A 3D Phase Space Analysis of Scalar Field Potentials

TL;DR

This paper conducts a phase-space analysis of two scalar field potentials in Quintessence models, revealing new scaling solutions and attractors that could address the cosmic coincidence problem.

Contribution

It introduces a new broken exponential-law potential and systematically studies its cosmological evolution alongside the Recliner potential.

Findings

Discovery of new scaling solutions with constant energy density ratios

Identification of attractor solutions in the models

Construction of double potential models for cosmic acceleration

Abstract

In this study, we present the phase-space analysis of Quintessence models specified by the choice of two potentials, namely the Recliner potential and what we call the broken exponential-law potential, which is a new proposal. Using a dynamical system analysis we provide a systematic study of the cosmological evolution of the two models and their properties. We find new scaling solutions characterised by a constant ratio between the energy density of the scalar field and that of the matter component. These solutions are of high interest in light of the possibility to alleviate the coincidence problem. Additionally, the models also show attractor solutions. We finally construct concrete models built using a double potential according to which one potential realises the early-time scaling regime and the second one allows to exit this regime and to enter in the epoch of cosmic acceleration driven by a scalar-field dominated attractor point.