Reconstruction of Five-dimensional Bounce cosmological Models From Deceleration Factor

Details Reconstruction of Five-dimensional Bounce cosmological Models From Deceleration Factor Reconstruction of Five-dimensional Bounce cosmological Models From Deceleration Factor

2006-01-20

arxiv.org/abs/astro-ph/0601471v1

Int.J.Theor.Phys.45:843-850,2006

Astronomy and Astrophysics

Astrophysics

5 pages, 1 figure, to be published in IJTP

Scientific paper

10.1007/s10773-006-9073-8

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.

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