A Mille-feuille universe

Motivated by seeking kinetic origins for seeds of the large-scale structure formation in the universe, we investigate the properties of a generalized axisymmetric Bianchi IX type model. Such a model, which is supposed to desc ribe nun-interacting radiation of dust like matter posterior to decoupling, has the advantage of behaving asymptotically as a close FRW model with a c osmological constant. It shows a vanishing vorticity, a decreasing shear of matter with time and a FRW chronology, which are properties that make it l ikely when compared to observational constraints. The formula which provide s us with the redshifts of sources is derived.