Bouncing Model in Brane World Theory

Abstract

We examine the nonlinear dynamics of a closed Friedmann-Robertson-Walker universe in the framework of Brane World formalism with a timelike extra dimension. In this scenario, the Friedmann equations contain additional terms arising from the bulk-brane interaction which provide a concrete model for nonsingular bounces in the early phase of the Universe. We construct a nonsingular cosmological scenario sourced with dust, radiation and a cosmological constant. The structure of the phase space shows a nonsingular orbit with two accelerated phases, separated by a smooth transition corresponding to a decelerated expansion. Given observational parameters we connect such phases to a primordial accelerated phase, a soft transition to Friedmann (where the classical regime is valid), and a graceful exit to a de Sitter accelerated phase.

References in corpus (4)

• Cosmology without inflation
• The Wheeler-DeWitt Quantization Can Solve the Singularity Problem
• Bouncing Braneworld Cosmologies and Initial Conditions to Inflation
• Gravitational Collapse and Black Hole Thermodynamics In Braneworld Scenario

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