Friedmann-like equations for High Energy Area of Universe
arXiv:1207.1801 · doi:10.1007/s10773-012-1243-2
Abstract
In this paper, evolution of the high energy area of universe, through the scenario of 5 dimensional (5D) universe, has been studied. For this purpose, we solve Einstein equations for 5D metric and 5D perfect fuid to derive Friedmann-like equations. Then we obtain the evolution of scale factor and energy density with respect to both space-like and time-like extra dimensions. We obtain the novel equations for the space-like extra dimension and show that the matter with zero pressure cannot exist in the bulk. Also, for dark energy fuid and vacuum fluid, we have both accelerated expansion and contraction in the bulk.
9 pages, Accepted to publication in IJTP 26 June 2012. arXiv admin note: substantial text overlap with arXiv:1202.4973
References in corpus (9)
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Cosmic Acceleration and Modified Gravitational Models
- f(R)-Brane
- Accelerating Universe from the Evolution of Extra Dimensions
- Quantum-Corrected Black Hole Thermodynamics in Extra Dimensions
- Five Dimensional Cosmological Models in General Relativity
- A Way to the Dark Side of the Universe through Extra Dimensions
- Bulk Scale Factor at Very Early Universe
- Alternative inflationary scenario due to compact extra dimensions