Scalar Field in Cosmology: Potential for Isotropization and Inflation process. One needs to introduce
scalar field with nonlinear
potential for the isotropization process
A new look at the Schrödinger equation in exact scalar field cosmology parameter and
scalar potential can be written in closed form. Earlier results are regained in our approach.
Renormalization for the self-potential of a scalar charge in static space-timesA method is presented which allows for the renormalization of the self-
potential for a
scalar point
Non-minimal two-loop inflation potential of a self-interacting
scalar field theory in curved spacetime. We use the
potential which contains
Flat Friedmann universe filled by dust and scalar field with multiple exponential potential scalar field with an unbounded from below
potential of the form V(phi) = W-0 - V-0 sinh(root3/2kappaphi
Model of Decaying Dark Energy Based on the Kaluza–Klein Theory© 2017 Springer Science+Business Media, LLC On the basis of a
scalar potential associated
Cold black holes and conformal continuationsWe study Einstein gravity minimally coupled to a
scalar field in a static, spherically symmetric