English

Non Singular Origin of the Universe and the Cosmological Constant Problem (CCP)

General Relativity and Quantum Cosmology 2015-05-28 v1 High Energy Physics - Theory

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 Φd4x\Phi d^{4}x, where Φ\Phi is a metric independent density, also curvature, curvature square terms, first order formalism and for scale invariance a dilaton field ϕ\phi 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\phi \rightarrow \infty relevant for the non singular origin of the Universe and ϕ\phi \rightarrow -\infty, describing our present Universe. Surprisingly, avoidance of singularities and stability as ϕ\phi \rightarrow \infty imply a positive but small vacuum energy as ϕ\phi \rightarrow -\infty. Zero vacuum energy density for the present universe is the "threshold" for universe creation.

Keywords

Cite

@article{arxiv.1105.3312,
  title  = {Non Singular Origin of the Universe and the Cosmological Constant Problem (CCP)},
  author = {E. I. Guendelman},
  journal= {arXiv preprint arXiv:1105.3312},
  year   = {2015}
}

Comments

awarded an honorable mention in the Gravity Research Foundation 2011 Awards for Essays in Gravitation for 2011