Exact Results for the Kepler Problem in General Relativity
Abstract
Exact results are derived, specifically the perihelion shift and the Kepler orbit, for a bound test particle in the Schwarzschild metric with cosmological constant =0. A series expansion, of φ = 2(2(1-2M/p(3-e))-1/2 K((4eM/p)/(1-2M/p(3-e)))-π), the exact perihelion shift, admits the standard approximation φ=6Mπ/p as the leading order term. In a similar fashion, a series expansion of the exact Kepler orbit, represented by a Jacobi elliptic function, gives u(φ)=(1+eφ)/p to first order. The results are valid for M/p<1/(2(3+e)) or rs<p/(3+e).
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