An Open Inflationary Model for Dimensional Reduction and its Effects on the Observable Parameters of the Universe

Details An Open Inflationary Model for Dimensional Reduction and its Effects on the Observable Parameters of the Universe An Open Inflationary Model for Dimensional Reduction and its Effects on the Observable Parameters of the Universe

2005-01-11

arxiv.org/abs/astro-ph/0501200v1

Int.J.Mod.Phys. A20 (2005) 2449-2453

Astronomy and Astrophysics

Astrophysics

5 pages, accepted for publication in Int. J. of Mod. Phys. A

Scientific paper

10.1142/S0217751X05024754

Assuming that higher dimensions existed in the early stages of the universe where the evolution was inflationary, we construct an open, singularity-free, spatially homogeneous and isotropic cosmological model to study the effects of dimensional reduction that may have taken place during the early stages of the universe. We consider dimensional reduction to take place in a stepwise manner and interpret each step as a phase transition. By imposing suitable boundary conditions we trace their effects on the present day parameters of the universe.

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