders.
Abstract
We compute the classical Compton amplitude for graviton interaction with a non-spinning massive body up to the third post-Minkowskian order. Our novel result utilizes the enhanced computational efficiency provided by worldline effective field theory in a non-trivial background spacetime. Physical constraints, such as infrared factorization, provide a useful cross-check of the result and we also consider its consistency with computations in black hole perturbation theory.
