Dilaton Coupled Quintessence Model in the Plane
arXiv:hep-th/0610018 · doi:10.1142/S0218271807010614
Abstract
In this paper, we regard dilaton in Weyl-scaled induced gravitational theory as a coupled quintessence. Based on this consideration, we investigate the dilaton coupled quintessence(DCQ) model in plane, which is defined by the equation of state parameter for the dark energy and its derivative with respect to (the logarithm of the scale factor ). We find the scalar field equation of motion in plane, and show mathematically the property of attractor solutions which correspond to , . Finally, we find that our model is a tracking one which belongs to "freezing" type model classified in plane.
7 pages, 4 figures, some references added
References in corpus (75)
- 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
- Dynamics of dark energy
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Cosmology and the Fate of Dilatation Symmetry
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- k-Inflation
- Essentials of k-essence
- Kinetically Driven Quintessence
- Can the dark energy equation-of-state parameter w be less than -1?
- Properties of singularities in (phantom) dark energy universe
- The Cosmic Triangle: Revealing the State of the Universe
- Accelerated expansion of the universe driven by tachyonic matter
- Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
- Quantum deSitter cosmology and phantom matter
- Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
- Cosmology with a Primordial Scaling Field
- Reconstruction of a scalar-tensor theory of gravity in an accelerating universe
- Cosmological Evolution of a Quintom Model of Dark Energy
- Inhomogeneous Equation of State of the Universe: Phantom Era, Future Singularity and Crossing the Phantom Barrier
- Cosmic String Production Towards the End of Brane Inflation
- The final state and thermodynamics of dark energy universe
- Quintessence arising from exponential potentials
- Cosmological Evolution of the Rolling Tachyon
- Purely kinetic k-essence as unified dark matter
- Cosmology with tachyon field as dark energy
- The Confrontation between General Relativity and Experiment
- Cosmological Dynamics of Phantom Field
- 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
- Scalar-tensor gravity in an accelerating universe
- Modified gravity and its reconstruction from the universe expansion history
- Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
- Extended tachyon field, Chaplygin gas and solvable k-essence cosmologies
- Tachyon couplings on non-BPS D-branes and Dirac-Born-Infeld action
- Power-Law Inflation from the Rolling Tachyon
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Interacting holographic dark energy model in non-flat universe
- Assisted inflation via tachyon condensation
- Prospects and Problems of Tachyon Matter Cosmology
- Inflation from a Tachyon Fluid?
- Cosmological implications of the MAXIMA-I high resolution Cosmic Microwave Background anisotropy measurement
- Proposal for non-BPS D-brane action
- The Robustness of Quintessence
- Tracking and coupled dark energy as seen by WMAP
- Tracking K-essence
- The new form of the equation of state for dark energy fluid and accelerating universe
- Aspects of Tachyonic Inflation with Exponential Potential
- Statefinder diagnostic for coupled quintessence
- Bulk-Brane Interaction and Holographic Dark Energy
- A new view of k-essence
- Assisted Tachyonic Inflation
- Challenges for scaling cosmologies
- Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem
- Structure Formation in Inhomogeneous Dark Energy Models
- Loop Corrections to Scalar Quintessence Potentials
- Two-Field Quintom Models in the w-w' Plane
- Implementing Power Law Inflation with Tachyon Rolling on the Brane
- Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter
- On the way from matter-dominated era to dark energy universe
- Phantom Field with O(N) Symmetry in Exponential Potential
- Phantom damping of matter perturbations
- Phantom energy mediates a long-range repulsive force
- Dynamical Relaxation of Dark Energy: A Solution to Early Inflation, Late-time Acceleration and the Cosmological Constant Problem
- Cosmology with a Nonlinear Born-Infeld type Scalar Field
- Quintessence Cosmology and the Cosmic Coincidence
- The Evolution of Universe with th B-I Type Phantom Scalar Field
- Coupled Quintessence and Phantom Based On a Dilaton
- The Quintom Model of Dark Energy
- Exponential Potentials and Attractor Solution of Dilatonic Cosmology
- Dark Energy and Dilaton Cosmology
- Quantum Cosmology and Dark Energy Model of Born-Infeld Type Scalar Field
- Einstein-Brans-Dicke Cosmology
Cited by in corpus (11)
- Reconstructing the universe history, from inflation to acceleration, with phantom and canonical scalar fields
- Charged Dilatonic Black Holes in Gravity's Rainbow
- Dilatonic black holes in gravity's rainbow with a nonlinear source: the effects of thermal fluctuations
- Statefinder Diagnostic for Dilaton Dark Energy
- Cosmic Behavior, Statefinder Diagnostic and Analysis for Interacting NADE model in Non-flat Universe
- Statefinder diagnostic and analysis for interacting polytropic gas dark energy model
- Dilatonic Equation of Hydrostatic Equilibrium and Neutron Star Structure
- Thermodynamic topology of topological charged dilatonic black holes
- An effective quintessence field with a power-law potential
- Exploring the new Tsallis agegraphic dark energy with interaction through statefinder
- Diagnostic for Dilaton Dark Energy