Abstract
Motivated by seeking kinetic origins for seedsof the large-scale structure formation in the universe,we investigate the properties of a generalizedaxisymmetric Bianchi IX type model. Such a model, which is supposed to describe non-interactingradiation of dust-like matter posterior to decoupling,has the advantage ofbehaving asymptotically as a closefrw model with a cosmological constant. It shows avanishing vorticity, a decreasing shear of matter withtime and a frw chronology, which are properties thatmake it likely when compared to observationalconstraints. The formula which provides us with theredshifts of sources is derived.
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Triay, R., Villalba, V.M. A Mille-feuille Universe. General Relativity and Gravitation 31, 1913–1920 (1999). https://doi.org/10.1023/A:1026790923015
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DOI: https://doi.org/10.1023/A:1026790923015