  We study homogeneous and isotropic cosmologies in a Weyl spacetime. We show
that the field equations can be reduced to the Einstein equations with a
two-fluid source and analyze the qualitative, asymptotic behavior of the
models. Assuming an interaction of the two fluids we impose conditions so that
the solutions of the corresponding dynamical system remain in the physically
acceptable phase space. We show that in Weyl integrable spacetime, the
corresponding scalar field acts as a phantom field and therefore, it may give
rise to a late accelerated expansion of the Universe.
