Dynamical analysis of interacting dark energy model in the framework of particle creation mechanism

Abstract

In this work we present the cosmological dynamics of interacting dark energy models in the framework of particle creation mechanism. The particle creation mechanism presented here describes the true non equilibrium thermodynamics of the universe. In spatially flat Friedmann-Lema{\^ı}tre-Robertson-Walker universe considered here, the dissipative bulk viscous pressure is due to the non conservation of particle number. For simplicity, we assume that the creation of perfect fluid particles to be isentropic (adiabatic) and consequently the viscous pressure obeys a linear relationship with particle creation rate. Due to complicated nature of the Einstein's field equations, dynamical systems analysis has been performed to understand deeply about the cosmological dynamics. We have found some interesting cosmological scenarios like late-time evolution of universe dominated by dark energy which could mimic quintessence, cosmological constant or phantom field through a dark matter dominated era. We also obtained a possibility of crossing the phantom divide line which is favored by observations.

arXiv comment19 pages, 10 figures; version accepted for publication in Physical Review D

References in corpus (84)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Planck 2015 results. XIII. Cosmological parameters
• Planck 2013 results. XVI. Cosmological parameters
• Dynamics of dark energy
• A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
• Cosmological Constant - the Weight of the Vacuum
• The Case for a Positive Cosmological Lambda-term
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• Can the dark energy equation-of-state parameter w be less than -1?
• The phantom menaced: constraints on low-energy effective ghosts
• Scaling solutions in general non-minimal coupling theories
• Interacting quintessence solution to the coincidence problem
• Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey
• Cosmological constant and vacuum energy: old and new ideas
• Bulk Viscous Cosmology
• Dynamics of dark energy with a coupling to dark matter
• Indications of a late-time interaction in the dark sector
• Super-acceleration as Signature of Dark Sector Interaction
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Le Chatelier-Braun principle in cosmological physics
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• First evidence of running cosmic vacuum: challenging the concordance model
• Linear and nonlinear interactions in the dark sector
• Hubble expansion & Structure Formation in Time Varying Vacuum Models
• Variable Cosmological Constant as a Planck Scale Effect
• Large-scale curvature and entropy perturbations for multiple interacting fluids
• Effective equation of state for dark energy: mimicking quintessence and phantom energy through a variable Lambda
• Dark Interactions and Cosmological Fine-Tuning
• New constraints on interacting dark energy from cosmic chronometers
• Testing the Interaction between Dark Energy and Dark Matter with Planck Data
• Hints of dynamical vacuum energy in the expanding Universe
• Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
• Phase-space analysis of interacting phantom cosmology
• LXCDM: a cosmon model solution to the cosmological coincidence problem?
• Testing the running of the cosmological constant with Type Ia Supernovae at high z
• Gradient instability for w < -1
• CDM Accelerating Cosmology as an Alternative to LCDM model
• Accelerating Cold Dark Matter Cosmology (${\Omega }_{\Lambda }\equiv 0$)
• An Accelerating Cosmology Without Dark Energy
• An analytic model for interacting dark energy and its observational constraints
• Cosmological particle production, causal thermodynamics, and inflationary expansion
• Decaying Cold Dark Matter Model and Small-Scale Power
• New Cosmic Accelerating Scenario without Dark Energy
• On phenomenological models of dark energy interacting with dark matter
• Cosmological consequences of an adiabatic matter creation process
• Dynamical dark energy or variable cosmological parameters?
• "Understanding" cosmological bulk viscosity
• Is Emergent Universe a Consequence of Particle Creation Process?
• Dark energy perturbations and cosmic coincidence
• Chasing the phantom: A closer look at Type Ia supernovae and the dark energy equation of state
• Irreversible thermodynamic description of interacting dark energy - dark matter cosmological models
• Entropy evolution of universes with initial and final de Sitter eras
• Classical and quantum ghosts
• Phantom behavior via cosmological creation of particles
• Evolution and Dynamics of a Matter creation model
• Dynamics of dark energy models and centre manifolds
• Dark Energy Constraints after Planck
• A third alternative to explain recent observations: Future deceleration
• Interacting Dark Energy in f(T) cosmology : A Dynamical System analysis
• Cosmic acceleration without dark energy: Background tests and thermodynamic analysis
• A cosmographic analysis of holographic dark energy models
• Scalar-Fluid interacting dark energy: cosmological dynamics beyond the exponential potential
• Gravitationally induced adiabatic particle production: From Big Bang to de Sitter
• Effective equation of state for running vacuum: "mirage" quintessence and phantom dark energy
• A complete cosmic scenario from inflation to late time acceleration: Non-equilibrium thermodynamics in the context of particle creation
• Quintessence From The Decay of a Superheavy Dark Matter
• A new approach to the analysis of the phase space of f(R)-gravity
• Decaying Cold Dark Matter and the Evolution of the Cluster Abundance
• Cosmological dynamics of scalar fields with kinetic corrections: Beyond the exponential potential
• Is the continuous matter creation cosmology an alternative to $\Lambda$CDM?
• The Dark Side of the Universe after Planck
• Dynamical Systems analysis of an interacting dark energy model in the Brane Scenario
• Cosmological model of the interaction between dark matter and dark energy
• Will there be future deceleration? A study of particle creation mechanism in non-equilibrium thermodynamics
• Complete cosmic scenario in the Randall-Sundrum braneworld from the dynamical systems perspective
• Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld
• Exactly solved models of interacting dark matter and dark energy
• Phase space analysis for a scalar-tensor model with kinetic and Gauss-Bonnet couplings
• Formation Of Emergent Universe in Brane Scenario as a Consequence of Particle Creation
• Phase space analysis of some interacting Chaplygin gas models
• A unified cosmic evolution: Inflation to late time acceleration

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• The trace of the trace of the energy-momentum tensor-dependent Einstein's field equations
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• Phase Space Analysis and Thermodynamics of Interacting Umami Chaplygin gas in FRW Universe
• Van der Waals Universe with Adiabatic Matter Creation
• A study of interacting scalar field model from the perspective of the dynamical systems theory
• Interacting phantom dark energy: new accelerating scaling attractors
• Dynamical system analysis of logotropic dark fluid with a power law in the rest-mass energy density
• Dynamical stability of an interacting quintessence with varying-mass dark matter particles in Lyra manifold
• Stability analysis of an interacting holographic dark energy model
• Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
• Integrable Cosmological Model with van der Waals Gas and Matter Creation
• Effects of particle creation rate in two-fluid interacting cosmologies
• Interacting Dark Energy: New parametrization and observational constraints
• Dynamical systems analysis of a cosmological model with interacting Umami Chaplygin fluid in adiabatic particle creation mechanism: Some bouncing features
• Wormhole Formation with Gravitational Particle Creation Mechanism
• Matter Creation Cosmologies and Accelerated Expansion
• Correspondence between particle creation and dark components interaction in the context of $f(\mathcal{G})$ gravity
• Phase space analysis and cosmography of a two-fluid cosmological model