A generalized equation of state for dark energy
arXiv:0905.4052 · doi:10.1103/PhysRevD.80.043521
Abstract
A generalized parameterization for the dark energy equation of state (EoS) is proposed and some of its cosmological consequences are investigated. We show that in the limit of the characteristic dimensionless parameter and -1 some well-known EoS parameterizations are fully recovered whereas for other values of the proposed parameterization admits a wider and new range of cosmological solutions. We also discuss possible constraints on the parameters from current observational data.
6 pages, 4 figures, Accepted for publication in Phys. Rev. D
References in corpus (46)
- 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
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- 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
- The Case for a Positive Cosmological Lambda-term
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Constraints on the redshift dependence of the dark energy potential
- Can the dark energy equation-of-state parameter w be less than -1?
- Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
- Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
- Cosmology with a Primordial Scaling Field
- WMAP constraints on low redshift evolution of dark energy
- Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and Three-Year Wilkinson Microwave Anisotropy Probe Observations
- New dark energy constraints from supernovae, microwave background and galaxy clustering
- A parametric model for dark energy
- The foundations of observing dark energy dynamics with the Wilkinson Microwave Anisotropy Probe
- The Fate of Bound Systems in Phantom and Quintessence Cosmologies
- Gravitational Lensing as a Probe of Quintessence
- Kinematic Constraints to the Transition Redshift from SNe Ia Union Data
- Superquintessence
- Opportunities for future supernova studies of cosmic acceleration
- Testing dark energy beyond the cosmological constant barrier
- Cosmological Constraints from Hubble Parameter versus Redshift Data
- Mapping the Cosmological Expansion
- Supernovae and the Nature of the Dark Energy
- Scalar-field-dominated cosmology with a transient accelerating phase
- Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
- Measuring Time-Dependence of Dark Energy Density from Type Ia Supernova Data
- Dark Energy and Some Alternatives: a Brief Overview
- Energy Conditions and Segre Classification of Phantom Fields
- Testing the Cosmological Constant as a Candidate for Dark Energy
- Cosmological Constraints from Hubble Parameter on f(R) Cosmologies
- Looking Beyond Lambda with the Union Supernova Compilation
- Baryon Acoustic Oscillations and Dynamical Dark Energy
- The Evolution of Inverse Power Law Quintessence at Low Redshift
- Lectures on Dark Energy and Cosmic Acceleration
- Cosmology with interaction in the dark sector
- Probing the nature of cosmic acceleration
- Hybrid dark energy
- Dynamical age of the universe as a constraint on the parametrization of dark energy equation of state
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- Dynamical dark energy confronted with multiple CMB missions
- Status on bidimensional dark energy parameterizations using SNe Ia JLA and BAO datasets
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- A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
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- Linear and non-linear perturbations in dark energy models
- The tension on the cosmological parameters from different observational data
- Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
- Reconstruction of cosmological matter perturbations in Modified Gravity
- Implications of JLA data for essence model of dark energy with given equation of state
- Testing dark energy models with data
- Modified Equations of State for Dark Energy and Observational Limitations
- Smoothing expansion rate data to reconstruct cosmological matter perturbations
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- Symmetries of F-manifolds with eventual identities and special families of connections
- Scalar field description of a parametric model of dark energy
- A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
- Probing the Dynamics of Gaussian Dark Energy Equation of State Using DESI BAO
- Bayesian deep learning for dark energy
- Exploring the deviation of cosmological constant by a generalized pressure dark energy model
- Accretion of Dark Energy Candidates Following Redshift Parametrization Type Equation of State : Horava-Lifshitz Gravity
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- Observational Constraints and Geometric Diagnostics of Barboza-Alcaniz and Logarithmic Dark Energy Parametrizations
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