Non Singular Origin of the Universe and the Cosmological Constant Problem (CCP)
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 and , where is a metric independent density, also curvature, curvature square terms, first order formalism and for scale invariance a dilaton field 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 relevant for the non singular origin of the Universe and , describing our present Universe. Surprisingly, avoidance of singularities and stability as imply a positive but small vacuum energy as . 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