The ideas presented by Szydlowski and Lapeta [Phys. Lett. A 148 (1990)
239] are developed in the context of general relativity. We show the
ineffectiveness of the classical criteria of the chaotic behaviour (Ly
apunov exponents) in general relativity and in its cosmological applic
ations. This is a simple consequence of general covariance of this the
ory. We investigate chaotic behaviour by reducing respective dynamical
systems to geodesic flows on a Riemannian space. In our approach ''Ly
apunov like exponents'' are invariant forms independently of any time-
coordinate transformations. The criterion of the local instability of
a geodesic flow and ''Lyapunov exponents'' are formulated in terms of
the Ricci scalar R and other invariants of the Riemannian curvature te
nsor. Possible cosmological applications of the proposed formalism are
also discussed.