Constants of motion and fundamental frequencies for elliptic orbits at fourth post-Newtonian order
David Trestini

TL;DR
This paper derives a precise map between constants of motion and fundamental frequencies for nonspinning compact binaries on quasi-elliptic orbits at fourth post-Newtonian order, including tail effects and eccentricity resummation.
Contribution
It provides the first comprehensive fourth post-Newtonian order map incorporating tail effects and eccentricity, with explicit phase-space transformations and validation against self-force results.
Findings
Derived the conservative map at 4PN order including tail contributions.
Expressed the map using an eccentricity enhancement function with resummation.
Validated the redshift invariant against analytical self-force calculations.
Abstract
In the case of nonspinning compact binary systems on quasi-elliptic orbits, I obtain the conservative map between the constants of motion (energy and angular momentum) and the fundamental (radial and azimuthal) frequencies at the fourth post-Newtonian order, including both instantaneous and tail contributions. This map is expressed in terms of an enhancement function of the eccentricity, which is appropriately resummed to ensure accuracy for any eccentricity; in particular, I recover known results for circular orbits. In order to obtain this map, the local dynamics are expressed using an action-angle formulation. The tail term is treated as a perturbation, which is first localized in time, then Delaunay-averaged. Both operations require a contact transformation of the phase-space variables, which I explicitly control. Using the first law of binary black hole mechanics, I then obtain the…
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