Post-Newtonian corrections to the motion of spinning bodies in NRGR
Rafael A. Porto
TL;DR
This work extends NRGR, an effective field theory approach to gravity in the post-Newtonian regime, to include spin and permanent multipole moments of extended bodies. By formulating a spinful worldline action and deriving spin-graviton interactions, the authors obtain leading spin-orbit and spin-spin potentials, a quadrupole-spin coupling, and the corresponding quadrupole radiation formula, while also clarifying the equivalence of different spin supplementary conditions. They analyze divergences and classify finite-size effects as tidal (logarithmic, RG-flow) or self-induced (power-law, scale-independent), deriving their scaling and showing how they renormalize within NRGR. The results provide a systematic framework for incorporating spin and internal structure into PN gravitational-wave templates, with explicit predictions for higher-order effects and clear guidance for future extensions.
Abstract
In this paper we include spin and multipole moment effects in the formalism used to describe the motion of extended objects recently introduced in hep-th/0409156. A suitable description for spinning bodies is developed and spin-orbit, spin-spin and quadrupole-spin Hamiltonians are found at leading order. The existence of tidal, as well as self induced finite size effects is shown, and the contribution to the Hamiltonian is calculated in the latter. It is shown that tidal deformations start formally at O(v^6) and O(v^10) for maximally rotating general and compact objects respectively, whereas self induced effects can show up at leading order. Agreement is found for the cases where the results are known.
