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arXiv · gr-qc/9711068

Exponential potentials and cosmological scaling solutions

Edmund J Copeland·Andrew R Liddle·David Wands
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Abstract

We present a phase-plane analysis of cosmologies containing a barotropic fluid with equation of state $p_γ= (γ-1) ρ_γ$, plus a scalar field $ϕ$ with an exponential potential $V \propto \exp(-λκϕ)$ where $κ^2 = 8πG$. In addition to the well-known inflationary solutions for $λ^2 < 2$, there exist scaling solutions when $λ^2 > 3γ$ in which the scalar field energy density tracks that of the barotropic fluid (which for example might be radiation or dust). We show that the scaling solutions are the unique late-time attractors whenever they exist. The fluid-dominated solutions, where $V(ϕ)/ρ_γ\to 0$ at late times, are always unstable (except for the cosmological constant case $γ= 0$). The relative energy density of the fluid and scalar field depends on the steepness of the exponential potential, which is constrained by nucleosynthesis to $λ^2 > 20$. We show that standard inflation models are unable to solve this `relic density' problem.

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Edmund J Copeland, Andrew R Liddle, David Wands. 1998-07-01. Exponential potentials and cosmological scaling solutions. https://doi.org/10.1103/physrevd.57.4686

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