Ultralocality and slow contraction

We study the detailed process by which slow contraction smooths and flattens universe using an improved numerical relativity code that accepts initial conditions with non-perturbative deviations from homogeneity isotropy along two independent spatial directions. Contrary to common descriptions of early universe, we find geometry first rapidly converges inhomogeneous, spatially-curved anisotropic ultralocal state in all gradient contributions equations motion decrease as exponential time negligible values. This is followed a second stage homogeneous, spatially flat isotropic spacetime. In particular, decay appears follow same history whether entire spacetime or only parts it are smoothed end contraction.