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We present a special case of the Stephani solution with spherical symmetrywhile considering different values of spatial curvature. We investigate thedynamics of the universe evolution in our model, build the R--T-regions for theresulting spacetime and analyze the behavior of the deceleration parameter. Thesingularities of the model are also discussed. The geometry of the spatial partof the obtained solution is explored.

Accelerated expansion of the universe from the perspective of inhomogeneous cosmology