Slow-roll freezing quintessence
arXiv:1106.0012 · doi:10.1016/j.physletb.2011.09.034
Abstract
We examine the evolution of quintessence models with potentials satisfying (V'/V)^2<<1 and V"/V<<1, in the case where the initial field velocity is nonzero. We derive an analytic approximation for the evolution of the equation of state parameter, w, for the quintessence field. We show that such models are characterized by an initial rapid freezing phase, in which the equation of state parameter w decreases with time, followed by slow thawing evolution, for which w increases with time. These models resemble constant-V models at early times but diverge at late times. Our analytic approximation gives results in excellent agreement with exact numerical evolution.
6 pages, 5 figures, references added
References in corpus (19)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Quintom Cosmology: Theoretical implications and observations
- Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
- The Effective Theory of Quintessence: the w<-1 Side Unveiled
- Thawing quintessence with a nearly flat potential
- The cluster gas mass fraction as a cosmological probe: a revised study
- Dark energy from a quintessence (phantom) field rolling near potential minimum (maximum)
- Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
- Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
- Phantom Dark Energy Models with a Nearly Flat Potential
- The null energy condition and instability
- Quintessence reconstructed: new constraints and tracker viability
- Measuring deviations from a cosmological constant: a field-space parameterization
- Big Bang nucleosynthesis with a stiff fluid
- The Equation of State of Tracker Fields
- Parameterizing and Measuring Dark Energy Trajectories from Late-Inflatons
- Old Dark Energy
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