5 research outputs found

    Cosmological dynamics of exponential gravity

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    We present a detailed investigation of the cosmological dynamics based on exp⁡(−R/Λ)\exp (-R/{\Lambda}) gravity. We apply the dynamical system approach to both the vacuum and matter cases and obtain exact solutions and their stability in the finite and asymptotic regimes. The results show that cosmic histories exist which admit a double de-Sitter phase which could be useful for describing the early and the late-time accelerating universe.Comment: 17 pages LaTeX, 3 figure

    Compactifying the state space for alternative theories of gravity

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    In this paper we address important issues surrounding the choice of variables when performing a dynamical systems analysis of alternative theories of gravity. We discuss the advantages and disadvantages of compactifying the state space, and illustrate this using two examples. We first show how to define a compact state space for the class of LRS Bianchi type I models in RnR^n-gravity and compare to a non--compact expansion--normalised approach. In the second example we consider the flat Friedmann matter subspace of the previous example, and compare the compact analysis to studies where non-compact non--expansion--normalised variables were used. In both examples we comment on the existence of bouncing or recollapsing orbits as well as the existence of static models.Comment: 18 pages, revised to match published versio

    Dynamics of f(R)-cosmologies containing Einstein static models

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    We study the dynamics of homogeneous isotropic FRW cosmologies with positive spatial curvature in f(R)f(R)-gravity, paying special attention to the existence of Einstein static models and only study forms of f(R)=Rnf(R)=R^n for which these static models have been shown to exist. We construct a compact state space and identify past and future attractors of the system and recover a previously discovered future attractor corresponding to an expanding accelerating model. We also discuss the existence of universes which have both a past and future bounce, a phenomenon which is absent in General Relativity.Comment: 14 pages, 6 figure
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