Next-to-leading order gravitational spin-orbit coupling in an effective field theory approach
Michele Levi
TL;DR
This work computes the next-to-leading order spin-orbit interaction for a binary of spinning compact objects within an effective field theory framework. By employing nonrelativistic gravitational (NRG) fields and a detailed Feynman-rule set, the authors systematically evaluate one-, two-, and cubic-gravitational contributions, including nonstationary effects and spin supplementary-condition complexities. The resulting NLO spin-orbit Lagrangian is Legendre-transformed to a Hamiltonian and then related to canonical ADM results through noncanonical and canonical transformations, establishing precise equivalence with known Damour-DJS expressions. The analysis demonstrates the practicality and precision of EFT with NR gravity fields for high-order spin effects, setting the stage for future higher-order spin corrections in gravitational-wave physics.
Abstract
We use an effective field theory (EFT) approach to calculate the next to leading order (NLO) gravitational spin-orbit interaction between two spinning compact objects. The NLO spin-orbit interaction provides the most computationally complex sector of the NLO spin effects, previously derived within the EFT approach. In particular, it requires the inclusion of non-stationary cubic self-gravitational interaction, as well as the implementation of a spin supplementary condition (SSC) at higher orders. The EFT calculation is carried out in terms of the non-relativistic gravitational field parametrization, making the calculation more efficient with no need to rely on automated computations, and illustrating the coupling hierarchy of the different gravitational field components to the spin and mass sources. Finally, we show explicitly how to relate the EFT derived spin results to the canonical results obtained with the ADM Hamiltonian formalism. This is done using non-canonical transformations, required due to the implementation of covariant SSC, as well as canonical transformations at the level of the Hamiltonian, with no need to resort to the equations of motion or the Dirac brackets.
