Quadratic-in-Spin Hamiltonian at $\mathcal{O}(G^2)$ from Scattering Amplitudes
Dimitrios Kosmopoulos, Andres Luna
TL;DR
This work derives the conservative two-body Hamiltonian for spinning compact objects at quadratic order in spin up to ${O}(G^2)$, valid for all velocities, by matching full-theory scattering amplitudes to an EFT with non-minimal gravity couplings. The authors compute tree-level and one-loop amplitudes for a scalar and a spinning particle in the center-of-mass frame, then perform EFT matching to fix long-range spin-dependent potentials and obtain the position-space Hamiltonian, including the Kerr limit ${C_{ES^2}}=1$. They verify consistency with known PN results and test-body limits, reproduce the aligned-spin BH scattering angle, and demonstrate that the Bern:2020buy eikonal-phase relation extends to quadratic-in-spin, strengthening the link between scattering data and classical observables. The results provide a robust framework for incorporating higher-spin and finite-size effects in gravitational binaries and suggest avenues for extending to higher PM orders and tidal corrections.
Abstract
We obtain the quadratic-in-spin terms of the conservative Hamiltonian describing the interactions of a binary of spinning bodies in General Relativity through $\mathcal{O}(G^2)$ and to all orders in velocity. Our calculation extends a recently-introduced framework based on scattering amplitudes and effective field theory to consider non-minimal coupling of the spinning objects to gravity. At the order that we consider, we establish the validity of the formula proposed in \cite{Bern:2020buy} that relates the impulse and spin kick in a scattering event to the eikonal phase.
