  We modify Einstein General Relativity by adding non-dynamical scalar fields
to account simultaneously for both dark matter and dark energy. The dark energy
in this case can be distributed in-homogeneously even within horizon scales.
Its inhomogeneities can contribute to the late time integrated Sachs-Wolfe
effect, possibly removing some of the low multipole anomalies in the
temperature fluctuations of the CMB spectrum. The presence of the inhomogeneous
dark matter also influences structure formation in the universe.
