The transition of equation of state of effective dark energy in the DGP model with bulk contents
arXiv:0708.0992 · doi:10.1103/PhysRevD.76.124026
Abstract
We investigate the effect of the bulk contents in the DGP braneworld on the evolution of the universe. We find that although the pure DGP model cannot accommodate the transition of the effective equation of state of dark energy, once the bulk matter T^5_5 is considered, the modified model can realize the w_{eff} crossing -1. However this transition of the equation of state cannot be realized by just considering bulk-brane energy exchange or the GB effect while the bulk matter contribution is not included. T^5_5 plays the major role in the modified DGP model to have the w crossing -1 behavior. We show that our model can describe the super-acceleration of our universe with the equation of state of the effective dark energy and the Hubble parameter in agreement with observations.
arXiv comment25 pages, 11 figures, revised version, accepted for publication in Phys. Rev. D
References in corpus (69)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- A Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- Cosmological Imprint of an Energy Component with General Equation of State
- 4D Gravity on a Brane in 5D Minkowski Space
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- An alternative to quintessence
- Phantom Energy and Cosmic Doomsday
- A Model of Holographic Dark Energy
- Cosmological Tracking Solutions
- Constraints on the redshift dependence of the dark energy potential
- Dark Energy Constraints from the Cosmic Age and Supernova
- Properties of singularities in (phantom) dark energy universe
- Quantum deSitter cosmology and phantom matter
- Cosmology on a Brane in Minkowski Bulk
- Cosmological Evolution of a Quintom Model of Dark Energy
- Formalising the Slow-Roll Approximation in Inflation
- The phantom menaced: constraints on low-energy effective ghosts
- Can dark energy evolve to the Phantom?
- Transition of the dark energy equation of state in an interacting holographic dark energy model
- Quintessential inflation
- The final state and thermodynamics of dark energy universe
- Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB
- Is there Supernova Evidence for Dark Energy Metamorphosis ?
- Quantum effects can render w<-1 on cosmological scales
- The Holographic Dark Energy in a Non-flat Universe
- Cosmological dynamics on the brane
- The case for dynamical dark energy revisited
- Cosmic Structure Growth and Dark Energy
- Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom
- Constraints on the interacting holographic dark energy model
- Cosmological parameters from supernova observations: A critical comparison of three data sets
- Cosmology and Astrophysical Constraints of Gauss-Bonnet Dark Energy
- Gauss-Bonnet Quintessence: Background Evolution, Large Scale Structure and Cosmological Constraints
- Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
- B-Inflation
- Bulk-Brane Interaction and Holographic Dark Energy
- Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data
- Two-field Models of Dark Energy with Equation of State Across -1
- Uncorrelated Measurements of the Cosmic Expansion History and Dark Energy from Supernovae
- Crossing w=-1 in Gauss-Bonnet Brane World with Induced Gravity
- A Single Scalar Field Model of Dark Energy with Equation of State Crossing -1
- Direct Determination of the Kinematics of the Universe and Properties of the Dark Energy as Functions of Redshift
- Loop Corrections to Scalar Quintessence Potentials
- Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
- Brane cosmology with curvature corrections
- Model independent analysis of dark energy I: Supernova fitting result
- Vacuum Fluctuations of Energy Density can lead to the observed Cosmological Constant
- Late acceleration and crossing in induced gravity
- Dark energy transition between quintessence and phantom regimes - an equation of state analysis
- Induced Gravity on RS Branes
- Cosmological evolution with brane-bulk energy exchange
- Holography and Brane-bulk Energy Exchange
- Effective State Metamorphosis in Semi-Classical Loop Quantum Cosmology
- Super-acceleration on the Brane by Energy Flow from the Bulk
- A late-accelerating universe with no dark energy - and a finite-temperature big bang
- Brane-bulk energy exchange : a model with the present universe as a global attractor
- Brane cosmological evolution with a general bulk matter configuration
- The Generalized Dark Radiation and Accelerated Expansion in Brane Cosmology
- String inspired explanation for the super-acceleration of our universe
- Brane Cosmological Evolution With Bulk Matter
- Observational Constraints on Accelerating Brane Cosmology with Exchange between the Bulk and Brane
- On the thin-shell limit of branes in the presence of Gauss-Bonnet interactions
- Dark energy from bulk matter
- Modified brane cosmologies with induced gravity, arbitrary matter content and a Gauss-Bonnet term in the bulk
- Observational constrains on the DGP brane-world model with a Gauss-Bonnet term in the bulk
Cited by in corpus (21)
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
- Effects of dark sectors' mutual interaction on the growth of structures
- A Completely Regular Quantum Stress Tensor with
- Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
- Dynamical analysis for a vector-like dark energy
- A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane
- Metastable dark energy
- Phantom-like behaviour in a brane-world model with curvature effects
- Fractional dark energy
- The Dark Sector Cosmology
- A note on interacting holographic dark energy with a Hubble-scale cutoff
- Cosmological perturbations and dynamical analysis for interacting quintessence
- Crossing the cosmological constant line in a dilatonic brane-world model with and without curvature corrections
- Cosmological tracking solution and the Super-Higgs mechanism
- Constraints on interacting dark energy revisited: implications for the Hubble tension
- Backreaction of superhorizon perturbations in scalar field cosmologies
- A Lorentz Invariance Violating Cosmology on the DGP Brane
- Phantom-like effects in asymmetric brane embedding with induced gravity and the Gauss-Bonnet term in the Bulk
- Dark Energy and Modified Scale Covariant Theory of Gravitation
- Behavior of gravity around a crossing of the phantom divide