Figure - available from: International Journal of Theoretical Physics
This content is subject to copyright. Terms and conditions apply.
Download
View publication
The proper energy density (a) and the Euclidean energy density (b), for ψ0=1

The proper energy density (a) and the Euclidean energy density (b), for ψ0=1

Source publication
The reduced field amplitude ψ(s) (a) and the rescaled pressure...
The proper energy density (a) and the Euclidean energy density (b)
The logarithmic scale factor F(s) (a) and the cosmological scale factor...
The rescaled field ψ (a) and the rescaled pressure...
+1 The proper energy density (a) and the Euclidean energy density (b), for...
Spatially-Hyperbolic Friedmann–Robertson–Walker Universe with Potentially Broken Z 2−Symmetry
Article
Full-text available
  • Sep 2016
For the Friedmann–Robertson–Walker (FRW) Universe with negative curvature, sustained by a spontaneous Z 2− symmetry breaking scalar field, depending on time alone, we have derived the Einstein–Gordon system of equations. For physically relevant cases, the matter-curvature system have been numerically analyzed.
Cite
Download full-text

Similar publications

View