Creating the Universe Without a Singularity and the Cosmological Constant Problem

preprint2013arXivOpen access

Abstract

We consider a non singular origin for the Universe starting from an Einstein static Universe in the framework of a theory which uses two volume elements −gd4x\sqrt{-{g}}d^{4}x and Φd4xΦd^{4}x, where ΦΦ is a metric independent density, also curvature, curvature square terms, first order formalism and for scale invariance a dilaton field ϕϕ are considered in the action. In the Einstein frame we also add a cosmological term that parametrizes the zero point fluctuations. The resulting effective potential for the dilaton contains two flat regions, for ϕ→∞ϕ\rightarrow \infty relevant for the non singular origin of the Universe and ϕ→−∞ϕ\rightarrow -\infty, describing our present Universe. Surprisingly, avoidance of singularities and stability as ϕ→∞ϕ\rightarrow \infty imply a positive but small vacuum energy as ϕ→−∞ϕ\rightarrow -\infty. Zero vacuum energy density for the present universe is the "threshold" for universe creation. This requires a modified emergent universe scenario, where the universe although very old, it does have a beginning.

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