  We construct a FLRW universe considering an anisotropic scaling between space
and time at extremely high and low energies only. In this context, Friedmann
equations contain an additional term arising from spatial curvature which
implements nonsingular bounces in the early Universe. The matter content of the
model is a nonrelativistic pressureless perfect fluid and radiation. By
breaking covariance diffeomorphism also at extreme large scales, an additional
term furnishes late-time acceleration due to spatial curvature so that a
cosmological constant is not needed. In order to probe the final fate of the
universe we also introduce a lower order curvature term which dominates in deep
IR. Given the observational parameters we obtain a concrete model in eternal
recurrence in which the end of late-time acceleration takes place at a redshift
$z \simeq -0.14$ and the universe recollapses at $z\simeq - 0.32$.
