  In the macroscopic gravity approach to the averaging problem in cosmology,
the Einstein field equations on cosmological scales are modified by appropriate
gravitational correlation terms. We present exact cosmological solutions to the
equations of macroscopic gravity for a spatially homogeneous and isotropic
macroscopic space-time and find that the correlation tensor is of the form of a
spatial curvature term. We briefly discuss the physical consequences of these
results.
