Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe

Abstract

We study the correspondence between the interacting new agegraphic dark energy and the polytropic gas model of dark energy in the non-flat FRW universe. This correspondence allows to reconstruct the potential and the dynamics for the scalar field of the polytropic model, which describe accelerated expansion of the universe.

9 pages

References in corpus (44)

• 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
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Cosmological parameters from SDSS and WMAP
• A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
• A Model of Holographic Dark Energy
• Coupled Quintessence
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Holographic dark energy and cosmic coincidence
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Scaling solutions in general non-minimal coupling theories
• A Dark Energy Model Characterized by the Age of the Universe
• A New Model of Agegraphic Dark Energy
• Probable Values of the Cosmological Constant in a Holographic Theory
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• 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
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• Equation of state for an interacting holographic dark energy model
• Reconstructing holographic quintessence
• Cosmological Constraints on New Agegraphic Dark Energy
• 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
• 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
• 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
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe

Cited by in corpus (22)

• Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models
• Interacting entropy-corrected new agegraphic dark energy in Brans-Dicke cosmology
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Statefinder diagnostic and $w-w^{\prime }$ analysis for interacting polytropic gas dark energy model
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Interacting viscous ghost tachyon, K-essence and dilaton scalar field models of dark energy
• An effective quintessence field with a power-law potential
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Cosmological implications of interacting polytropic gas dark energy model in non-flat universe
• Cosmological constraints on polytropic gas model
• Thermodynamical description of interacting entropy-corrected new agegraphic dark energy
• QCD modified ghost scalar field dark energy models
• Thermodynamic behavior and stability of Polytropic gas
• Reconstructing $f(T)$ modified gravity from ECHDE and ECNADE models
• Polytropic gas scalar field models of dark energy
• Black holes immersed in polytropic scalar field gas
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
• Power Law Entropy Corrected New-Agegraphic Dark Energy in Hořava-Lifshitz Cosmology
• Thermodynamic descriptions of Polytropic gas and its viscous type as the dark energy candidates
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• The $D$-dimensional charged AdS black holes solutions in polytropic dark energy from Barrow entropy
• Chaplygin and Polytropic gases Teleparallel Robertson-Walker $F(T)$ gravity solutions