A 5D Holographic Dark Energy in DGP-Brane Cosmology

Abstract

This paper is aimed at investigating a 5D holographic dark energy in DGP-BRANE cosmology by employing a combination of Sne Ia, BAO and CMB observational data to fit the cosmological parameters in the model. We describe the dynamic of a FRW for the normal branch ($\epsilon$ = +1) of solutions of the induced gravity brane-world model. We take the matter in 5D bulk as holographic dark energy that its holographic nature is reproduced effectively in 4D. The cosmic evolution reveals that the effective 4D holographic dark energy behaves as quintessence while taking into account the 4D cold dark matter results in matter dominated universe followed by late time acceleration.

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• Holographic Dark Energy
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• Rényi Holographic Dark Energy
• Interacting Agegraphic Dark Energy Model in DGP Braneworld Cosmology: Dynamical System Approach
• Barrow Holographic Dark Energy in Brane World Cosmology
• Holographic Dark Energy from the Anti-de Sitter Black Hole
• Constant-roll Inflation in Brane Induced Gravity Cosmology
• Dynamical System Analysis of Randall-Sundrum Model with Tachyon Field on the Brane
• The Stability Analysis of Brane Induced Gravity with Quintessence Field on the Brane with a Gaussian Potential