Reconstruction of 5D Cosmological Models From Equation of State of Dark Energy
Abstract
We consider a class of five-dimensional cosmological solutions which contains two arbitrary function μ(t) and (t). We found that the arbitrary function μ(t) contained in the solutions can be rewritten in terms of the redshift z as a new arbitrary function f(z). We further showed that this new arbitrary function f(z) could be solved out for four known parameterized equations of state of dark energy. Then the 5D models can be reconstructed and the evolution of the density and deceleration parameters of the universe can be determined.
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