Interacting Quintessence

Abstract

We demonstrate that a suitable coupling between a quintessence scalar field and a pressureless cold dark matter (CDM) fluid leads to a constant ratio of the energy densities of both components which is compatible with an accelerated expansion of the Universe.

12 pages, LaTeX; new material on the stability analysis and on the interaction potential added, reference list enlarged and updated; to be published in PLB

References in corpus (6)

• Cosmology and the Fate of Dilatation Symmetry
• Stationary dark energy: the present universe as a global attractor
• Cosmic acceleration without quintessence
• A Quintessence Scalar Field in Brans-Dicke Theory
• Quintessence dissipative superattractor cosmology
• Testing Cosmic Acceleration with Type Ia Supernovae

Cited by in corpus (455)

• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Properties of singularities in (phantom) dark energy universe
• Beyond the Cosmological Standard Model
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Dark Energy
• Inhomogeneous Equation of State of the Universe: Phantom Era, Future Singularity and Crossing the Phantom Barrier
• Holographic dark energy and cosmic coincidence
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Interacting quintessence solution to the coincidence problem
• Dynamical systems applied to cosmology: dark energy and modified gravity
• Holographic Dark Energy
• Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
• Large-scale instability in interacting dark energy and dark matter fluids
• Probing the Coupling between Dark Components of the Universe
• Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
• Dynamics of dark energy with a coupling to dark matter
• Aspects of the cosmological "coincidence problem"
• Constraints on the interacting holographic dark energy model
• Dynamics of interacting dark energy
• 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
• Cosmologies with Energy Exchange
• Coupled dark energy: Towards a general description of the dynamics
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Le Chatelier-Braun principle in cosmological physics
• Theoretical Models of Dark Energy
• Interacting dark energy, holographic principle and coincidence problem
• Observational constraints on interacting quintessence models
• Linear and nonlinear interactions in the dark sector
• Equation of state for an interacting holographic dark energy model
• Hubble expansion & Structure Formation in Time Varying Vacuum Models
• Observational constraints on an interacting dark energy model
• Stability of the curvature perturbation in dark sectors' mutual interacting models
• Interacting Dark Energy -- constraints and degeneracies
• Dark Interactions and Cosmological Fine-Tuning
• Statefinder parameters for interacting dark energy
• Cosmological Evolution of Hessence Dark Energy and Avoidance of the Big Rip
• Interacting Agegraphic Dark Energy
• Acceleration at z>1?
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Scaling Cosmology
• Models of coupled dark matter to dark energy
• Stationary dark energy with a baryon-dominated era: solving the coincidence problem with a linear coupling
• Cosmological coincidence problem in interacting dark energy models
• Cosmological Evolution of Interacting Phantom Energy with Dark Matter
• Interacting Vector-like Dark Energy, the First and Second Cosmological Coincidence Problems
• Growth of perturbations in dark matter coupled with quintessence
• Interacting models may be key to solve the cosmic coincidence problem
• Statefinder Diagnostic and w-w' Analysis for the Agegraphic Dark Energy Models without and with Interaction
• Entropic cosmology for a generalized black-hole entropy
• Toward a solution of the coincidence problem
• Matter density perturbations in interacting quintessence models
• Interacting holographic dark energy
• Interacting holographic dark energy in Brans-Dicke theory
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• The Growth of Structure in Interacting Dark Energy Models
• Interacting Chaplygin gas
• Dynamics of Teleparallel Dark Energy
• Interacting Phantom Energy
• LXCDM: a cosmon model solution to the cosmological coincidence problem?
• Observational constraints on the dark energy and dark matter mutual coupling
• Cosmology with a Variable Chaplygin Gas
• A Tracker Solution for a Holographic Dark Energy Model
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Observational $H(z)$ Data and Cosmological Models
• Generalized hybrid metric-Palatini gravity
• Interacting Dark Energy and Cosmological Equations of State
• The Parameterized Post-Friedmannian Framework for Interacting Dark Energy Theories
• Coupled dark matter-dark energy in light of near Universe observations
• Adiabatic initial conditions for perturbations in interacting dark energy models
• Interacting agegraphic dark energy models in non-flat universe
• Dynamics of Quintessence Models of Dark Energy with Exponential Coupling to the Dark Matter
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• Interacting models of soft coincidence
• An analytic model for interacting dark energy and its observational constraints
• A new interacting two fluid model and its consequences
• On the Dark Sector Interactions
• Selected topics in scalar-tensor theories and beyond
• The Cosmological Constant Problem and Running Vacuum in the Expanding Universe
• Generalized Second Law of Thermodynamics in $f(T)$ Gravity with Entropy Corrections
• On holographic dark-energy models
• Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension
• Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
• Curvature force and dark energy
• Dynamics of Interacting Quintessence Models: Observational Constraints
• Effects of dark sectors' mutual interaction on the growth of structures
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• Evolution of the universe in entropic cosmologies via different formulations
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• A Field Theory Model for Dark Matter and Dark Energy in Interaction
• Interacting Ghost Dark Energy in Non-Flat Universe
• Arbitrary scalar field and quintessence cosmological models
• Dynamics of interacting dark energy model in Einstein and Loop Quantum Cosmology
• Power-Law Entropy Corrected Holographic Dark Energy Model
• Cosmological Constraints on the Sign-Changeable Interactions
• Current constraints on interacting holographic dark energy
• Dark Coupling and Gauge Invariance
• Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector
• Testing coupled dark energy with large scale structure observation
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• Quintessence Model With Double Exponential Potential
• A model with interaction of dark components and recent observational data
• Dark energy perturbations and cosmic coincidence
• K-Chameleon and the Coincidence Problem
• Spinor Dark Energy and Cosmological Coincidence Problem
• Observational constraints on holographic tachyonic dark energy in interaction with dark matter
• Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
• Scattering of Dark Matter and Dark Energy
• Observational constraints on Rastall's cosmology
• Irreversible thermodynamic description of interacting dark energy - dark matter cosmological models
• Cosmological dynamics with non-linear interactions
• The State Equation of the Yang-Mills field Dark Energy Models
• Cosmological constraints on parametrized interacting dark energy
• Phase Space Analysis of the Accelerating Multi-fluid Universe
• Dynamics of interacting quintessence
• Holographic dark energy from minimal supergravity
• Interacting Phantom Energy and Avoidance of the Big Rip Singularity
• Ricci-Gauss-Bonnet holographic dark energy
• Dynamics of dark energy models and centre manifolds
• Quintessence with quadratic coupling to dark matter
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Dark Energy in Practice
• Looking for interactions in the cosmological dark sector
• Interacting new agegraphic dark energy in non-flat Brans-Dicke cosmology
• Kinetic k-essence ghost dark energy model
• Observational constraints on a logarithmic scalar field dark energy model and black hole mass evolution in the Universe
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Scalar-field dark energy nonminimally and kinetically coupled to dark matter
• Can Dark Matter Decay in Dark Energy?
• Coupled dark energy with perturbed Hubble expansion rate
• Super-acceleration on the Brane by Energy Flow from the Bulk
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• An evaluation of cosmological models from expansion and growth of structure measurements
• Cosmological consequences of a possible $\Lambda$-dark matter interaction
• The universe dominated by the extended Chaplygin gas
• AIC and BIC for cosmological interacting scenarios
• The accelerating universe in brane-world cosmology
• Cosmological constraints on coupled dark energy
• Non-adiabatic-like accelerated expansion of the late universe in entropic cosmology
• Dark energy, matter creation and curvature
• Cosmological model with interactions in the dark sector
• Late Universe expansion dominated by domain walls and dissipative dark matter
• Attractor solutions for general hessence dark energy
• Particle vs. future event horizon in interacting holographic dark energy model
• Cosmological evolution of interacting phantom (quintessence) model in Loop Quantum Gravity
• Scalar field description of decaying-$\Lambda$ cosmologies
• How to Distinguish Dark Energy and Modified Gravity?
• Interacting Ricci Dark Energy with Logarithmic Correction
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
• Cheng-Weyl Vector Field and its Cosmological Application
• Transient cosmic acceleration from interacting fluids
• Holographic dark energy in Brans-Dicke theory with log correction
• New coupled quintessence cosmology
• Scalar-Fluid interacting dark energy: cosmological dynamics beyond the exponential potential
• Interacting Energy Components and Observational $H(z)$ Data
• Interacting entropy-corrected new agegraphic dark energy in Brans-Dicke cosmology
• Quasi-local variables in spherical symmetry: numerical applications to dark matter and dark energy sources
• Cosmic accelerated expansion and the entropy corrected holographic dark energy
• CMB constraints on interacting cosmological models
• Tachyon Reconstruction of Ghost Dark Energy
• Viscous dark energy and generalized second law of thermodynamics
• $\Lambda (t)$ cosmology induced by a slowly varying Elko field
• Dark energy: investigation and modeling
• Chaplygin gas with non-adiabatic pressure perturbations
• Anisotropic brane gravity with a confining potential
• A Note on Gravitational Baryogenesis
• A new approach on the stability analysis in ELKO cosmology
• Scaling solutions and weak gravity in dark energy with energy and momentum couplings
• Probing the imprints of generalized interacting dark energy on the growth of perturbations
• The spherical collapse model in time varying vacuum cosmologies
• Entropic cosmology in a dissipative universe
• Interacting Cosmological Fluids and the Coincidence Problem
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Coupled dark energy: a dynamical analysis with complex scalar field
• Cosmological implications and structure formation from a time varying vacuum
• Cosmological Perturbations in Models of Coupled Dark Energy
• Dynamics of coupled phantom and tachyon fields
• Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
• Thermodynamics of interacting entropy-corrected holographic dark energy in a non-flat FRW universe
• Towards testing interacting cosmology by distant type Ia supernovae
• Are $H_0$ and ${\sigma }_8$ tensions generic to present cosmological data?
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• Reconstructing the interaction rate in holographic models of dark energy
• Exact models with non-minimal interaction between dark matter and (either phantom or quintessence) dark energy
• Quintessence From The Decay of a Superheavy Dark Matter
• Current and future supernova constraints on decaying $\Lambda$ cosmologies
• Interacting viscous dark fluids
• Interacting new agegraphic viscous dark energy with varying $G$
• Composite dark energy: cosmon models with running cosmological term and gravitational coupling
• J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
• Dynamical Evolution of Interacting Modified Chaplygin Gas
• Dark energy with a gradient coupling to the dark matter fluid: cosmological dynamics and structure formation
• Two-scalar-field model for the interaction of dark energy and dark matter
• Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields
• Weak cosmic growth in coupled dark energy with a Lagrangian formulation
• Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
• Dynamical analysis for a vector-like dark energy
• Coupled quintessence and vacuum decay
• A preliminary analysis of the energy transfer between the dark sectors of the Universe
• Fixed points in interacting dark energy models
• Exact solutions for the interacting tachyonic-dark matter system
• Bayesian Comparison of Interacting Scenarios
• FLRW cosmology with EDSFD parametrization
• Unified model of baryonic matter and dark components
• Origin of Delta N_eff as a Result of an Interaction between Dark Radiation and Dark Matter
• Soft coincidence in late acceleration
• Cosmological implications of an interacting model of dark matter \& dark energy
• Variable Cosmological Constant model: the reconstruction equations and constraints from current observational data
• Non-adiabatic perturbations in decaying vacuum cosmology
• Metastable dark energy
• Effective growth of matter density fluctuations in the running LCDM and LXCDM models
• Mass varying neutrinos, symmetry breaking, and cosmic acceleration
• A model-independent reconstruction of dark sector interactions
• Statefinder diagnosis for holographic dark energy in the DGP braneworld
• Cosmology with interaction in the dark sector
• Dark Energy Interacting with Dark Matter in Classical Einstein and Loop Quantum Cosmology
• Dark energy interacting with two fluids
• Quantum Corrections in Quintessence Models
• Non-adiabatic Chaplygin gas
• Hybrid Dark Sector: Locked Quintessence and Dark Matter
• Higher-order coupled quintessence
• General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter
• Solving the main cosmological puzzles with a generalized time varying vacuum energy
• Dynamics of three-form dark energy with dark matter couplings
• Dark-Energy Dynamics Required to Solve the Cosmic Coincidence
• Some remarks on the attractor behaviour in ELKO cosmology
• Anisotropic k-essence cosmologies
• Cosmic microwave background radiation temperature in a dissipative universe
• Late-time acceleration and Phantom Divide Line Crossing with Non-minimal Coupling and Lorentz Invariance Violation
• Interacting viscous ghost tachyon, K-essence and dilaton scalar field models of dark energy
• Conformally Coupled Tachyonic Dark Energy
• Kinetically coupled dark energy
• SNLS data are consistent with acceleration at z=3
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• Can noncommutative effects account for the present speed up of the cosmic expansion?
• Equations of State in the Brans-Dicke cosmology
• On the phantom barrier crossing and the bounds on the speed of sound in non-minimal derivative coupling theories
• Observational Constraints on Dynamical Dark Energy Models
• Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off
• Finsler-Randers-Sasaki gravity and cosmology
• Physical constraints on interacting dark energy models
• Notes on interacting holographic dark energy model in a closed universe
• CMB and matter power spectra with non-linear dark-sector interactions
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Thermodynamical description of the interacting new agegraphic dark energy
• J-PAS: forecasts on interacting vacuum energy models
• A tachyonic scalar field with mutually interacting components
• Coupled vector dark energy
• Scrutinizing Various Phenomenological Interactions In The Context Of Holographic Ricci Dark Energy Models
• Coincidence Problem in $f(R)$ Gravity Models
• The Dark Sector Cosmology
• Dark Matter-Dark Energy Interaction and the Shape of Cosmic Voids
• Reconstruction of interaction rate in Holographic dark energy
• Gravitational Baryogenesis in Anisotropic Universe
• Archimedean-type force in a cosmic dark fluid: I. Exact solutions for the late-time accelerated expansion
• Sourced Friedmann equations with holographic energy density
• Dark energy interacting with dark matter and unparticle
• Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• The impact of neutrino masses on the determination of dark energy properties
• Testing the interaction model with cosmological data and gamma-ray bursts
• Observational constraints on a generalized equation of state model
• Effective dark energy equation of state in interacting dark energy models
• Dark Gravitational Sectors on a Generalized Scalar-Tensor Vector Bundle Model and Cosmological Applications
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Archimedean-type force in a cosmic dark fluid: II. Qualitative and numerical study of a multistage Universe expansion
• Self-interacting holographic dark energy
• An exact model of conformal quintessence
• $w_d=-1$ in interacting quintessence model
• Cosmological perturbations and dynamical analysis for interacting quintessence
• Spherically symmetric solutions and gravitational collapse in brane-worlds
• Limits on the parameters of the equation of state for interacting dark energy
• A New Type of Dark Energy Model
• Interacting Tsallis holographic dark energy: Cosmic behaviour, statefinder analysis and ${\omega }_D-{\omega }_D^{\prime }$ pair in the non-flat universe
• Interacting Tsallis and Rényi Holographic Dark Energy with Hybrid Expansion Law
• Dynamics of Dirac-Born-Infeld dark energy interacting with dark matter
• Symmetry breaking and the onset of cosmic acceleration in scalar field models
• Holographic interacting dark energy in the braneworld cosmology
• Phase Space Analysis and Thermodynamics of Interacting Umami Chaplygin gas in FRW Universe
• Wormhole solutions supported by interacting dark matter and dark energy
• Exploring the new Tsallis agegraphic dark energy with interaction through statefinder
• Unmodified Gravity
• Lagrangian description of cosmic fluids: mapping dark energy into unified dark energy
• The generalized second law of thermodynamics for interacting $f(R)$ gravity
• Constraining the interacting dark energy models from weak gravity conjecture and recent observations
• Dynamics of viscous cosmologies in the full Israel-Stewart formalism
• Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
• A study of generalized second law of thermodynamics in modified f(R) Horava-Lifshitz gravity
• QCD modified ghost scalar field dark energy models
• Crossing the phantom divide line in the Holographic dark energy model in a closed universe
• Coupling dark energy to dark matter inhomogeneities
• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• Revisiting The Coincidence Problem in $f(R)$ Gravitation
• Exact cosmological solutions of models with an interacting dark sector
• An interacting model for the cosmological dark sector
• A quantitative criteria for the coincidence problem
• Crossing the Phantom divide line in the Chaplygin gas model
• Interacting agegraphic quintessence dark energy in non-flat universe
• Time-averaging axion-like interacting scalar fields models
• QCD ghost dark energy cannot (even roughly) explain the main features of the accepted cosmological paradigm
• Unconventional cosmology on the (thick) brane
• The BICEP2 data and a single Higgs-like interacting tachyonic field
• Quintessence as k-essence
• Unphysical properties in a class of interacting dark energy models
• Inhomogeneous models of interacting dark matter and dark energy
• Coupled quintessence with a possible transient accelerating phase
• Expanding Universe: slowdown or speedup?
• Superconducting dark energy
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Cosmic acceleration from interaction of ordinary fluids
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Duality invariance and cosmological dynamics
• Quintessence Model and Observational Constraints
• Power-law solutions and accelerated expansion in scalar-tensor theories
• $H(z)$ diagnostics on the nature of dark energy
• From inflation to late time acceleration with a decaying vacuum coupled to radiation or matter
• Non-flat universe and interacting dark energy model
• (m,n)-type holographic dark energy models
• Cosmological constraints on a dark matter -- dark energy interaction
• Reconstructing the interaction between the dark matter and holographic dark energy
• Interaction between phantom field and modified Chaplygin gas
• Constraints on $\Lambda (t)$-cosmology with power law interacting dark sectors
• Evolution of shifted cosmological parameter and shifted dust matter in a two-phase tachyonic field universe
• Thawing in a coupled quintessence model
• A model of dark matter dark energy interaction with some cosmic consequences
• Interacting dark energy in the dark $SU(2{)}_R$ model
• New Tsallis Agegraphic Dark Energy
• Interacting Ricci Logarithmic Entropy Corrected Holographic Dark Energy in Brans-Dicke Cosmology
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• A Lorentz Invariance Violating Cosmology on the DGP Brane
• Addressing the High-$f$ Problem in Pseudo-Nambu-Goldstone Boson Dark Energy Models with Dark Matter - Dark Energy Interaction
• Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
• Bulk viscous cosmological model with interacting dark fluids
• Interacting holographic tachyon model of dark energy
• Interacting viscous entropy-corrected holographic scalar field models of dark energy with time-varying G in modified FRW cosmology
• Cosmological models with running cosmological term and decaying dark matter
• Interacting agegraphic dark energy models in phase space
• Structure and evolution of Zel'dovich pancakes as probes of dark energy models
• Ghost dark energy with sign-changeable interaction term
• The Extended Analysis On New Generalized Chaplygin Gas
• The accelerated scaling attractor solution of the interacting agegraphic dark energy in Brans-Dicke theory
• Decaying Vacuum Inflationary Cosmologies: A Complete Scenario Including Curvature Effects
• II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Interacting warm dark matter
• New Cosmographic Constraints on the Dark Energy and Dark Matter Coupling
• Exploring evidence of interaction between dark energy and dark matter
• A low-$z$ test for interacting dark energy
• Thermodynamic descriptions of Polytropic gas and its viscous type as the dark energy candidates
• Bulk viscosity, interaction and the viability of phantom solutions
• Holographic field theory models of dark energy in interaction with dark matter
• Cosmology In Terms Of The Deceleration Parameter. Part II
• Spherical collapse in coupled quintessence with a $\Lambda$CDM background
• Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
• Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
• Coupled Quintessence scalar field model in light of observational datasets
• Internal symmetry in Bianchi type-I cosmologies
• Cosmological constraints on superconducting dark energy models
• Stability analysis of an interacting holographic dark energy model
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Cosmological Constraints on the Phenomenological Interacting Dark Energy Model with Fermi Gamma-Ray Bursts and DESI DR2
• Interacting Holographic dark energy with matter creation: A dynamical system analysis
• Ghost Chaplygin scalar field model of dark energy
• Constraints on Dark Energy state equation with varying pivoting redshift
• Interacting parametrized post-Friedmann method
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Thermodynamical description of modified generalized Chaplygin gas model of dark energy
• Late-Time Anisotropy Sourced by a 2-Form Field Non-Minimally Coupled to Cold Dark Matter
• Anisotropic Dark Energy and the Generalized Second Law of Thermodynamics
• 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
• Interacting Barrow Holographic Dark Energy in Non-flat Universe
• APPLIED COSMOGRAPHY: A Pedagogical Review
• Can local bulk effects explain the galactic dark matter?
• Interactions in the dark sector of the Universe
• Non-local dilaton coupling to dark matter: cosmic acceleration and pressure backreaction
• Is interacting vacuum viable?
• Global asymptotic dynamics of the cubic galileon interacting with dark matter
• Ricci-cubic holographic dark energy
• Interacting Kasner-type cosmologies
• Coincidence problem within dark energy as a coupled self-interacting Bose-Einstein gas
• Qualitative analysis for viscous cosmologies in a non linear regime of the Israel-Stewart formalism
• Probing extra dimensions through cosmological observations of dark energy
• Future cosmological evolution in $f(R)$ gravity using two equations of state parameters
• The role of Dark Matter interaction in galaxy clusters
• Interacting dark energy: the role of microscopic feedback in the dark sector
• Gravitational waves during inflation from a 5D large-scale repulsive gravity model
• Thermodynamical study of FRW universe in Quasi-Topological Theory
• The coincidence problem in $f(R)$ gravity models
• The Maxwell--Boltzmann gas with non-standard self--interactions: a novel approach to galactic dark matter
• Impact of dark energy on the equation of state in light of the latest cosmological data
• Coupled quintessence inspired by warm inflation
• Non-Linearly Interacting Ghost Dark Energy in Brans-Dicke Cosmology
• A new way to test the WIMP dark matter models
• Dynamics of expansion of the Universe in the models with non-minimally coupled dark energy
• Constraining an Expanding Locally Anisotropic metric from the Pioneer anomaly
• Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
• Prospects of probing dark energy with eLISA: Standard versus null diagnostics
• Eternal vs singular observers in interacting dark energy-dark matter models
• Bayesian analysis of running holographic Ricci dark energy
• Evolution of cosmological perturbations in the models with interacting dynamical dark energy
• Coupled quintessence and curvature-assisted acceleration
• Layzer-Irvine equation: new perspectives and the role of interacting dark energy
• Fermionic and scalar fields as sources of interacting dark matter-dark energy
• On a class of scaling FRW cosmological models
• Curvature Coupling and Accelerated Expansion of the Universe
• Chameleon dark matter stars
• Deviations from the von Laue condition: Implications for the on-shell Lagrangian of particles and fluids
• Perturbation in an interacting dark universe
• Agegraphic dark energy with the sign-changeable interaction in non-flat universe
• Cosmic Evolution in a Modified Brans-Dicke Theory
• Dark Energy from Topology
• Is the Cosmological Constant of Topological Origin?
• Probing the independence within the dark sector in the fluid approximation
• Power-law solutions for TeVeS
• Non-linear coupling in the dark sector as a running vacuum model
• Coupling q-deformed dark energy to dark matter
• Massive gravitons dark matter scenario revisited
• Statefinder diagnosis of nearly flat and thawing non-minimal quintessence
• Cosmology from a running vacuum model driven by a scalar field
• Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
• Preheating and Dark Sector of Universe
• Degeneracy between warm and coupled cold dark matter: A clarifying note
• Inconsistences in Interacting Agegraphic Dark Energy Models
• Interacting Models of Generalised Chaplygin Gas and Modified Chaplygin Gas with Barotropic Fluid
• Cosmology with dark energy decaying through its chemical-potential contribution
• Interacting dark fluid in the universe bounded by event horizon : A non-equilibrium prescription
• Reconstructing f(R) model from Holographic DE: Using the observational evidence
• Coupled Dark Energy field variation
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Recovery of fluctuation spectrum evolution from tomographic shear spectra
• Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
• Generic autonomous system approach to interacting dark energy models
• Some Classes of Interacting Two-Fluid Model of the Expanding Universe
• An exotic k-essence interpretation of interactive cosmological models
• A Thousand Problems in Cosmology: Interaction in the Dark Sector
• Is the cosmological dark sector better modeled by a generalized Chaplygin gas or by a scalar field?
• Dynamical analysis of Brans-Dicke Universe with inverse power-law effective potential
• Generalized Semi-Holographic Universe
• Massive neutrinos and dark energy
• Equivalence between generalized phenomenological schemes for the interaction of cosmological fluids: applications to arbitrary linear barotropic fluids and vacuum decay
• Probing Interacting Dark Sectors with upcoming Post-Reionization and Galaxy Surveys
• A topological origin for Dark Energy
• Crunching, Bouncing, and Cyclical Cosmologies from Dark Sector Interactions
• Halos of dark energy
• Background dynamics and observational constraints of flat and non-flat $\Lambda (t)$CDM models from $H(z)$ and DESI DR2 BAO measurements
• Linearly Interacting Barrow Holographic Dark Energy in Modified Cosmology
• The creation of radiation and the relic of inflaton potential
• Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
• Correspondence between particle creation and dark components interaction in the context of $f(\mathcal{G})$ gravity
• Accelerating scaling solutions from dark matter particle creation