Quantum deSitter cosmology and phantom matter

Abstract

We consider deSitter universe and Nariai universe induced by quantum CFT with classical phantom matter and perfect fluid. The model represents the combination of trace-anomaly driven inflation and phantom driven deSitter universe. The similarity of phantom matter with quantum CFT indicates that phantom scalar may be the effective description for some quantum field theory. It is demonstrated that it is easier to achieve the acceleration of the scale factor preserving the energy conditions in such unified model. Some properties of unified theory (anti-gravitating solutions, negative ADM mass Nariai solution, relation with steady state) are briefly mentioned.

LaTeX file 12 pages, version to appear in PLB

Cited by in corpus (603)

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• Future state of the Universe
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• Interaction between modified Chaplygin gas and ghost dark energy in presence of extra dimensions
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• Observational constraints on the braneworld model with brane-bulk energy exchange
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• A Finite Quantum Gravity Field Theory Model
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• Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology
• Interacting new agegraphic Phantom model of dark energy in non-flat universe
• Quintom potentials from quantum cosmology using the FRW cosmological model
• Rip Brane Cosmology from 4d Inhomogeneous Dark Fluid Universe
• Cosmic acceleration from coupling of baryonic and dark matter components: Analysis and diagnostics
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Weyl Anomaly and Initial Singularity Crossing
• Parametrizing the transition to the phantom epoch with Supernovae Ia and Standard Rulers
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• Interacting phantom dark energy: new accelerating scaling attractors
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• The universe dynamics in the tachyon cosmology with non-minimal coupling to matter
• No "big trips" for the universe
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• Tachyon model of Tsallis holographic dark energy
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• Wave dynamics of phantom scalar perturbation in the background of Schwarzschild black hole
• Polytropic gas scalar field models of dark energy
• Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory
• Phantom fields: bounce solutions in the early Universe and S-branes
• Testing gravity of a regular and slowly rotating phantom black hole by quasi-periodic oscillations
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• First-order formalism for the quintom model of dark energy
• Self-accelerating solutions of scalar-tensor gravity
• Interacting agegraphic dark energy models in phase space
• Remarks on generalized scalar-tensor models of dark energy
• Extension of non-minimal derivative coupling theory and Hawking radiation in black-hole spacetime
• The Quantum State Of The Universe From Deformation Quantization and Classical-Quantum Correlation
• LRS Bianchi I model with constant deceleration parameter
• The accelerated scaling attractor solution of the interacting agegraphic dark energy in Brans-Dicke theory
• A Universe with a generalized ghost dark energy and Van der Waals fluid interacting with a fluid
• Knot Universes in Bianchi Type I Cosmology
• Comments on Scalar-Tensor Representation of $f(R)$ Theories
• Scalar field exact solutions for non-flat FLRW cosmology: A technique from non-linear Schrödinger-type formulation
• Black hole solutions in modified gravity induced by quantum metric fluctuations
• Scalar-tensor black holes in an expanding universe
• Ghost dark energy with sign-changeable interaction term
• Effects of anisotropy on interacting ghost dark energy in Brans-Dicke theories
• Renormalizable toy model of massive spin two field and new bigravity
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• Braneworld cosmology in the sourced-Taub background
• Non-minimal coupling of the phantom field and cosmic acceleration
• Are we seeing the beginnings of Inflation?
• Universal procedure to cure future singularities of dark energy models
• Quantum induced w = -1 crossing of the quintessence and phantom models
• Stability analysis of agegraphic dark energy in Brans-Dicke cosmology
• Reconstruction of the equation of state for the cyclic universes in homogeneous and isotropic cosmology
• Cosmology In Terms Of The Deceleration Parameter. Part II
• Turbulence Accelerating Cosmology from an Inhomogeneous Dark Fluid
• Thermodynamics in Kaluza-Klein Universe
• Phantom shell around black hole and global geometry
• Deformation of the quintom cosmological model and its consequences
• Late-time-accelerated expansion arisen from gauge fields in an anisotropic background and a fruitful trick for Noether's approach
• Reconstructing FHDE with Scalar and Gauge Fields
• Anisotropic Born-Infeld-f(R) Cosmologies
• Dark Energy and Cosmological Horizon Thermal Effects
• Cosmology with higher-derivative matter fields
• Dynamical evolution of phantom scalar perturbation in the background of Schwarzschild black String spacetime
• Thermodynamical description of modified generalized Chaplygin gas model of dark energy
• Cosmological observations in non-local $F(R)$ cosmology
• Evolutionary quantum cosmology in a gauge-fixed picture
• Anisotropic Dark Energy and the Generalized Second Law of Thermodynamics
• The Strong Energy Condition and the S-Brane Singularity Problem
• De Sitter cosmology from Gauss-Bonnet dark energy with quantum effects
• On Friedmann-Lema\^ıtre-Robertson-Walker cosmologies in non-standard gravity
• Power-law expansion cosmology in Schrödinger-type formulation
• Symmetry operators and separation of variables in the $(2+1)$-dimensional Dirac equation with external electromagnetic field
• Tachyon fields with effects of quantum matter in an Anti-de Sitter Universe
• Phantom Divide Crossing with General Non-minimal Kinetic Coupling
• Interacting Three Fluid System and Thermodynamics of the Universe Bounded by the Event Horizon
• Quantum Entropy-Driven Modifications to Holographic Dark Energy in $f(G,T)$ Gravity
• Observational constraints on G-corrected holographic dark energy using a Markov chain Monte Carlo method
• A cosmological model of the early universe based on ECG with variable $\Lambda$-term in Lyra geometry
• Pre-big bang collapsing universe from modern Kaluza-Klein theory of gravity
• Friedmann-Robertson-Walker Models with Late-Time Acceleration
• Phantom cosmology with a decaying cosmological function $\Lambda (t)$ induced from five-dimensional (5D) geometrical vacuum
• The linearization method and new classes of exact solutions in cosmology
• New holographic Chaplygin gas model of dark energy
• Cosmological implications of Born-Infeld-$f(R)$ gravity
• Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
• Interacting Viscous Dark Energy in Bianchi Type-III Universe
• Statefinder Diagnostic for Dark Energy Models in Bianchi I Universe
• The torsion cosmology in Kaluza-Klein theory
• Brane cosmology from observational surveys and its comparison with standard FRW cosmology
• Phantom expansion with non-linear Schrödinger-type formulation of scalar field cosmology
• Evolution of Dark Energy Perturbations for Slotheon Field and Power Spectrum
• Variable $G$ Correction for Dark Energy Model in Higher Dimensional Cosmology
• Exploring the deviation of cosmological constant by a generalized pressure dark energy model
• The Friedmann equations in deformed Hořava-Lifshitz gravity and Debye model
• Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
• Slow-roll, acceleration, the Big Rip and WKB approximation in NLS-type formulation of scalar field cosmology
• Analytical considerations about the cosmological constant and dark energy
• A class of regular bouncing cosmologies
• D-bound and Bekenstein bound for McVittie solution surrounded by dark energy cosmological fields
• Observational Constraints on Phantom Crossing DGP Gravity
• Hawking radiation and thermodynamics of dynamical black holes in phantom dominated universe
• On a class of scaling FRW cosmological models
• Cosmological Evolution of Viscous Dark Energy in f(Q,C) Gravity: Two-Fluid Approach
• Probing Dark Energy Properties in $fQ,C)$ Gravity with FLRW Cosmological Models
• On the necessity of phantom fields for solving the horizon problem in scalar cosmologies
• Singular behavior of the dark universe under the effect of thermal radiation in curved spacetime
• Asymptotic solutions in f(R)-gravity
• G-corrected holographic dark energy model
• $f(T)$ gravity from holographic Ricci dark energy model with new boundary conditions
• Potentials of Coupled Quintessence Based on a Dilaton
• Accelerating cosmology in modified gravity with scalar field
• Phantom scalar emission in the Kerr black hole spacetime
• A Thermodynamic Model for Dark Energy Including Particle Creation or Destruction Processes
• Qualitative behaviour of higher-curvature gravity with boundary terms i.e the f(Q) gravity models by dynamical system analysis
• Evolution of perturbations in the model of Tsallis holographic dark energy
• Nonlinear evolution of anisotropic matter configurations under higher-order curvature corrections
• Viscous coupled fluids in terms of a log-corrected equation of state
• Morris-Thorne Wormhole in the Vector-Tensor theories with Abelian gauge symmetry breaking
• Phantom BTZ black holes
• Cosmological singularities in non-canonical models of dark energy
• Behavior of $F(R)$ gravity around a crossing of the phantom divide
• Holographic bounce cosmological models induced by viscous dark fluid from a generalized non-singular entropy function
• $f(R)$ gravity in the solar system and cosmological scalarons
• Observational constraints on thawing quintessence scalar field model
• Phase space analysis of a FRW cosmology in the Maxwell$-$Cattaneo approach
• Revisiting Holographic Dark Energy in Cyclic Cosmology
• Reconstructing cosmic evolution with a density parametrization
• The presence of a Phantom field in a Randall-Sundrum scenario
• The role of potential in the ghost-condensate dark energy model
• Dark energy from conformal symmetry breaking
• Neutrino Interactions with perturbed Rastall Gravity: A Novel Approach to Reducing the Hubble Tension
• Coupled fluids model in FRW space-time
• Holographic F(Q,T) Gravity with Lambert Solution
• Brane World Dynamics and Adiabatic Matter creation
• Isotropic turbulence in the dark fluid universe with inhomogeneous equation of state
• A Heuristic Approach to the Far-Future State of a Universe Dominated by Phantom Energy
• Revisiting Barrow's Graduated Inflationary Universe: A Warm perspective
• Evolution of the horizons for dark energy universe
• Acceleration of the universe in matter dominant era by conformal symmetry breaking
• Spacetime Instability and Quantum Gravity as Low Energy Effective Field Theory
• Generic autonomous system approach to interacting dark energy models
• Inflation and Linear Expansion in the Radiation Dominated era in Jordan-Brans-Dicke Cosmology
• A new approach to modified-gravity models
• Hyperbolic symmetries, inflaton-phantom cosmology, and inflation
• Gravity and induced matter on Nearly Kahler Manifolds
• Confronting phantom inflation with Planck data
• A new topological perspective of expanding space-times with applications to cosmology
• Cosmological models with Big rip and Pseudo rip Scenarios in extended theory of gravity
• Dynamics of Linear Scalar Perturbation in f(Q)+f(T) class of f(Q,T) gravity
• Singularity softening and avoidance by the action of thermal radiation in a generalized entropic cosmology
• Quantum Quintom Cosmology
• Matter loops corrected modified gravity in Palatini formulation
• The relation between Geometry and Matter in classical and quantum Gravity and Cosmology
• Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology