On the dynamics of the universe in D spatial dimensions

In this paper we present the equations of the evolution of the universe in D spatial dimensions, as a generalization of the work of Lima (2001). We discuss the Friedmann-Robertson-Walker cosmological equations in D spatial dimensions for a simple fluid with equation of state p = ωD ρ. It is possible to reduce the multidimensional equations to the equation of a point particle system subject to a linear force. This force can be expressed as an oscillator equation, anti-oscillator or a free particle equation, depending on the k parameter of the spatial curvature. An interesting result is the independence on the dimension D in a de Sitter evolution. ® We also stress the generality of this procedure with a cosmological A term. A more interesting result is that the reduction of the dimensionality leads naturally to an accelerated expansion of the scale factor in the plane case.

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Bibliographic Details
Main Authors: Holanda,R. F. L., Pereira,S. H.
Format: Digital revista
Language:English
Published: Universidad Nacional Autónoma de México, Instituto de Astronomía 2012
Online Access:http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012012000200009
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