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A Degenerate Bogdanov-Takens Normal Form for FLRW Cosmologies

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arxiv 1607.02401 v2 pith:TWMEXSNH submitted 2016-07-08 gr-qc hep-th

classification gr-qchep-th
keywords constanteinsteinequationsfieldformnormalbogdanov-takenscosmological
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abstract

In this paper, we first show that the Einstein field equations for all perfect-fluid FLRW cosmologies can be written as a planar dynamical system with the equation of state parameter $w$ and cosmological constant $\Lambda$ as parameters. An important equilibrium point of this dynamical system is the origin which represents Minkowski spacetime. It is shown that the Einstein field equations in a neigbourhood of this point are equivalent to a degenerate Bogdanov-Takens normal form. This normal form admits a set of equilibrium points that describes a set of solutions to the Einstein field equations that have a constant rate of expansion, negative spatial curvature, zero cosmological constant and dust.

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Cited by 1 Pith paper

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  1. Geodesic dynamics in brane-de Sitter wormholes

    gr-qc 2025-04 conditional novelty 5.0 of 10

    For an asymptotically de Sitter brane wormhole, the throat is shown to be an unstable fixed point and photon sphere, with a claimed Bogdanov-Takens bifurcation for radial null geodesics.

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