Parametrization of Born-Infeld Type Phantom Dark Energy Model
arXiv:0905.0935 · doi:10.1007/s10509-009-0139-y
Abstract
Applying the parametrization of dark energy density, we can construct directly independent-model potentials. In Born-Infeld type phantom dark energy model, we consider four special parametrization equation of state parameter. The evolutive behavior of dark energy density with respect to red-shift , potentials with respect to and are shown mathematically. Moreover, we investigate the effect of parameter upon the evolution of the constructed potential with respect to . These results show that the evolutive behavior of constructed Born-Infeld type dark energy model is quite different from those of the other models.
5 pages, 4 figures, Accepted for publication in Astrophysics & Space Science
References in corpus (39)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- The Cosmological Constant and Dark Energy
- Cosmological parameters from SDSS and WMAP
- Cosmological Constant - the Weight of the Vacuum
- The Case for a Positive Cosmological Lambda-term
- Cosmology and the Fate of Dilatation Symmetry
- The Cosmological Constant
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- A Model of Holographic Dark Energy
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- Kinetically Driven Quintessence
- Rolling Tachyon
- Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
- The final state and thermodynamics of dark energy universe
- Cosmological Evolution of the Rolling Tachyon
- Purely kinetic k-essence as unified dark matter
- Cosmology with tachyon field as dark energy
- Is there Supernova Evidence for Dark Energy Metamorphosis ?
- Can the clustered dark matter and the smooth dark energy arise from the same scalar field ?
- The State of the Dark Energy Equation of State
- Unified phantom cosmology: inflation, dark energy and dark matter under the same standard
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra
- Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra
- Tachyon couplings on non-BPS D-branes and Dirac-Born-Infeld action
- A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy
- Gravitational Lensing as a Probe of Quintessence
- Probing the dark side: Constraints on the dark energy equation of state from CMB, large scale structure and Type Ia supernovae
- Problems with Tachyon Inflation
- Born-Infeld Theory and Stringy Causality
- Assisted Tachyonic Inflation
- Challenges for scaling cosmologies
- Parametrization of Quintessence and Its Potential
- Parametrizations of the Dark Energy Density and Scalar Potentials
- Probing quintessence: reconstruction and parameter estimation from supernovae
- Cosmology with a Nonlinear Born-Infeld type Scalar Field
- The Evolution of Universe with th B-I Type Phantom Scalar Field
- Potentials of Coupled Quintessence Based on a Dilaton