Interacting Phantom Energy
arXiv:astro-ph/0411524 · doi:10.1103/PhysRevD.71.023501
Abstract
We investigate the role of a suitable interaction between a matter fluid and a phantom field for the coincidence problem. There exists a stationary scaling solution which is a stable attractor at late times. Furthermore, the cosmic doomsday is avoided in one region of the parameter space.
5 pages, 5 figures, RevTeX
References in corpus (33)
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Cosmology and the Fate of Dilatation Symmetry
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- Phantom Energy and Cosmic Doomsday
- Cosmological Tracking Solutions
- Kinetically Driven Quintessence
- Can the dark energy equation-of-state parameter w be less than -1?
- Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
- Quantum deSitter cosmology and phantom matter
- Interacting Quintessence
- Interacting quintessence solution to the coincidence problem
- Cosmological Dynamics of Phantom Field
- Is there Supernova Evidence for Dark Energy Metamorphosis ?
- The case for dynamical dark energy revisited
- Dilatonic ghost condensate as dark energy
- Phantom cosmologies
- Phantom Field and the Fate of Universe
- Mirage Cosmology
- K-Essential Phantom Energy: Doomsday around the corner?
- deSitter brane universeinduced by phantom and quantum effects
- Quintessence, super-quintessence and observable quantities in Brans-Dicke and non-minimally coupled theories
- Phantom Inflation and Primordial Perturbation Spectrum
- Relic Dark energy from Trans-Planckian Regime
- Loop Corrections to Scalar Quintessence Potentials
- Nearly Scale-Invariant Spectrum of Adiabatic Fluctuations May be from a Very Slowly Expanding Phase of the Universe
- Phantom Cosmologies
- The Tensor to Scalar Ratio of Phantom Dark Energy Models
- Thermodynamics, Spectral Distribution and the Nature of Dark Energy
- Phantom k-essence cosmologies
- On big rip singularities
- How to Test Stringy Dark Energy?
- Attractor Behavior of Phantom Cosmology
- Modified Dispersion Relations from Closed Strings in Toroidal Cosmology
Cited by in corpus (85)
- Properties of singularities in (phantom) dark energy universe
- Holographic dark energy and cosmic coincidence
- Phantom energy traversable wormholes
- Probing the Coupling between Dark Components of the Universe
- The new form of the equation of state for dark energy fluid and accelerating universe
- Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
- Coupled dark energy: Towards a general description of the dynamics
- Thermodynamics of dark energy interacting with dark matter and radiation
- Crossing of the w=-1 Barrier by D3-brane Dark Energy Model
- Two Loop Scalar Self-Mass during Inflation
- Crossing w=-1 in Gauss-Bonnet Brane World with Induced Gravity
- Interacting Agegraphic Dark Energy
- Cosmological Evolution of Interacting Phantom Energy with Dark Matter
- Interacting Vector-like Dark Energy, the First and Second Cosmological Coincidence Problems
- Statefinder Diagnostic and w-w' Analysis for the Agegraphic Dark Energy Models without and with Interaction
- Phase-space analysis of interacting phantom cosmology
- Charged Black Holes in Phantom Cosmology
- Interacting Chaplygin gas
- A Tracker Solution for a Holographic Dark Energy Model
- Observational Data and Cosmological Models
- Interacting Dark Energy and Cosmological Equations of State
- Exactly Solvable SFT Inspired Phantom Model
- Phantom Friedmann Cosmologies and Higher-Order Characteristics of Expansion
- Entropy-Corrected Holographic Dark Energy
- Critical comments on the paper "Crossing by a single scalar field on a Dvali-Gabadadze-Porrati brane" by H Zhang and Z-H Zhu [Phys.Rev.D75,023510(2007)]
- Crossing by a single scalar on a Dvali-Gabadadze-Porrati brane
- K-Chameleon and the Coincidence Problem
- Dual interacting cosmologies and late accelerated expansion
- The State Equation of the Yang-Mills field Dark Energy Models
- Interacting Phantom Energy and Avoidance of the Big Rip Singularity
- Constraints on coupling constant between dark energy and dark matter
- Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem
- Testing the phenomenological interacting dark energy with observational data
- Cosmological evolution of interacting phantom (quintessence) model in Loop Quantum Gravity
- Cheng-Weyl Vector Field and its Cosmological Application
- Interacting Energy Components and Observational Data
- Interacting modified Chaplygin gas in loop quantum cosmology
- Coupled dark energy: a dynamical analysis with complex scalar field
- Dynamics of coupled phantom and tachyon fields
- Some remarks about non-minimally coupled scalar field models
- Exact models with non-minimal interaction between dark matter and (either phantom or quintessence) dark energy
- The Cosmic Coincidence as a Temporal Selection Effect Produced by the Age Distribution of Terrestrial Planets in the Universe
- Statefinder Parameters for Interacting Phantom Energy with Dark Matter
- Dynamical analysis for a vector-like dark energy
- Observational constraints on generalized Chaplygin gas model
- Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
- Natural Phantom Dark Energy, Wiggling Hubble Parameter and Direct Data
- Metastable dark energy
- Interacting cosmic fluids in power-law Friedmann-Robertson-Walker cosmological models
- Dark-Energy Dynamics Required to Solve the Cosmic Coincidence
- Fractional dark energy
- Interacting fluids generating identical, dual and phantom cosmologies
- Interacting closed string tachyon with modified Chaplygin gas and its stability
- Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
- A new holographic dark energy model in Brans-Dicke theory with logarithmic scalar field
- A note on interacting holographic dark energy with a Hubble-scale cutoff
- Testing the interaction model with cosmological data and gamma-ray bursts
- Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
- Cosmological perturbations and dynamical analysis for interacting quintessence
- A New Type of Dark Energy Model
- Latest data constraint of some parameterized dark energy models
- On sign-changeable interaction in FLRW cosmology
- Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld
- Time-averaging axion-like interacting scalar fields models
- Dynamical system analysis of Dirac-Born-Infeld scalar field cosmology in coincident gravity
- Constraints on interacting dark energy revisited: implications for the Hubble tension
- Interacting dark energy in the dark model
- Statefinder Diagnostic for Phantom Model with
- Stability analysis in Modified Non-Local Gravity
- Form invariant transformations between n-- and m-- dimensional flat Friedmann--Robertson--Walker cosmologies
- Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
- Interacting warm dark matter
- Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
- Braneworld cosmology in the sourced-Taub background
- Semi-Holographic Universe
- Hybrid Chaplygin gas and phantom divide crossing
- Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
- Interacting Kasner-type cosmologies
- Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
- Asymptotic Estimation for Eigenvalues in the Exponential Potential and for Zeros of with Respect to Order
- Inconsistences in Interacting Agegraphic Dark Energy Models
- A Thousand Problems in Cosmology: Interaction in the Dark Sector
- Generalized Semi-Holographic Universe
- Viscous effect in the late time evolution of phantom universe
- Reconstruction of a dark energy model for the Dirac-Born-Infeld scalar field with the Hubble and DESI data via Gaussian process