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Analytic determination of the eight-and-a-half post-Newtonian self-force contributions to the two-body gravitational interaction potential
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 (as well as the square of Euler’s constant ) starting at the seventh post-Newtonian order. We study the convergence of the post-Newtonian expansion as the expansion parameter leaves the weak-field domain to enter the strong field domain .
Article Text
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