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Analytic determination of the eight-and-a-half post-Newtonian self-force contributions to the two-body gravitational interaction potential

Donato Bini1 and Thibault Damour2

  • 1Istituto per le Applicazioni del Calcolo “M. Picone”, CNR, I-00185 Rome, Italy
  • 2Institut des Hautes Etudes Scientifiques, 91440 Bures-sur-Yvette, France

Phys. Rev. D 89, 104047 – Published 23 May, 2014

DOI: https://doi.org/10.1103/PhysRevD.89.104047

Abstract

We analytically compute, to the eight-and-a-half post-Newtonian order, and to linear order in the mass ratio, the radial potential describing (within the effective one-body formalism) the gravitational interaction of two bodies, thereby extending previous analytic results. These results are obtained by applying analytical gravitational self-force theory (for a particle in circular orbit around a Schwarzschild black hole) to Detweiler’s gauge-invariant redshift variable. We emphasize the increase in “transcendentality” of the numbers entering the post-Newtonian expansion coefficients as the order increases, in particular we note the appearance of ζ(3) (as well as the square of Euler’s constant γ) starting at the seventh post-Newtonian order. We study the convergence of the post-Newtonian expansion as the expansion parameter u=GM/(c2r) leaves the weak-field domain u1 to enter the strong field domain u=O(1).

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