  In this paper the dynamic compactification in Lovelock gravity with a cubic
term is studied. The ansatz will be of space-time where the three dimensional
space and the extra dimensions are constant curvature manifolds with
independent scale factors. The numerical analysis shows that there exist a
phenomenologically realistic compactification regime where the three
dimensional hubble parameter and the extra dimensional scale factor tend to a
constant. This result comes as surprise as in Einstein-Gauss-Bonnet gravity
this regime exists only when the couplings of the theory are such that the
theory does not admit a maximally symmetric solution (i.e. "geometric
frustration"). In cubic Lovelock gravity however there always exists at least
one maximally symmetric solution which makes it fundamentally different from
the Einstein-Gauss-Bonnet case. Moreover, in opposition to
Einstein-Gauss-Bonnet Gravity, it is also found that for some values of the
couplings and initial conditions these compactification regimes can coexist
with isotropizing solutions.
