  A reformulation of the Schwarzschild solution of the linearised Einstein
field equations in post-Riemannian Finsler spacetime is derived. The solution
is constructed in three stages: the exterior solution, the event-horizon
solution and the interior solution. It is shown that the exterior solution is
asymptotically similar to Newtonian gravity at large distances implying that
Newtonian gravity is a low energy approximation of the solution. Application of
Eddington-Finklestein coordinates is shown to reproduce the results obtained
from standard general relativity at the event horizon. Further application of
Kruskal-Szekeres coordinates reveals that the interior solution contains
maximally extensible geodesics.
