The effective early universe in the presence of extra dimensions

Physics

Scientific paper

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Scientific paper

The Robertson-Walker geometry in an empty five-dimensional universe is derived, and the effective four-dimensional evolution is analyzed. The radius of the compact fifth dimension is regarded as a non-static quantity. The ``fine structure'' constancy is asymptotically respected only provided the cosmological constant vanishes and the ordinary three-space is open. Characteristically, the evolution of the very early universe is governed by the Zeldovich equation of state P=ϱ.

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