The oscillating dark energy: future singularity and coincidence problem
arXiv:hep-th/0603062 · doi:10.1016/j.physletb.2006.04.026
Abstract
We consider the oscillating dark energy with periodic equation of state in two equivalent formulations: ideal fluid or scalar-tensor theory. It is shown that such dark energy suggests the natural way for the unification of early-time inflation with late-time acceleration. We demonstrate how it describes the transition from deceleration to acceleration or from non-phantom to phantom era and how it solves the coincidence problem. The occurence of finite-time future singularity for the oscillating (phantom) universe is also investigated.
LaTeX file, 9 pages, version to appear in PLB
References in corpus (21)
- Cosmological Constant - the Weight of the Vacuum
- Properties of singularities in (phantom) dark energy universe
- Quantum deSitter cosmology and phantom matter
- Cosmic Evolution in a Cyclic Universe
- Inhomogeneous Equation of State of the Universe: Phantom Era, Future Singularity and Crossing the Phantom Barrier
- The final state and thermodynamics of dark energy universe
- Unified phantom cosmology: inflation, dark energy and dark matter under the same standard
- Quantum escape of sudden future singularity
- The dS/CFT Correspondence and the Big Smash
- Phantom Field and the Fate of Universe
- Dark Energy: the equation of state description versus scalar-tensor or modified gravity
- K-Essential Phantom Energy: Doomsday around the corner?
- Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
- The Fate of Bound Systems in Phantom and Quintessence Cosmologies
- B-Inflation
- Solving the Coincidence Problem: Tracking Oscillating Energy
- Cosmological model with viscosity media (dark fluid) described by an effective equation of state
- Phantom Inflation and Primordial Perturbation Spectrum
- Nearly Scale-Invariant Spectrum of Adiabatic Fluctuations May be from a Very Slowly Expanding Phase of the Universe
- On big rip singularities
- Phantom inflation and the "Big Trip"
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- Finite-time Cosmological Singularities and the Possible Fate of the Universe
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- Non-singular Bounce Cosmology from Lagrange Multiplier Gravity
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- Cosmological Hysteresis and the Cyclic Universe
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- A FRW Dark Fluid with a Non-Linear Inhomogeneous Equation of State
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- Pre-Inflationary Spacetime in String Cosmology
- Cosmological consequences of a scalar field with oscillating equation of state: A possible solution to the fine-tuning and coincidence problems
- Will there be future deceleration? A study of particle creation mechanism in non-equilibrium thermodynamics
- Sourcing Dark Matter and Dark Energy from -attractors
- New late-time constraints on gravity
- Testing an oscillatory behavior of dark energy
- New parametrization of the dark-energy equation of state with a single parameter
- Cosmological bounds on oscillating dark energy models
- Archimedean-type force in a cosmic dark fluid: II. Qualitative and numerical study of a multistage Universe expansion
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- Crossing the phantom divide line in the Holographic dark energy model in a closed universe
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- The oscillating dark energy and cosmological Casimir effect
- The frozen vanilla model: Exploring dark sector interactions with delta effective theories
- Bayesian evidence and model selection approach for time-dependent dark energy