Inflationary solutions with a five dimensional complex scalar field

TL;DR

This paper explores inflationary solutions in a five-dimensional spacetime with a complex scalar field that depends on an extra dimension, revealing multiple oscillation periods that can cause accelerated cosmic expansion.

Contribution

It introduces a novel five-dimensional inflationary model with a complex scalar field exhibiting Kaluza-Klein modes, leading to multiple oscillation-driven inflationary phases.

Findings

Multiple oscillation periods of the scalar field are possible.

Oscillations can induce periods of accelerated expansion.

The model incorporates Kaluza-Klein excited modes.

Abstract

We discuss inflationary solutions of the coupled Einstein-Klein-Gordon equations for a complex field in a five dimensional spacetime with a compact $x^5$-dimension. As a new feature, the scalar field contains a dependence on the extra dimension of the form $\exp(i m x^5) $, corresponding to Kaluza-Klein excited modes. In a four dimensional picture, a nonzero $m$ implies the presence of a new term in the scalar field potential. An interesting feature of these solutions is the possible existence of several periods of oscillation of the scalar field around the equilibrium value at the minimum of the potential. These oscillations lead to cosmological periods of accelerated expansion of the universe.