Single field inflationary models with non-compact Kaluza-Klein theory

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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version accepted in Phys. Lett. B

Scientific paper

10.1016/j.physletb.2003.11.055

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.

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