Single field inflationary models with non-compact Kaluza-Klein theory
arXiv:gr-qc/0310130 · doi:10.1016/j.physletb.2003.11.055
Abstract
We discuss a semiclassical treatment to inflationary models from Kaluza-Klein theory without the cylinder condition. We conclude that the evolution of the early universe could be described by a geodesic trayectory of a cosmological 5D metric here proposed, so that the effective 4D FRW background metric should be a hypersurface on a constant fifth dimension.
version accepted in Phys. Lett. B
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