Phantom Field with O(N) Symmetry in Exponential Potential
arXiv:hep-th/0303093 · doi:10.1103/PhysRevD.69.107303
Abstract
In this paper, we study the phase space of phantom model with O(\emph{N}) symmetry in exponential potential. Different from the model without O(\emph{N}) symmetry, the introduction of the symmetry leads to a lower bound on the equation of state for the existence of stable phantom dominated attractor phase. The reconstruction relation between the potential of O(\textit{N}) phantom system and red shift has been derived.
5 pages, 3 figures, replaced with the version to appear on Phys. Rev. D
References in corpus (16)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Cosmological Constant - the Weight of the Vacuum
- Phantom Energy and Cosmic Doomsday
- Cosmological Results from High-z Supernovae
- Can the dark energy equation-of-state parameter w be less than -1?
- Cosmological Dynamics of Phantom Field
- Phantom cosmologies
- Constructing Phantom Cosmologies from Standard Scalar Field Universes
- Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
- Born-Infeld Quantum Condensate as Dark Energy in the Universe
- Attractor Solution of Phantom Field
- Phantom with Born-Infield type Lagrangian
- Born-Infeld-type phantom on the brane world
- Constructing dark energy models with late time de Sitter attractor
- Ghosts in a Mirror
Cited by in corpus (73)
- Properties of singularities in (phantom) dark energy universe
- The final state and thermodynamics of dark energy universe
- Dynamical systems applied to cosmology: dark energy and modified gravity
- Quantum effects can render w<-1 on cosmological scales
- Cosmological parameters from supernova observations: A critical comparison of three data sets
- Reconstructing the universe history, from inflation to acceleration, with phantom and canonical scalar fields
- The Fate of Bound Systems in Phantom and Quintessence Cosmologies
- The stability of modified gravity models
- Solar System experiments do not yet veto modified gravity models
- Cosmological expansion and local physics
- Cosmological Evolution of Hessence Dark Energy and Avoidance of the Big Rip
- Dark energy cosmology with generalized linear equation of state
- A viability criterion for modified gravity with an extra force
- Phantom Cosmologies
- Phantom-like GCG and the constraints of its parameters via cosmological dynamics
- Quintom model with O() symmetry
- The phase space view of f(R) gravity
- Phantom cosmology with general potentials
- Noether symmetry approach in phantom quintessence cosmology
- Phantom Friedmann Cosmologies and Higher-Order Characteristics of Expansion
- Curvature invariants, geodesics and the strength of singularities in Bianchi-I loop quantum cosmology
- Viscous generalized Chaplygin gas
- Modified gravity and the stability of de Sitter space
- Phantom field dynamics in loop quantum cosmology
- SO(1,1) dark energy model and the universe transition
- Exact Analysis of Scaling and Dominant Attractors Beyond the Exponential Potential
- Phase Space Analysis of Quintessence Cosmologies with a Double Exponential Potential
- Large-scale inhomogeneities in modified Chaplygin gas cosmologies
- Statefinder Diagnostic for Dilaton Dark Energy
- Dynamics of Quintessence with Thermal Interactions
- Revisiting the parametrization of Equation of State of Dark Energy via SNIa Data
- Scalar phantom energy as a cosmological dynamical system
- Aspects of Scalar Field Dynamics in Gauss-Bonnet Brane Worlds
- New "Bigs" in cosmology
- Coupled Quintessence and Phantom Based On a Dilaton
- Preventing eternality in phantom inflation
- Type I singularities and the Phantom Menace
- Torsion cosmological dynamics
- Analytical approach of late-time evolution in a torsion cosmology
- Phantom cosmologies and fermions
- Extended quintessence, inflation, and stable de Sitter spaces
- Stability analysis of an autonomous system in loop quantum cosmology
- Non-chaotic dynamics in general-relativistic and scalar-tensor cosmology
- Global behavior of cosmological dynamics with interacting Veneziano ghost
- Quasinormal modes of a black hole with quintessence-like matter and a deficit solid angle: scalar and gravitational perturbations
- Quintessence and phantom dark energy from ghost D-branes
- Alternative mechanism of avoiding the big rip or little rip for a scalar phantom field
- Scalar field cosmology in phase space
- Heteroclinic orbit and tracking attractor in cosmological model with a double exponential potential
- Dilaton Coupled Quintessence Model in the Plane
- Born-Infeld Type Phantom Model in the Plane
- Exponential Cardassian Universe
- Dark energy and supermassive black holes
- Dynamics of Quintessential Inflation
- Statefinder diagnostic in a torsion cosmology
- Global monopole surrounded by quintessence-like matter
- Galileons, phantom fields, and the fate of the Universe
- Towards realistic models with nonminimal torsion-matter coupling extension
- Cosmological dynamics of scalar fields with O(N) symmetry
- Bifurcation and Global Dynamical Behavior of the Theory
- No "big trips" for the universe
- Torsion Cosmology of Poincaré gauge theory and the constraints of its parameters via SNeIa data
- Scalar field exact solutions for non-flat FLRW cosmology: A technique from non-linear Schrödinger-type formulation
- de Sitter Gauge Theory of Gravity: An Alternative Torsion Cosmology
- Power-law expansion cosmology in Schrödinger-type formulation
- Phantom expansion with non-linear Schrödinger-type formulation of scalar field cosmology
- How Much NEC Breaking Can the Universe Endure?
- Slow-roll, acceleration, the Big Rip and WKB approximation in NLS-type formulation of scalar field cosmology
- Potentials of Coupled Quintessence Based on a Dilaton
- Action functional of the Cardassian universe
- Cosmological Dynamics of de Sitter Gravity
- Dynamics of phantom model with O(N) symmetry in loop quantum cosmology
- Viscous effect in the late time evolution of phantom universe