In this paper we give a summary of basic definitions of Finsler geometry as
well as a possible extension of General Relativity, in the vacuum case, fo
r these spaces, followed by a brief account of symmetry imposition for Fins
ler metrics. We then make use of these results in order to generalise, for
up to first order departures from the Riemannian setting, the well-known Bi
rkhoff's theorem from General Relativity, thereby establishing a perturbati
ve, first order version of this theorem for Finsler spaces, where some simp
lifying assumptions have been made. This result has been fully accomplished
by means of computer algebra - actually, the very problem of explicitly de
termining non-Riemannian solutions for some generalised theory of gravity h
as only been made possible by computer algebra. The process is described in
detail within the paper. (C) 1998 Elsevier Science B.V.