Generalized models of unification of dark matter and dark energy
arXiv:1208.0449 · doi:10.1103/PhysRevD.87.023510
Abstract
A model of unification of dark matter and dark energy based on the modeling of the speed of sound as a function of the parameter of the equation of state is introduced. It is found that the model in which the speed of sound depends on the power of the parameter of the equation of state, , contains the generalized Chaplygin gas models as its subclass. An effective scalar field description of the model is obtained in a parametric form which in some cases can be translated into a closed form solution for the scalar field potential. A constraint on model parameters is obtained using the observational data on the Hubble parameter at different redshifts.
arXiv commentv1: 18 pages, 6 figures; v2: 19 pages, minor changes, references added; v3: version published in PRD
References in corpus (56)
- 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
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Dynamics of dark energy
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- An alternative to quintessence
- Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
- The 3D power spectrum of galaxies from the SDSS
- Constraining Cosmological Parameters Based on Relative Galaxy Ages
- Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
- Quintom Cosmology: Theoretical implications and observations
- Purely kinetic k-essence as unified dark matter
- Can the clustered dark matter and the smooth dark energy arise from the same scalar field ?
- The end of unified dark matter?
- Uncorrelated Estimates of Dark Energy Evolution
- Extended tachyon field, Chaplygin gas and solvable k-essence cosmologies
- WMAP and the Generalized Chaplygin Gas
- Constraints on the generalized Chaplygin gas from supernovae observations
- Density perturbations in an Universe dominated by the Chaplygin gas
- Are Chaplygin gases serious contenders to the dark energy throne?
- Dust of Dark Energy
- Accelerated Universe from Modified Chaplygin Gas and Tachyonic Fluid
- Constraints on modified Chaplygin gas from recent observations and a comparison of its status with other models
- Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
- Born-Infeld Phantom Gravastars
- Gauge-invariant analysis of perturbations in Chaplygin gas unified models of dark matter and dark energy
- The dark degeneracy and interacting cosmic components
- Unified Dark Matter in Scalar Field Cosmologies
- A Particle Field Theorist's Lectures on Supersymmetric, Non-Abelian Fluid Mechanics and d-Branes
- A Note on Classical Solution of Chaplygin-gas as D-brane
- The Role of Baryons in Unified Dark Matter Models
- Constraints on the Dark Side of the Universe and Observational Hubble Parameter Data
- How the Scalar Field of Unified Dark Matter Models Can Cluster
- Affine equation of state from quintessence and k-essence fields
- Cosmological tachyon condensation
- Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach
- Nonlinear evolution of dark matter and dark energy in the Chaplygin-gas cosmology
- ISW effect in Unified Dark Matter Scalar Field Cosmologies: an analytical approach
- Unified Dark Fluid with Constant Adiabatic Sound Speed and Cosmic Constraints
- Observational constraints on a unified dark matter and dark energy model based on generalized Chaplygin gas
- Statistical techniques in cosmology
- Scalar models for the generalized Chaplygin gas and the structure formation constraints
- Matter Power Spectrum for the Generalized Chaplygin Gas Model: The Newtonian Approach
- Skewness as a test for Quartessence
- Matter power spectrum for the generalized Chaplygin gas model: The relativistic case
- Contraints on unified models for dark matter and dark energy using H(z)
- Bayesian Statistics and Parameter Constraints on the Generalized Chaplygin Gas Model using SNe Ia Data
- Measuring Unified Dark Matter with 3D Cosmic Shear
- Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
- Fitting the Supernova Type Ia Data with the Chaplygin Gas
- Transient acceleration from a hybrid Chaplygin gas
- Observational Constraints on the Generalized Chaplygin Gas
- A Modified Generalized Chaplygin Gas as the Unified Dark Matter-Dark Energy Revisited
- Reconstructing the expansion history of the Universe with a one-fluid approach
- The Power of Cosmic Flexion in Testing Modified Matter and Gravity
Cited by in corpus (7)
- Barotropic fluid compatible parametrizations of dark energy
- Modeling of accelerating Universe with bulk viscous fluid in Bianchi V space-time
- Global cosmological dynamics for the scalar field representation of the modified Chaplygin gas
- Dark sector unifications: dark matter-phantom energy, dark matter -- constant dark energy, dark matter-dark energy-dark matter
- Fate of an Accretion Disc around a Black Hole when both the Viscosity and Dark Energy is Effecting
- Transient dark energy, cosmological constant boundary crossing and dark energy data fits
- Dark matter fluid constraints from galaxy rotation curves