arXiv · hep-ph/9501293
A new cosmological constant model
Abstract
We propose a new cosmological model with a time-dependent cosmological constant ($Λ\propto 1/t^2$), which starting at the Planck time as $Λ_{Pl}\sim M^2_{Pl}$, evolves to the present-day allowed value of $Λ_0\sim10^{-120}M^2_{Pl}$. This scenario is supported by non-critical string theory considerations. We compute the age of the Universe and the time-dependence of the scale factor in this model, and find general agreement with recent determinations of the Hubble parameter for substantial values of $Ω_{\rm Λ}$. This effectively low-density open Universe model differs from the traditional cosmological constant model, and has observable implications for particle physics and cosmology.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
J. Lopez, D. Nanopoulos. 1995-01-13. A new cosmological constant model. https://doi.org/10.1142/s0217732396000023
Cite the original work for its findings. Save a collection to share your selection of sources.