Phantom-Like Behavior of a DGP-Inspired Scalar-Gauss-Bonnet Gravity
arXiv:0910.0611 · doi:10.1088/1475-7516/2009/10/022
Abstract
We study the phantom-like behavior of a DGP-inspired braneworld scenario where curvature correction on the brane is taken into account. We include a possible modification of the induced gravity on the brane by incorporating higher order curvature terms of Gauss-Bonnet type. We investigate the cosmological implications of the model and we show that the normal branch of the scenario self-accelerates in this modified scenario without introducing any dark energy component. Also, a phantom-like behavior can be realized in this model without introducing any phantom field that suffers from serious difficulties such as violation of the null energy condition.
20 pages, revised version, typos fixed, new references, to appear in JCAP
References in corpus (31)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Disappearing cosmological constant in f(R) gravity
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Dark energy in modified Gauss-Bonnet gravity: late-time acceleration and the hierarchy problem
- Dark energy cosmology from higher-order, string-inspired gravity and its reconstruction
- Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
- String-inspired Gauss-Bonnet gravity reconstructed from the universe expansion history and yielding the transition from matter dominance to dark energy
- The future evolution and finite-time singularities in -gravity unifying the inflation and cosmic acceleration
- Cosmology and Astrophysical Constraints of Gauss-Bonnet Dark Energy
- Gauss-Bonnet Quintessence: Background Evolution, Large Scale Structure and Cosmological Constraints
- Dark Interactions and Cosmological Fine-Tuning
- Observational constraints on self-accelerating cosmology
- Accelerating cosmologies from non-local higher-derivative gravity
- Constructing stabilized brane world models in five-dimensional Brans-Dicke theory
- Ghosts in the self-accelerating universe
- Interacting Vector-like Dark Energy, the First and Second Cosmological Coincidence Problems
- Stability of the Einstein static universe in modified Gauss-Bonnet gravity
- Crossing the phantom divide without phantom matter
- Mimicking Lambda with a spin-two ghost condensate
- Reconstructing the dark energy equation of state with varying couplings
- Phantom Dark Energy Models with Negative Kinetic Term
- Holographic Dark Energy and the Universe Expansion Acceleration
- Phantom-Like Behavior in -Gravity
- Modified gravity as realistic candidate for dark energy, inflation and dark matter
- Phantom-like behaviour in a brane-world model with curvature effects
- A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane
- Crossing the Phantom Divide Line in a DGP-Inspired -Gravity
- Dynamical-Screening and the Phantom-Like Effects in a DGP-Inspired Model
Cited by in corpus (5)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Observational Constraints on the Normal Branch of a Warped DGP Cosmology
- Observational constraints on Chaplygin cosmology in a braneworld scenario with induced gravity and curvature effect
- Phantom-like effects in asymmetric brane embedding with induced gravity and the Gauss-Bonnet term in the Bulk
- Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane