Reconstruction of Five-dimensional Bounce cosmological Models From Deceleration Factor

Abstract

In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions $\mu (t)$ and $\nu (t)$. It is shown that $\mu (t)$ can be rewritten as a new arbitrary function $f(z)$ in terms of redshift $z$ and the $f(z)$ can be determined by choosing particular deceleration parameters $q(z)$ which gives early deceleration and late time acceleration. In this way, the $5D$ cosmological model can be reconstructed and the evolution of the universe can be determined.

5 pages, 1 figure, to be published in IJTP

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Cited by in corpus (6)

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• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• Statefinder Parameters for Five-Dimensional Cosmology
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
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