Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe

Abstract

We study the correspondence between the tachyon, K-essence and dilaton scalar field models with the interacting new agegraphic dark energy model in the non-flat FRW universe. We reconstruct the potentials and the dynamics for these scalar field models, which describe accelerated expansion of the universe.

arXiv comment9 pages

References in corpus (95)

• 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
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Cosmological parameters from SDSS and WMAP
• A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
• Cosmology and the Fate of Dilatation Symmetry
• An alternative to quintessence
• A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
• Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• A Model of Holographic Dark Energy
• k-Inflation
• Essentials of k-essence
• Coupled Quintessence
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Kinetically Driven Quintessence
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Properties of singularities in (phantom) dark energy universe
• Rolling Tachyon
• Perturbations in k-inflation
• Tachyon Matter
• Accelerated Universe from Gravity Leaking to Extra Dimensions
• Accelerated expansion of the universe driven by tachyonic matter
• Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
• Quantum deSitter cosmology and phantom matter
• A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background
• Braneworld models of dark energy
• Holographic dark energy and cosmic coincidence
• Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Scaling solutions in general non-minimal coupling theories
• A high resolution foreground cleaned CMB map from WMAP
• A Dark Energy Model Characterized by the Age of the Universe
• Ghost Inflation
• A New Model of Agegraphic Dark Energy
• The Emergent Universe: inflationary cosmology with no singularity
• Probable Values of the Cosmological Constant in a Holographic Theory
• Can the clustered dark matter and the smooth dark energy arise from the same scalar field ?
• Quintessence as a run-away dilaton
• Supersymmetric World-volume Action for Non-BPS D-branes
• Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background
• The Holographic Dark Energy in a Non-flat Universe
• Probing the Coupling between Dark Components of the Universe
• T-duality and Actions for Non-BPS D-branes
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• Dilatonic ghost condensate as dark energy
• New infrared cut-off for the holographic scalar fields models of dark energy
• Constraints on the interacting holographic dark energy model
• Dynamics of interacting dark energy
• deSitter brane universeinduced by phantom and quantum effects
• Interacting dark energy, holographic principle and coincidence problem
• Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Cosmological dynamics of the tachyon with an inverse power-law potential
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• Equation of state for an interacting holographic dark energy model
• Cosmological constraints from Archeops
• Is the Low CMB Quadrupole a Signature of Spatial Curvature?
• B-Inflation
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Reconstructing holographic quintessence
• Cosmological Constraints on New Agegraphic Dark Energy
• The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• A unified approach to scaling solutions in a general cosmological background
• Instability of agegraphic dark energy models
• Interacting Agegraphic Dark Energy
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• Interacting holographic dark energy in Brans-Dicke theory
• Agegraphic dark energy as a quintessence
• Holographic tachyon model
• Interacting agegraphic dark energy models in non-flat universe
• Quintessence reconstruction of the new agegraphic dark energy model
• Can we have inflation with Omega > 1?
• WMAP data and the curvature of space
• New holographic scalar field models of dark energy in non-flat universe
• General analytic formulae for attractor solutions of scalar-field dark energy models and their multi-field generalizations
• Interacting agegraphic tachyon model of dark energy
• The Abell Cluster A586 and the Detection of the Equivalence Principle
• Expansion, Geometry, and Gravity
• Interacting polytropic gas model of phantom dark energy in non-flat universe
• A Note on Agegraphic Dark Energy
• Cosmological model with energy transfer
• New agegraphic dark energy model with generalized uncertainty principle
• On the Stability of Phantom K-essence Theories
• Interacting new agegraphic dark energy in non-flat Brans-Dicke cosmology
• Probing the curvature of the Universe from supernova measurement
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• New agegraphic dark energy as a rolling tachyon
• The transient and the late time attractor tachyon dark energy: Can we distinguish it from quintessence ?
• Comment on "Interacting holographic dark energy model and generalized second law of thermodynamics in a non-flat universe", by M.R. Setare (JCAP 01, 023, 2007)

Cited by in corpus (40)

• Power-Law Entropy Corrected Holographic Dark Energy Model
• Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology
• Interacting holographic dark energy with logarithmic correction
• Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models
• Interacting entropy-corrected agegraphic-tachyon dark energy
• Interacting Ricci Dark Energy with Logarithmic Correction
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Interacting entropy-corrected new agegraphic dark energy in Brans-Dicke cosmology
• Cosmic acceleration in non-flat $f(T)$ cosmology
• Interacting entropy-corrected new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Tachyon Reconstruction of Ghost Dark Energy
• Reconstruction of quintessence field for the THDE with swampland correspondence in $f(R,T)$ gravity
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Agegraphic dark energy: growth index and cosmological implications
• Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe
• Evaluation of cosmological models in $f(R,T)$ gravity in different dark energy scenario
• Restoring New Agegraphic Dark Energy in RS II Braneworld
• Interacting viscous ghost tachyon, K-essence and dilaton scalar field models of dark energy
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Compatibility between the scalar field models of tachyon, $k$-essence and quintessence in $f(R,T)$ gravity
• Interacting New Agegraphic Dark Energy in a Cyclic Universe
• QCD modified ghost scalar field dark energy models
• Agegraphic reconstruction of modified $F(R)$ and $F(\mathcal{G})$ gravities
• Thermodynamical description of interacting entropy-corrected new agegraphic dark energy
• The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Cosmological Evolution of Pilgrim Dark Energy
• Power-law entropy corrected new holographic scalar field models of dark energy with modified IR-cutoff
• Interacting entropy-corrected holographic scalar field models in non-flat universe
• Cosmological Model of Interacting Tachyon Field
• Reconstructing $f(T)$ modified gravity from ECHDE and ECNADE models
• Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory
• The universe dynamics in the tachyon cosmology with non-minimal coupling to matter
• Chameleon mechanism with a new potential
• Power Law Entropy Corrected New-Agegraphic Dark Energy in Hořava-Lifshitz Cosmology
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
• Ghost Chaplygin scalar field model of dark energy
• Modified gravity in a viscous and non-isotropic background
• Constraining tachyonic inflationary β-exponential model with Continuous Spontaneous Localization collapse scheme
• Quintessence reconstruction of interacting HDE in a non-flat universe
• Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology