Abstract
We examine the simplest inflection point quintessence model, with a potential given by V(ϕ)=V0+V3ϕ3. This model can produce either asymptotic de Sitter expansion or transient acceleration, and we show that it does not correspond to either pure freezing or thawing behavior. We derive observational constraints on the initial value of the scalar field, ϕi, and V3/V0 and find that small values of either ϕi or V3/V0 are favored. While most of the observationally-allowed parameter space yields asymptotic de Sitter evolution, there is a small region, corresponding to large V3/V0 and small ϕi, for which the current accelerated expansion is transient. The latter behavior is potentially consistent with a cyclic universe.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.