Cosmological Evolution of Interacting Phantom Energy with Dark Matter

Abstract

We investigate the cosmological evolution of an interacting phantom energy model in which the phantom field has interaction with the dark matter. We discuss the existence and stability of scaling solutions for two types of specific interactions. One is motivated by the conformal transformation in string theory and the other is motivated by analogy with dissipation. In the former case, there exist no scaling solutions. In the latter case, there exist stable scaling solutions, which may give a phenomenological solution of the coincidence problem. Furthermore, the universe either accelerates forever or ends with a singularity, which is determined by not only the model parameters but also the initial velocity of the phantom field.

7 pages, 11 figures, RevTeX

References in corpus (42)

• 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
• Exponential potentials and cosmological scaling 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
• Cosmological Evolution of a Quintom Model of Dark Energy
• Scaling solutions in general non-minimal coupling theories
• Interacting Quintessence
• Interacting quintessence solution to the coincidence problem
• Cosmological Dynamics of Phantom Field
• Quantum effects can render w<-1 on cosmological scales
• The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
• Dilatonic ghost condensate as dark energy
• Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
• Phantom cosmologies
• Phantom Field and the Fate of Universe
• Nuclear Reaction Network for Primordial Nucleosynthesis: a detailed analysis of rates, uncertainties and light nuclei yields
• You need not be afraid of phantom energy
• deSitter brane universeinduced by phantom and quantum effects
• Interactions in Scalar Field Cosmology
• Quintessence, super-quintessence and observable quantities in Brans-Dicke and non-minimally coupled theories
• A unified approach to scaling solutions in a general cosmological background
• Relic Dark energy from Trans-Planckian Regime
• Hyperbolic Space Cosmologies
• Nearly Scale-Invariant Spectrum of Adiabatic Fluctuations May be from a Very Slowly Expanding Phase of the Universe
• Phantom Cosmologies
• Interacting Phantom Energy
• The Tensor to Scalar Ratio of Phantom Dark Energy Models
• Phantom k-essence cosmologies
• Attractor Behavior of Phantom Cosmology
• Phantom Dark Energy, Cosmic Doomsday, and the Coincidence Problem
• Cosmological Scaling Solutions and Multiple Exponential Potentials
• SO(1,1) dark energy model and the universe transition
• Cosmological Scaling Solutions and Cross-coupling Exponential Potential
• Cosmological Scaling Solutions of Multiple Tachyon Fields with Inverse Square Potentials
• Inflationary Cosmologies from Compactification?
• Partial rip scenario - a cosmology with a growing cosmological term

Cited by in corpus (97)

• Holographic dark energy and cosmic coincidence
• Dynamical systems applied to cosmology: dark energy and modified gravity
• Probing the Coupling between Dark Components of the Universe
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• The new form of the equation of state for dark energy fluid and accelerating universe
• Thermodynamics of dark energy interacting with dark matter and radiation
• Cosmological Evolution of Hessence Dark Energy and Avoidance of the Big Rip
• Interacting Agegraphic Dark Energy
• Cosmological coincidence problem in interacting dark energy models
• 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
• Interacting holographic dark energy
• Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
• Phase-space analysis of interacting phantom cosmology
• Galactic Dark Matter in the Phantom Field
• Interacting Chaplygin gas
• Dynamics of Teleparallel Dark Energy
• Observational $H(z)$ Data and Cosmological Models
• Dynamical Systems Perspective of Cosmological Finite-time Singularities in $f(R)$ Gravity and Interacting Multifluid Cosmology
• Probing the curvature and dark energy
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Cosmological Constraints on the Sign-Changeable Interactions
• Phantom evolution in power-law potentials
• Bouncing cosmologies with dark matter and dark energy
• Entropy-Corrected Holographic Dark Energy
• Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector
• Critical comments on the paper "Crossing $\omega =-1$ by a single scalar field on a Dvali-Gabadadze-Porrati brane" by H Zhang and Z-H Zhu [Phys.Rev.D75,023510(2007)]
• Crossing $w=-1$ by a single scalar on a Dvali-Gabadadze-Porrati brane
• Spinor Dark Energy and Cosmological Coincidence Problem
• Testing models of vacuum energy interacting with cold dark matter
• Dual interacting cosmologies and late accelerated expansion
• The State Equation of the Yang-Mills field Dark Energy Models
• Dynamics of interacting phantom scalar field dark energy in Loop Quantum Cosmology
• Interacting Phantom Energy and Avoidance of the Big Rip Singularity
• Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem
• In search of the dark matter dark energy interaction: a kinematic approach
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Exact Analysis of Scaling and Dominant Attractors Beyond the Exponential Potential
• A Quintom scenario with mixed kinetic terms
• Cosmological evolution of interacting phantom (quintessence) model in Loop Quantum Gravity
• Particle vs. future event horizon in interacting holographic dark energy model
• Cheng-Weyl Vector Field and its Cosmological Application
• Transient cosmic acceleration from interacting fluids
• Interacting Energy Components and Observational $H(z)$ Data
• A Note on Gravitational Baryogenesis
• Coupled dark energy: a dynamical analysis with complex scalar field
• Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
• Exact models with non-minimal interaction between dark matter and (either phantom or quintessence) dark energy
• A Study of Finite-time Singularities of Loop Quantum Cosmology Interacting Multifluids
• Statefinder Parameters for Interacting Phantom Energy with Dark Matter
• Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
• Chaotic universe model: Lotka-Volterra dynamics of the universe evolution
• Dynamical analysis for a vector-like dark energy
• Metastable dark energy
• Non-adiabatic perturbations in decaying vacuum cosmology
• Absence of the Fifth Force Problem in a Model with Spontaneously Broken Dilatation Symmetry
• Dark Energy Interacting with Dark Matter in Classical Einstein and Loop Quantum Cosmology
• Cosmological model of the interaction between dark matter and dark energy
• Statefinder parameters in two dark energy models
• Extended Phase Space Analysis of Interacting Dark Energy Models in Loop Quantum Cosmology
• The Classical and Loop Quantum Cosmology Phase Space of Interacting Dark Energy and Superfluid Dark Matter
• Fractional dark energy
• Searching for a matter bounce cosmology with low redshift observations
• Quintom evolution in power-law potentials
• A note on interacting holographic dark energy with a Hubble-scale cutoff
• A single model of interacting dark energy: generalized phantom energy or generalized Chaplygin gas
• Cosmological perturbations and dynamical analysis for interacting quintessence
• Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2
• A New Type of Dark Energy Model
• Latest data constraint of some parameterized dark energy models
• A Two-field Dilaton Model of Dark Energy
• Generalized Logarithmic Equation of State in Classical and Loop Quantum Cosmology Dark Energy-Dark Matter Coupled Systems
• Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld
• QCD ghost dark energy cannot (even roughly) explain the main features of the accepted cosmological paradigm
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• Expanding Universe: slowdown or speedup?
• Cosmological Evolution of Einstein-Aether Models with Power-law-like Potential
• Interacting holographic dark energy models: A general approach
• Noether Symmetry Approach for Dirac-Born-Infeld Cosmology
• Interacting dark energy in the dark $SU(2{)}_R$ model
• Statefinder Diagnostic for Phantom Model with $V(\varphi )=V_0\exp (-\lambda {\varphi }^2)$
• Interacting dark sector: a dynamical system perspective
• Interacting phantom dark energy: new accelerating scaling attractors
• Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
• Interacting agegraphic dark energy models in phase space
• The accelerated scaling attractor solution of the interacting agegraphic dark energy in Brans-Dicke theory
• Cosmology In Terms Of The Deceleration Parameter. Part II
• Generalized second law of thermodynamics in presence of interacting tachyonic field and scalar(phantom)field
• Late-time-accelerated expansion arisen from gauge fields in an anisotropic background and a fruitful trick for Noether's approach
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Dynamics of two-scalar-field cosmological models beyond the exponential potential
• Dynamical evolution of quintessence cosmology in a physical phase space
• Agegraphic dark energy with the sign-changeable interaction in non-flat universe
• Phantom cosmology with arbitrary potential: New accelerating scaling attractors
• Late time attractors of some varying Chaplygin gas cosmological models
• Viscous effect in the late time evolution of phantom universe