Holographic Dark Energy from a Modified GBIG Scenario

Abstract

We construct a holographic dark energy model in a braneworld setup that gravity is induced on the brane embedded in a bulk with Gauss-Bonnet curvature term. We include possible modification of the induced gravity and its coupling with a canonical scalar field on the brane. Through a perturbational approach to calculate the effective gravitation constant on the brane, we examine the outcome of this model as a candidate for holographic dark energy.

13 pages, accepted for publication in IJMPD

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• Gauss-Bonnet Inflation after Planck2018
• DBI inflation with a non-minimally coupled Gauss-Bonnet term
• Fractional Holographic Dark Energy
• Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE
• Large Non-Gaussianity in Non-Minimally Coupled Derivative Inflation with Gauss-Bonnet Correction
• Tsallis holographic dark energy with power law ansatz approach
• Interacting Ricci Logarithmic Entropy Corrected Holographic Dark Energy in Brans-Dicke Cosmology
• Cosmological dynamics of a non-minimally coupled bulk scalar field in DGP setup
• On the holographic dark energy in chameleon scalar-tensor cosmology
• New perspectives on future rip scenarios with holographic dark energy
• Modified gravity in a viscous and non-isotropic background
• Rips and regular future scenario with Holographic Dark Energy: A comprehensive look
• Comments on ${}^{"}$Cosmic evolution in Brans-Dicke chameleon cosmology${}^{"}$