String inspired explanation for the super-acceleration of our universe
arXiv:0704.0666 · doi:10.1103/PhysRevD.75.123513
Abstract
We investigate the effect of the bulk content in the general Gauss-Bonnet braneworld on the evolution of the universe. We find that the Gauss-Bonnet term and the combination of the dark radiation and the matter content of the bulk play a crucial role in the universe evolution. We show that our model can describe the super-acceleration of our universe with the equation of state of the effective dark energy in agreement with observations.
12 pages, 9 figures, references added
References in corpus (60)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- Cosmological Imprint of an Energy Component with General Equation of State
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Cosmological Constant - the Weight of the Vacuum
- An alternative to quintessence
- A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
- Phantom Energy and Cosmic Doomsday
- A Model of Holographic Dark Energy
- Cosmological Tracking Solutions
- New Constraints on , , and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
- Dark Energy Constraints from the Cosmic Age and Supernova
- Properties of singularities in (phantom) dark energy universe
- Quantum deSitter cosmology and phantom matter
- Cosmological Evolution of a Quintom Model of Dark Energy
- Braneworld models 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
- Dark Matter and Dark Energy
- Is there Supernova Evidence for Dark Energy Metamorphosis ?
- The Holographic Dark Energy in a Non-flat Universe
- 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
- B-Inflation
- 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
- 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
- Unified dark energy models : a phenomenological approach
- 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
- Constraints on Scalar-Field Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift
- Brane-bulk energy exchange : a model with the present universe as a global attractor
- Realizing Scale-invariant Density Perturbations in Low-energy Effective String Theory
- Brane cosmological evolution with a general bulk matter configuration
- The Generalized Dark Radiation and Accelerated Expansion in Brane Cosmology
- Observational Constraints on Accelerating Brane Cosmology with Exchange between the Bulk and Brane
- Brane Cosmological Evolution With Bulk Matter
- Dark energy from bulk matter
Cited by in corpus (28)
- Bouncing Universe with Quintom Matter
- Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
- On Perturbations of Quintom Bounce
- Instability of QCD ghost dark energy model
- Effects of dark sectors' mutual interaction on the growth of structures
- Interacting Ghost Dark Energy in Non-Flat Universe
- Thermodynamics on the apparent horizon in generalized gravity theories
- Quintessence Ghost Dark Energy Model
- A Completely Regular Quantum Stress Tensor with
- Tsallis Agegraphic Dark Energy Model
- Cosmic acceleration with a negative cosmological constant in higher dimensions
- Effects of Anisotropy on the Sign-Changeable Interacting Tsallis Holographic Dark Energy
- Phantom-like behaviour in a brane-world model with curvature effects
- The transition of equation of state of effective dark energy in the DGP model with bulk contents
- Modified brane cosmologies with induced gravity, arbitrary matter content and a Gauss-Bonnet term in the bulk
- Crossing the phantom divide in brane cosmology with curvature corrections and brane-bulk energy transfer
- Brane-Bulk energy exchange and agegraphic dark energy
- Transient Crossing of Phantom divide line under Gauss-Bonnet interaction
- Sounds of instability from generalized QCD ghost dark energy
- Exploring the new Tsallis agegraphic dark energy with interaction through statefinder
- Crossing the cosmological constant line in a dilatonic brane-world model with and without curvature corrections
- Observational constrains on the DGP brane-world model with a Gauss-Bonnet term in the bulk
- Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
- Observational constraints on the braneworld model with brane-bulk energy exchange
- Phantom-like effects in asymmetric brane embedding with induced gravity and the Gauss-Bonnet term in the Bulk
- Behavior of gravity around a crossing of the phantom divide
- Effective cosmological equations of induced f(R) gravity
- Spherically symmetric solutions in a FRW background