Hereditary Terms at Next-To-Leading Order in Two-Body Gravitational Dynamics
Stefano Foffa, Riccardo Sturani
TL;DR
This work advances high-precision modeling of two-body gravitational dynamics by computing next-to-leading order hereditary terms at $5$PN within an EFT framework, including both tail and memory effects. It provides new conservative contributions from octupole and magnetic quadrupole tails, a logarithmic energy term for circular orbits, and local-in-time corrections from angular-momentum memory and GW self-interaction, all while confirming universal relations between tail flux and non-tail emissions. The analysis clarifies how far-zone dynamics feed into near-zone conservative physics, and it outlines the remaining steps to achieve a complete $5$PN description, with significant implications for accurate gravitational-wave templates and tests of GR in the strong-field regime.
Abstract
In the context of the two-body problem in General Relativity, hereditary terms in the long range gravitational field depend on the history rather than the instantaneous state of the source at retarded time. We compute the next-to leading effects of such hereditary terms, that comprise tail and memory, on the two-body dynamics, within effective field theory methods, including both dissipative and conservative effects. The former confirm known results at 2.5 post-Newtonian order with respect to the leading order in the luminosity function; the conservative part is a new result and is an unavoidable ingredient for a derivation of the conservative two-body dynamics at fifth post-Newtonian order.
