Bifurcations in Ratra-Peebles quintessence models and their extensions
arXiv:1901.06578 · doi:10.1140/epjc/s10052-019-7299-x
Abstract
We have used the dynamical system approach in order to investigate the dynamics of cosmological models of the flat Universe with a non-minimally coupled canonical and phantom scalar field and the Ratra-Peebles potential. Applying methods of the bifurcation theory we have found three cases for which the Universe undergoes a generic evolution emerging from either the deSitter or the static Universe state and finishing at the deSitter state, without the presence of the initial singularity. This generic class of solutions explains both the inflation and the late-time acceleration of the Universe. In this class inflation is an endogenous effect of dynamics itself.
LaTeX, 25 pages, 16 figures
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- The non-minimal coupling constant and the primordial de Sitter state
- Cosmological dynamics and bifurcation analysis of the general non-minimally coupled scalar field models
- Dynamical system analysis of quintessence dark energy model