Abstract
An axisymmetric rotating universe model is crossed with a time-dependent factor. Its evolution is studied. It turns out that for a particular choice it behaves exactly like that of a flat Friedmann universe.
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Bokhari, A.H., Pervez, A. & Mughal, M.A. Nonstatic axisymmetric universe model and its evolution. Int J Theor Phys 29, 1011–1014 (1990). https://doi.org/10.1007/BF00673687
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DOI: https://doi.org/10.1007/BF00673687