A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane

Abstract

We study dynamics of equation of state parameter for a non-minimally coupled quintom dark energy component on the warped DGP brane. We investigate crossing of the cosmological constant line in this scenario. This crossing occurs in both DGP${}^{\pm }$ branches of the model.

arXiv comment28 pages, 10 figures

References in corpus (64)

• 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
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• The Hierarchy Problem and New Dimensions at a Millimeter
• Dynamics of dark energy
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• f(R) Theories Of Gravity
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• New Dimensions at a Millimeter to a Fermi and Superstrings at a TeV
• 4D Gravity on a Brane in 5D Minkowski Space
• Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
• A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
• Phenomenology, Astrophysics and Cosmology of Theories with Sub-Millimeter Dimensions and TeV Scale Quantum Gravity
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
• Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
• MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees
• Properties of singularities in (phantom) dark energy universe
• Accelerated Universe from Gravity Leaking to Extra Dimensions
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Extended Theories of Gravity and their Cosmological and Astrophysical Applications
• Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters
• Cosmology on a Brane in Minkowski Bulk
• Cosmological Evolution of a Quintom Model of Dark Energy
• Can dark energy evolve to the Phantom?
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Is there Supernova Evidence for Dark Energy Metamorphosis ?
• Dark Energy: Vacuum Fluctuations, the Effective Phantom Phase, and Holography
• A Measurement of the Angular Power Spectrum of the CMB from l = 100 to 400
• Hessence: A New View of Quintom Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks
• Inflation and quintessence with nonminimal coupling
• Cosmological parameters from supernova observations: A critical comparison of three data sets
• Quintom models with an equation of state crossing -1
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data
• Non-minimal coupling of the scalar field and inflation
• Supernovae, CMB, and Gravitational Leakage into Extra Dimensions
• Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
• Uncorrelated Measurements of the Cosmic Expansion History and Dark Energy from Supernovae
• Crossing w=-1 in Gauss-Bonnet Brane World with Induced Gravity
• Effective Gravitational Equations on Brane World with Induced Gravity
• Coupled oscillators as models of quintom dark energy
• Direct Determination of the Kinematics of the Universe and Properties of the Dark Energy as Functions of Redshift
• Cosmic Duality in Quintom Universe
• A String-Inspired Quintom Model Of Dark Energy
• Dark energy, inflation and dark matter from modified F(R) gravity
• Quintom Cosmology with General Potentials
• Model independent analysis of dark energy I: Supernova fitting result
• Transition from quintessence to phantom phase in quintom model
• Crossing $w=-1$ by a single scalar on a Dvali-Gabadadze-Porrati brane
• Critical comments on the paper "Crossing $\omega =-1$ by a single scalar field on a Dvali-Gabadadze-Porrati brane" by H Zhang and Z-H Zhu [Phys.Rev.D75,023510(2007)]
• Oscillating universe with quintom matter
• QCD uncertainties at the LHC and the implications of HERA
• Induced gravity with a non-minimally coupled scalar field on the brane
• The transition of equation of state of effective dark energy in the DGP model with bulk contents
• Crossing the phantom divide in brane cosmology with curvature corrections and brane-bulk energy transfer
• Asymptotic behavior of w in general quintom model
• Dark Energy and its Implications for Gravity
• Non-Minimal Inflation on the Warped DGP Brane
• Quintom dark energy in DGP braneworld cosmology

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• Phantom-like effects in asymmetric brane embedding with induced gravity and the Gauss-Bonnet term in the Bulk
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