Cosmology and the Fate of Dilatation Symmetry

Abstract

We discuss the cosmological constant problem in the light of dilatation symmetry and its possible anomaly. For dilatation symmetric quantum theories realistic asymptotic cosmology is obtained provided the effective potential has a non-trivial minimum. For theories with dilatation anomaly one needs as a non-trivial "cosmon condition" that the energy-momentum tensor in the vacuum is purely anomalous. Such a condition is related to the short-distance renormalization group behavior of the fundamental theory. Observable deviations from the standard hot big bang cosmology are possible.

arXiv commentOriginal preprint from 1987, 15 pages

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• Massive fields temper anomaly-induced inflation: the clue to graceful exit?
• Non-local SFT Tachyon and Cosmology
• $\Lambda \alpha$DM: Observational constraints on unified dark matter with constant speed of sound
• Curvaton reheating: an application to braneworld inflation
• Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
• Gravity from Spinors
• Dynamics of interacting quintessence
• Split Two-Higgs-Doublet Model and Neutrino Condensation
• Cosmic slowing down of acceleration for several dark energy parametrizations
• Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
• FRW Quantum Cosmology with a Generalized Chaplygin Gas
• Age constraints and fine tuning in variable-mass particle models
• Dynamics of interacting phantom scalar field dark energy in Loop Quantum Cosmology
• Quintessence Saves Higgs Instability
• Inflation, quintessence, and the origin of mass
• Modeling Dynamical Dark Energy
• The impact of Early Dark Energy on non-linear structure formation
• Scalar Tensor Teleparallel Dark Gravity via Noether Symmetry
• Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy
• No fifth force in a scale invariant universe
• Constraints on barotropic dark energy models by a new phenomenological $q(z)$ parameterization
• Teleparallel quintessence with a nonminimal coupling to a boundary term
• Clarifying the effects of interacting dark energy on linear and nonlinear structure formation processes
• The reliability of the AIC method in Cosmological Model Selection
• Effect of Varying Bulk Viscosity on Generalized Chaplygin Gas
• Gauging scale symmetry and inflation: Weyl versus Palatini gravity
• CMB and BAO constraints for an induced gravity dark energy model with a quartic potential
• Gamma-ray bursts as dark energy-matter probes in the context of the generalized Chaplygin gas model
• Clarifying spherical collapse in coupled dark energy cosmologies
• The evidence of cosmic acceleration and observational constraints
• Statefinder diagnostic and stability of modified gravity consistent with holographic and new agegraphic dark energy
• Cosmic voids in coupled dark energy cosmologies: the impact of halo bias
• Constraining a spatially dependent rotation of the Cosmic Microwave Background Polarization
• Cosmological evolution in vector-tensor theories of gravity
• The Inflaton Field as Self-Interacting Dark Matter in the Braneworld Scenario
• Soundness of Dark Energy properties
• Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem
• Mass functions in coupled Dark Energy models
• Scale-Invariant Gravity: Geometrodynamics
• Graviton fluctuations erase the cosmological constant
• Asymptotic behavior of the warm inflation scenario with viscous pressure
• Inflation and Transition to a Slowly Accelerating Phase from S.S.B. of Scale Invariance
• Evolution of a Kerr-Newman black hole in a dark energy universe
• The effect of modified gravity on weak lensing
• A comprehensive comparison of cosmological models from latest observational data
• Invariant solutions and Noether symmetries in Hybrid Gravity
• Reconstructing the dark energy equation of state with varying couplings
• Small Scale Structure Formation in Chameleon Cosmology
• Probing Dark Energy Using Its Density Instead of Its Equation of State
• Physics of dark energy particles
• CMB Lensing Constraints on Neutrinos and Dark Energy
• Scaling solutions for Dilaton Quantum Gravity
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Can Structure Formation Influence the Cosmological Evolution?
• Galaxy morphology rules out astrophysically relevant Hu-Sawicki $f(R)$ gravity
• The stability of cosmological scaling solutions
• Chameleon dark energy models with characteristic signatures
• Cosmic acceleration and crossing of w=-1 barrier in non-local Cubic Superstring Field Theory model
• Dark Energy Model in Anisotropic Bianchi Type-III Space-Time with Variable EoS Parameter
• Manifestly scale-invariant regularization and quantum effective operators
• Dark energy, dissipation and the coincidence problem
• Interacting Ghost Dark Energy in Brans-Dicke Theory
• Quintessence reconstructed: new constraints and tracker viability
• Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos
• Phenomenology of dark energy: exploring the space of theories with future redshift surveys
• Long Range Interactions in Cosmology: Implications for Neutrinos
• Non-minimal Kinetic coupling to gravity and accelerated expansion
• Quintessence Models and the Cosmological Evolution of alpha
• On the Cosmological Constant Problems and the Astronomical Evidence for a Homogeneous Energy Density with Negative Pressure
• Kinetic k-essence ghost dark energy model
• Non-minimal quintessence and phantom with nearly flat potentials
• Description of Supernova Data in Conformal Cosmology without Cosmological Constant
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Cosmon dark matter?
• Cosmological constraints on induced gravity dark energy models
• Dark Energy Constraints after Planck
• Constraining power of asymptotic safety for scalar fields
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Constraining Modified Gravity and Growth with Weak Lensing
• Alpenglow - A Signature for Chameleons in Axion-Like Particle Search Experiments
• Phantom energy mediates a long-range repulsive force
• Independent cosmological constraints from high-z HII galaxies: new results from VLT-KMOS data
• New interactions in the dark sector mediated by dark energy
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Reconstruction of f(T) gravity from the Holographic dark energy
• Energy conditions in generalized teleparallel gravity models
• Connecting early and late universe by $f(R)$ gravity
• Exact Analysis of Scaling and Dominant Attractors Beyond the Exponential Potential
• Cosmological constraints on extended Galileon models
• Density Perturbations for Running Cosmological Constant
• Relaxing Nucleosynthesis Constraints on Brans-Dicke Theories
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Consistent perturbations in an imperfect fluid
• Constraints on long-range spin-gravity and monopole-dipole couplings of the proton
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• Of pNGB QuiNtessence
• Towards inflation and dark energy cosmologies from modified Gauss-Bonnet theory
• Quintessential Adjustment of the Cosmological Constant
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Inflation in a scale invariant universe
• Dynamical Relaxation of Dark Energy: A Solution to Early Inflation, Late-time Acceleration and the Cosmological Constant Problem
• Wormholes and Ringholes in a Dark-Energy Universe
• A model of interacting holographic dark energy at the Ricci's scale
• Notes on dark energy interacting with dark matter and unparticle in loop quantum cosmology
• Generalized Chaplygin Gas in a modified gravity approach
• High-z massive clusters as a test for dynamical coupled dark energy
• An evaluation of cosmological models from expansion and growth of structure measurements
• A Brane World Solution to the Cosmological Constant Problem
• Warm Quintessential Inflation
• Effects of dark energy on the efficiency of charged AdS black holes as heat engine
• Cosmic Acceleration from M Theory on Twisted Spaces
• The latitude dependence of the rotation measures of NVSS sources
• Stability analysis for cosmological models in $f(R)$ gravity using dynamical system analysis
• Spontaneously Broken Conformal Symmetry: Dealing with the Trace Anomaly
• New Constraints from High Redshift Supernovae and Lensing Statistics upon Scalar Field Cosmologies
• Inertial Spontaneous Symmetry Breaking and Quantum Scale Invariance
• Dark energy equation of state and anthropic selection
• Weak lensing in generalized gravity theories
• Evolution of dark-matter haloes in a variety of dark-energy cosmologies
• A Quintom scenario with mixed kinetic terms
• Observational constraints on the interacting Ricci dark energy model
• Traversable wormholes in the extended teleparallel theory of gravity with matter coupling
• Accelerating Universes and String Theory
• Early massive clusters and the bouncing coupled dark energy
• A Universe without expansion
• Cosmology with moving dark energy and the CMB quadrupole
• Chameleon scalar fields in relativistic gravitational backgrounds
• Models of Baryogenesis via Spontaneous Lorentz Violation
• Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
• The effective field theory of inflation/dark energy and the Horndeski theory
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• Mapping the Chevallier-Polarski-Linder parametrization onto Physical Dark Energy Models
• On the potentials yielding cosmological scaling solutions
• Modified gravity with $f(R)=\sqrt{R^2-R_0^2}$
• A New Approach to Quintessence and a Solution of Multiple Attractors
• Stability analysis of the Tsallis holographic dark energy model
• Tsallis Agegraphic Dark Energy Model
• Phantom-like behaviour in dilatonic brane-world scenario with induced gravity
• Holographic hessence models
• Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
• Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• Cosmological Evolution of Brane World Moduli
• Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
• Cosmological dynamics of dark energy in scalar-torsion $f(T,\varphi )$ gravity
• Cosmological Backreaction from Perturbations
• Dark energy scenario consistent with GW170817 in theories beyond Horndeski gravity
• Structure formation with scalar field dark matter: the field approach
• Primordial black holes from fifth forces
• Future CMB constraints on cosmic birefringence and implications for fundamental physics
• Interacting Entropy-Corrected Holographic Dark Energy and IR Cut-Off Length
• Tracking quintessential inflation from brane worlds
• Constraints on Cosmic Quintessence and Quintessential Inflation
• Remarks on the formulation of the cosmological constant/dark energy problems
• Measuring deviations from a cosmological constant: a field-space parameterization
• Accelerating cosmologies tested by distance measures
• Perturbation evolution with a non-minimally coupled scalar field
• Testing the Cosmological Constant as a Candidate for Dark Energy
• Cosmology in generalized Horndeski theories with second-order equations of motion
• Scalar-tensor theories with pseudoscalar couplings
• Unexorcized ghost in DGP brane world
• Noether Symmetry Approach in multiple scalar fields Scenario
• 2-loop Quantum Yang-Mills Condensate as Dark Energy
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Extended Quintessence with non-minimally coupled phantom scalar field
• Observational constraints on a holographic, interacting dark energy model
• Attractor solutions for general hessence dark energy
• Cosmological evolution of interacting phantom (quintessence) model in Loop Quantum Gravity
• Perturbations in cosmologies with a scalar field and a perfect fluid
• Gravitational wave constraints on dark sector models
• Interacting Ricci Dark Energy with Logarithmic Correction
• Large-scale inhomogeneities in modified Chaplygin gas cosmologies
• How to Distinguish Dark Energy and Modified Gravity?
• Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure
• Dark Energy Constraints from Baryon Acoustic Oscillations
• Current Observational Constraints on Cosmic Doomsday
• Gravitational waves from global cosmic strings in quintessential inflation
• Cheng-Weyl Vector Field and its Cosmological Application
• Exact scaling solutions and fixed points for general scalar field
• Tachyonic Teleparallel Dark Energy
• Transient Accelerated Expansion and Double Quintessence
• Fitting the Constitution SNIa Data with Redshift Binned Parameterization Method
• Consistency of $f(R)=\sqrt{R^2-R_0^2}$ Gravity with the Cosmological Observations in Palatini Formalism
• Dark Energy and Right-Handed Neutrinos
• On the equation of state of Dark Energy
• Hubble-induced phase transitions on the lattice with applications to Ricci reheating
• Dynamics of a scalar field in Robertson-Walker spacetimes
• CMBEASY:: an Object Oriented Code for the Cosmic Microwave Background
• Dynamical systems analysis in $f(T,\varphi )$ gravity
• Higgs-Dilaton Cosmology: An inflation - dark energy connection and forecasts for future galaxy surveys
• Cosmology with nonminimal kinetic coupling and a power-law potential
• New limits on Early Dark Energy from the South Pole Telescope
• Phantom phase power-law solution in $f(G)$ gravity
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• Transient cosmic acceleration from interacting fluids
• Conditions and instability in $f(R)$ gravity with non-minimal coupling between matter and geometry
• Dynamics of assisted quintessence
• Quintessence Cosmology and the Cosmic Coincidence
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Avoiding the Big-Rip Jeopardy in a Quintom Dark Energy Model with Higher Derivatives
• Cosmic vector for dark energy: constraints from SN, CMB and BAO
• Signatures of Horndeski gravity on the Dark Matter Bispectrum
• Constraints on a variable dark energy model with recent observations
• Non-minimally coupled scalar field cosmology on the phase plane
• UV Shadows in EFTs: Accidental Symmetries, Robustness and No-Scale Supergravity
• Challenges and Obstacles for a Bouncing Universe in Brane Models
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Thermal leptogenesis with triplet Higgs boson and mass varying neutrinos
• On the Magnitude of Dark Energy Voids and Overdensities
• Quintessential Baryogenesis
• Coincidence Problem in YM Field Dark Energy Model
• Generalized second law of thermodynamics for a phantom energy accreting BTZ black hole
• Statefinder Diagnostic for Dilaton Dark Energy
• Non-universal scalar-tensor theories and big bang nucleosynthesis
• Is the radion a chameleon?
• The dS swampland conjecture with the electroweak symmetry and QCD chiral symmetry breaking
• Looking Beyond Lambda with the Union Supernova Compilation
• Fine Tuning in Quintessence Models with Exponential Potentials
• Interacting entropy-corrected new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Dark energy: investigation and modeling
• Are Domain Walls ruled out ?
• Braneworld Mimetic Cosmology
• Dark energy records in lensed cosmic microwave background
• Current Constraints on Anisotropic and Isotropic Dark Energy Models
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Cosmological models with Lagrange Multiplier Field
• Complete Set of Homogeneous Isotropic Analytic Solutions in Scalar-Tensor Cosmology with Radiation and Curvature
• Emergent Universe from Scale Invariant Two Measures Theory
• Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
• Spinor Gravity
• Cosmic perturbations with running G and Lambda
• Coupled Quintessence and the Halo Mass Function
• Anisotropic brane gravity with a confining potential
• Classification of dark energy models in the (w_0,w_a) plane
• Gauge-Invariant Initial Conditions and Early Time Perturbations in Quintessence Universes
• Interacting Ghost Dark Energy Models with Variable $G$ and $\Lambda$
• Implication of Compensator Field and Local Scale Invariance in the Standard Model
• Field theory model giving rise to "quintessential inflation" without the cosmological constant and other fine tuning problems
• Massive Photon and Dark Energy
• The spherical collapse model in time varying vacuum cosmologies
• Principal Component Analysis of Modified Gravity using Weak Lensing and Peculiar Velocity Measurements
• Two-loop scale-invariant scalar potential and quantum effective operators
• The transient acceleration from time-dependent interacting dark energy models
• Dark Energy and the Fate of the Universe
• Modified gravity realizations of quintom dark energy after DESI DR2
• Cosmology with matter diffusion
• New Interaction between Dark Energy and Dark Matter Changes Sign during Cosmological Evolution
• New agegraphic dark energy as a rolling tachyon
• Shifting the Universe: Early Dark Energy and Standard Rulers
• Cosmological perturbations and observational constraints on nonlocal massive gravity
• Dark Energy from $\alpha$-Attractors
• Testing Einstein Gravity with Cosmic Growth and Expansion
• Volume elements of spacetime and a quartet of scalar fields
• Probing the imprints of generalized interacting dark energy on the growth of perturbations
• Running couplings with a vanishing scale anomaly
• Palatini $R^2$ Quintessential Inflation
• Power-law solutions in $f(T)$ gravity
• Quantum FRW cosmological solutions in the presence of Chaplygin gas and perfect fluid
• Anisotropic cosmological solutions in massive vector theories
• Vacuum Energy, the Cosmological Constant and Compact Extra Dimensions: Constraints from Casimir Effect Experiments
• Linear Growth of Structure in the Symmetron Model
• Dark matter-dark energy interaction for a time-dependent equation of state
• Cosmic age problem revisited in the holographic dark energy model
• Phenomenological Consequences of the Refined Swampland Conjecture
• ISW effect in Unified Dark Matter Scalar Field Cosmologies: an analytical approach
• Bayesian Evidences for Dark Energy models in light of current obsevational data
• Late Decaying Dark Matter, Bulk Viscosity and the Cosmic Acceleration
• Unified universe history through phantom extended Chaplygin gas
• Quintessential inflation: A tale of emergent and broken symmetries
• Evolving Planck Mass in Classically Scale-Invariant Theories
• Extended Chaplygin Gas in Horava-Lifshitz Gravity
• Constraining chameleon field theories using the GammeV afterglow experiments
• Early Dark Energy at High Redshifts: Status and Perspectives
• Coupling constant constraints in a nonminimally coupled phantom cosmology
• A few cosmological implications of tensor nonlocalities
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Dynamically avoiding fine-tuning the cosmological constant: the "Relaxed Universe"
• Eternal Universe
• Coupled Quintessence and Phantom Based On a Dilaton
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• Cosmological Evolution on Self-Tuned Branes and the Cosmological Constant
• Phantom crossing and quintessence limit in extended nonlinear massive gravity
• $\Lambda$CDM Bounce Cosmology without $\Lambda$CDM: the case of modified gravity
• Generalised cosmological scaling solutions
• The Imprint of f(R) Gravity on Non-Linear Structure Formation
• Unimodular $f(R,T)$ Gravity
• Effective equation of state for running vacuum: "mirage" quintessence and phantom dark energy
• Generalized Compactification and Assisted Dynamics of Multi--Scalar Field Cosmologies
• Very large scale structures in growing neutrino quintessence
• Fifth forces, Higgs portals and broken scale invariance
• Brane assisted quintessential inflation with transient acceleration
• Combined cosmological and solar system constraints on chameleon mechanism
• Does the Big Rip survive quantization?
• From spacetime foam to holographic foam cosmology
• Observational Constraints on Cardassian Expansion
• Late time acceleration due to generic modification of gravity and Hubble tension
• The Cosmic Microwave Background for a Nearly Flat Compact Hyperbolic Universe
• Testing the DGP model with ESSENCE
• Quintessential Affleck-Dine baryogenesis with non-minimal couplings
• Dynamics of coupled phantom and tachyon fields
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• The onset of star formation in primordial haloes
• Non-minimal kinetic coupling and the phenomenology of dark energy
• Testing dark energy models with a new sample of strong-lensing systems
• Approaching Lambda without fine-tuning
• Model-independent dark energy test with sigma_8 using results from the Wilkinson Microwave Anisotropy Probe
• Can Early Dark Energy be Detected in Non-Linear Structure?
• Reconstructing K-essence
• Toward a Unified Description of Dark Energy and Dark Matter from the Abnormally Weighting Energy Hypothesis
• Greybody factor for a scalar field coupling to Einstein's tensor
• Reconstructing the dark energy potential
• Some remarks about non-minimally coupled scalar field models
• When Did Cosmic Acceleration Start ?
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• The $F$-term Problem and other Challenges of Stringy Quintessence
• Reconstructing the interaction rate in holographic models of dark energy
• Stationary Configurations Imply Shift Symmetry: No Bondi Accretion for Quintessence / k-Essence
• Dark energy and dark matter from cosmological observations
• Cosmological Perturbations in Elastic Dark Energy Models
• Superbounce and Loop Quantum Cosmology Ekpyrosis from Modified Gravity
• A dual-isotope rubidium comagnetometer to search for anomalous long-range spin-mass (spin-gravity) couplings of the proton
• Conformal fixed point, Cosmological Constant and Quintessence
• Astrophysical Constraints on Scalar Field Models
• Observational constraints on non-minimally coupled Galileon model
• Number counts in homogeneous and inhomogeneous dark energy models
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land
• Frame (In)equivalence in Quantum Field Theory and Cosmology
• Solution of Dirac equation and greybody radiation around a regular Bardeen black hole surrounded by quintessence
• Implications for quintessence models from MAXIMA-1 and BOOMERANG-98
• Catch-Me-If-You-Can: The Overshoot Problem and the Weak/Inflation Hierarchy
• Dark Energy, the Swampland and the Equivalence Principle
• Interacting new agegraphic viscous dark energy with varying $G$
• On exact solutions for quintessential (inflationary) cosmological models with exponential potentials
• Holographic thermalization and gravitational collapse in the spacetime dominated by quintessence dark energy
• Cosmology with non-minimal derivative couplings: perturbation analysis and observational constraints
• Fine Tuning Free Paradigm of Two Measures Theory: K-Essence, Absence of Initial Singularity of the Curvature and Inflation with Graceful Exit to Zero Cosmological Constant State
• Photon Geodesics in FRW Cosmologies
• Unified Model for Dark Energy
• The halo mass function in interacting Dark Energy models
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Naturalness of exponential cosmon potentials and the cosmological constant problem
• Average Effective Potential for the Conformal Factor
• Bouncing Universe and Reconstructing Vector Field
• Cosmological Dynamics of a Dirac-Born-Infeld field
• General approach to the Lagrangian ambiguity in $f(R,T)$ gravity
• Relaxing a large cosmological constant
• Probing non-standard gravity with the growth index: a background independent analysis
• Scaling solutions from interacting fluids
• Search for Tracker Potentials in Quintessence Theory
• Statefinder Parameters for Tachyon Dark Energy Model
• Holographic dark energy in a non-flat universe with Granda-Oliveros cut-off
• Quintessence in a quandary: prior dependence in dark energy models
• On using the WMAP distance priors in constraining the time evolving equation of state of dark energy
• Quintessential perturbations during scaling regime
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Limits on coupling between dark components
• Einstein-Cartan gravity, matter, and scale-invariant generalization
• Cosmological evolution of general scalar fields in a brane-world cosmology
• New Limits on Coupled Dark Energy from Planck
• Composite dark energy: cosmon models with running cosmological term and gravitational coupling
• Bose-Einstein Condensation, Dark Matter and Acoustic Peaks
• Neutrino lumps and the Cosmic Microwave Background
• Dynamic wormhole geometries in hybrid metric-Palatini gravity
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Cosmic Dynamics in the Chameleon Cosmology
• Confronting pNGB quintessence with data
• Gravity, Scale Invariance and the Hierarchy Problem
• Analysis of two quintessence models with SN Ia data
• Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology
• Standard Model with spontaneously broken quantum scale invariance
• Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields
• Observational signatures of the theories beyond Horndeski
• Reconstructing a String-Inspired Quintom Model of Dark Energy
• Are Galaxies Cosmon Lumps?
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• Quintessence and the Transition to an Accelerating Universe
• Effects of quintessence on observations of Type Ia SuperNovae in the clumpy Universe
• Observational constraints on generalized Chaplygin gas model
• Initial conditions for quintessence after inflation
• Baryon Acoustic Oscillations and Dynamical Dark Energy
• Qualitative analysis of Kantowski-Sachs metric in a generic class of $f(R)$ models
• Fixed points in interacting dark energy models
• A preliminary analysis of the energy transfer between the dark sectors of the Universe
• Statefinder diagnostic and $w-w^{\prime }$ analysis for interacting polytropic gas dark energy model
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• New Agegraphic Dark Energy in Brans-Dicke Theory
• The QCD Axion and Gravitational Waves in light of NANOGrav results
• Black hole perturbations in vector-tensor theories: The odd-mode analysis
• The Fifth Force in the Local Cosmic Web
• Dynamical evolution of a scalar field coupling to Einstein's tensor in the Reissner-Nordström black hole spacetime
• Ricci Inverse Anisotropic Stellar Structures
• Exploring the Foundations of the Universe with Space Tests of the Equivalence Principle
• Exploring the Latest Union2 SNIa Dataset by Using Model-Independent Parametrization Methods
• Cosmological Constant Problems and Renormalization Group
• Dark energy, gravitation and supernovae
• The swampland conjecture and the Higgs expectation value
• Constraints on interacting dark energy models from galaxy Rotation Curves
• Generalized dark energy interactions with multiple fluids
• Holographic dark energy in Brans-Dicke cosmology with Granda-Oliveros cut-off
• Stability of scalar perturbations in scalar-torsion $f(T,\varphi )$ gravity theories in the presence of a matter fluid
• Cosmological model-independent test of $\Lambda$CDM with two-point diagnostic by the observational Hubble parameter data
• Yoga Dark Energy: Natural Relaxation and Other Dark Implications of a Supersymmetric Gravity Sector
• A Universe Without Dark Energy: Cosmic Acceleration from Dark Matter-Baryon Interactions
• Boosting Ultraviolet Freeze-in in NO Models
• Dark energy cosmologies for codimension-two branes
• The Impact of Coupled Dark Energy Cosmologies on the High-Redshift Intergalactic Medium
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Can Coupled Dark Energy Speed Up the Bullet Cluster?
• Dark Matter and Dark Energy from a single scalar field and CMB data
• Density Perturbation Growth in Teleparallel Cosmology
• New tracker models of dark energy
• Predictive model for dark matter, dark energy, neutrino masses and leptogenesis at the TeV scale
• Exotic Low Density Fermion States in the Two Measures Field Theory: Neutrino Dark Energy
• Averaging Robertson-Walker Cosmologies
• Perceiving the equation of state of Dark Energy while living in a Cold Spot
• Duality extended Chaplygin cosmologies with a big rip
• Evolution of large-scale perturbations in quintessence models
• Multiple Dark Matter as a self-regulating mechanism for dark sector interactions
• Quintessence Axion Revisited in Light of Swampland Conjectures
• Accretion of Phantom Energy and Generalized Second Law of Thermodynamics for Einstein-Maxwell-Gauss-Bonnet Black Hole
• Dynamics of Generalized Assisted Inflation
• Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha
• Quantum scale invariance on the lattice
• Fifth force constraints from the separation of galaxy mass components
• Statefinder diagnosis and the interacting ghost model of dark energy
• What $\xi$? Cosmological constraints on the non-minimal coupling constant
• Absence of the Fifth Force Problem in a Model with Spontaneously Broken Dilatation Symmetry
• A Comparison of Cosmological Models Using Strong Gravitational Lensing Galaxies
• Cardassian Expansion: Dark Energy Density from Modified Friedmann Equations
• Tracker and scaling solutions in DHOST theories
• Testing for dynamical dark energy models with redshift-space distortions
• Dark Energy in a Hyperbolic Universe
• Asymptotic behavior of a scalar field with an arbitrary potential trapped on a Randall-Sundrum's braneworld: the effect of a negative dark radiation term on a Bianchi I brane
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• Non-adiabatic perturbations in decaying vacuum cosmology
• Fluid observers and tilting cosmology
• Extending the Coyote emulator to dark energy models with standard $w_0$-$w_a$ parametrization of the equation of state
• A comprehensive numerical study on four categories of holographic dark energy models
• Cosmological viability conditions for $f(T)$ dark energy models
• Cosmon inflation
• Holographic, new agegraphic and ghost dark energy models in fractal cosmology
• Unsuccessful cosmology with Modified Gravity Models
• Probing Inflation and Dark Energy with Current Cosmological Observations
• The $H_0$ Tension in Non-flat QCDM Cosmology
• Effective growth of matter density fluctuations in the running LCDM and LXCDM models
• Hubble-induced phase transitions: Walls are not forever
• Supernova Constraints on Models of Neutrino Dark Energy
• Holographic superconductors in quintessence AdS black hole
• "Detuned" f(R) gravity and dark energy
• Cosmology with exponential potentials
• An equation of state for purely kinetic k-essence inspired by cosmic topological defects
• Hot big bang or slow freeze?
• Static Configurations of Dark Energy and Dark Matter
• Scalar Field Cosmologies with Barotropic Matter: Models of Bianchi class B
• Field redefinitions in theories beyond Einstein gravity using the language of differential forms
• Mass varying neutrinos, symmetry breaking, and cosmic acceleration
• Scale and Weyl Invariance in Einstein-Cartan Gravity
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• Quintessential Kination and Thermal Production of Gravitinos and Axinos
• Chaotic scalar fields as models for dark energy
• Effective field theory of modified gravity on the spherically symmetric background: leading order dynamics and the odd-type perturbations
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Constraining screened fifth forces with the electron magnetic moment
• WMAP constraints on Cardassian model
• The Effect of Coupled Dark Energy on the Alignment between Dark Matter and Galaxy Distributions in Clusters
• Have Pulsar Timing Arrays detected the Hot Big Bang? Gravitational Waves from Strong First Order Phase Transitions in the Early Universe
• Viscous Generalized Chaplygin Gas Interacting with f(R,T) gravity
• Statefinder diagnostic for Yang-Mills dark energy model
• Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
• Some Impacts of Lorentz Violation on Cosmology
• Is the Dynamics of Tracking Dark Energy Detectable?
• Halo Formation from Yukawa Forces in the Very Early Universe
• Two Component Model of Dark Energy
• SSB of scale symmetry, fermion families and quintessence without the long-range force problem
• Disentangling dark sector models using weak lensing statistics
• Statefinder diagnosis for holographic dark energy in the DGP braneworld
• Stability of Einstein-Aether Cosmological Models
• Dark energy from approximate U(1)_{de} symmetry
• Constraining Quintessence with the New CMB Data
• Perturbations in electromagnetic dark energy
• Current Acceleration from Dilaton and Stringy Cold Dark Matter
• Do Observations Favour Galileon Over Quintessence?
• Axion Homeopathy: Screening Dilaton Interactions
• Extended phase-space analysis of the Horava-Lifshitz cosmology
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Derivative Chameleons
• Constraints on alternative models to dark energy
• Perturbative approach for mass varying neutrinos coupled to the dark sector in the generalized Chaplygin gas scenario
• Is Dark Energy Dynamical in the DESI Era? A Critical Review
• On extended sign-changeable interactions in the dark sector
• Quantum Corrections in Quintessence Models
• Curvature Singularities from Gravitational Contraction in f(R) Gravity
• Gravitational Effects of Disformal Couplings
• The cosmological constant and general isocurvature initial conditions
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• Quintessence dynamics with two scalar fields and mixed kinetic terms
• Quantum scale-invariant models as effective field theories
• Clustering of Galaxies with Dynamical Dark Energy
• Distance Measurements from Supernovae and Dark Energy Constraints
• Tracking Quintessence Would Require Two Cosmic Coincidences
• The Accelerated Acceleration of the Universe
• Composition-dependent long range forces from varying m_p/m_e
• Dark Energy and Dark Matter unification via superfluid Chaplygin gas
• Revisiting the Scalar Weak Gravity Conjecture
• Diagnostic of Horndeski Theories
• Asymptotic freedom and safety in quantum gravity
• General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Anisotropic k-essence cosmologies
• Effects of early dark energy on strong cluster lensing
• Self-similar spherically symmetric cosmological models with a perfect fluid and a scalar field
• Universality for quintessence
• Dynamics of three-form dark energy with dark matter couplings
• Infrared limit of quantum gravity
• Dark Energy and the Observable Universe
• Bouncing universe with the non-minimally coupled scaler field and its reconstructing
• Interacting Dark Energy in Hořava-Lifshitz Cosmology
• Geometrical Constraints on Dark Energy
• Interacting varying Ghost Dark energy models in General Relativity
• Interaction between viscous varying modified cosmic Chaplygin gas and Tachyonic fluid
• Variable G correction to statefinder parameters of dark energy
• Assisted dark energy
• Nonlinear cosmological consistency relations and effective matter stresses
• Inflation as a spontaneous symmetry breaking of Weyl symmetry
• Goldstone's Theorem and Hamiltonian of Multi-galileon Modified Gravity
• Statefinder parameters in two dark energy models
• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Anisotropic Weyl symmetry and cosmology
• Building Supergravity Quintessence Model
• Connecting Dark Energy to Neutrinos with an Observable Higgs Triplet
• Variable Chaplygin Gas: Constraints from CMBR and SNe Ia
• Mirror World and Superstring-Inspired Hidden Sector of the Universe, Dark Matter and Dark Energy
• Late-time evolution of the Universe within a two-scalar-field cosmological model
• Thermodynamics of Dark Energy
• Observational Constraints with Recent Data on the DGP Modified Gravity
• Cosmology of strongly interacting fermions in the early universe
• Cosmological parameters estimation in the Quintessence Paradigm
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Power-law Parameterized Quintessence Model
• Observational constraints on phantom power-law cosmology
• Cosmological dynamics with non-minimally coupled scalar field and a constant potential function
• Cosmic age test in inhomogeneous cosmological models mimicking $\Lambda$CDM on the light cone
• Anisotropic $2$-form dark energy
• Approximation of the potential in scalar field dark energy models
• Clarifying Forecasts of Dark Energy Constraints from Baryon Acoustic Oscillations
• Generalized Holographic Dark Energy and its Observational Constraints
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Dark Energy and the MSSM
• Extending the Gravitational Growth Framework
• Generalized Chaplygin gas model: Cosmological consequences and statefinder diagnosis
• The Phase-space analysis of scalar fields with non-minimally derivative coupling
• Decoupling of the general scalar field mode and the solution space for Bianchi type I and V cosmologies coupled to perfect fluid sources
• Field Flows of Dark Energy
• The dynamical viability of scalar-tensor gravity theories
• Fundamental Scale Invariance
• The Higgs boson -- its implications and prospects for future discoveries
• The Cosmological Constant Problem, an Inspiration for New Physics
• Scalar field cosmology in the energy phase-space -- unified description of dynamics
• Novel constraints on fifth forces and ultralight dark sector with asteroidal data
• New solutions with accelerated expansion in string theory
• Structure formation in Multiple Dark Matter cosmologies with long-range scalar interactions
• Effects of dark energy on dynamic phase transition of charged AdS black holes
• Accelerating universes driven by bulk particles
• Uniting cosmological epochs through the twister solution in cosmology with non-minimal coupling
• Probing dark energy with the CMB: projected constraints from WMAP and Planck
• Stable accelerating universe with no hair
• An effective quintessence field with a power-law potential
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Optimal parameterizations for observational constraints on thawing dark energy
• Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy
• Weyl Scaling Invariant $R^2$ Gravity for Inflation and Dark Matter
• Cosmological tests of an axiverse-inspired quintessence field
• On astrophysical bounds of the cosmological constant
• On dark energy models of single scalar field
• Phenomenological Varying Modified Chaplygin Gas with Variable $G$ and $\Lambda$: Toy Models for Our Universe
• Cosmology with nonminimal kinetic coupling and a Higgs-like potential
• Agegraphic Dark Energy Model in Non-Flat Universe: Statefinder Diagnostic and $w-w^{\prime }$ Analysis
• Probing the Evolution of the Dark Energy Density with Future Supernova Surveys
• Reconstructing a model of quintessential inflation
• Cosmological Evolution Across Phantom Crossing and the Nature of the Horizon
• Generalized interacting Barrow Holographic Dark Energy: cosmological predictions and thermodynamic considerations
• Cosmological black holes from self-gravitating fields
• The effective theory of fluids at NLO and implications for dark energy
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Holographic dark energy and late cosmic acceleration
• Response of distance measures to the equation of state
• Perturbations in a scalar field model with virtues of $\Lambda$CDM
• Coupled Multi-Proca Vector Dark Energy
• Can we test Dark Energy with Running Fundamental Constants ?
• Observational Implications of Cosmological Event Horizons
• Physical Parameters for Stable $f(R)$ Models
• Weyl Symmetry Inspired Inflation and Dark Matter
• Constraints on field flows of quintessence dark energy
• On the parameters of the spherically symmetric parametrized Rezzolla-Zhidenko spacetime through solar system tests, orbit of S2 star about Sgr A${}^{\star }$, and quasiperiodic oscillations
• Mass-Varying Neutrinos from a Variable Cosmological Constant
• Constraining the dark energy dynamics with the cosmic microwave background bispectrum
• Dark energy in scalar-vector-tensor theories
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• A short review on clustering dark energy
• Quintessence and the cosmological constant
• Growth of spherical overdensities in scalar-tensor cosmologies
• Primordial cosmic fluctuations for variable gravity
• Cosmology with a successful Vainshtein screening in theories beyond Horndeski
• CMB and matter power spectra with non-linear dark-sector interactions
• Moving dark energy and the CMB dipole
• Vacuum energy and the cosmological constant
• The Cosmological Constant, False Vacua, and Axions
• Phenomenological Fluids from Interacting Tachyonic Scalar Fields
• Field localization and Nambu Jona-Lasinio mass generation mechanism in an alternative 5-dimensional brane model
• Cosmic slowing down of acceleration using $f_{gas}$
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Can we ever distinguish between quintessence and a cosmological constant?
• A Specific Case of Generalized Einstein-aether Theories
• Time variation of fundamental couplings and dynamical dark energy
• Oscillating nonlinear large scale structure in growing neutrino quintessence
• Holographic kinetic k-essence model
• The Influence of Free Quintessence on Gravitational Frequency Shift and Deflection of Light with 4D momentum
• Cosmological Large-scale Structures beyond Linear Theory in Modified Gravity
• Quintessence and phantom dark energy from ghost D-branes
• Liouville-Lifshitz theory in 3+1 dimensions
• A brief note on how to unify dark matter, dark energy, and inflation
• Reconstruction of scalar potentials in two-field cosmological models
• String Inspired Quintom Model with Non-minimally Coupled Modified Gravity
• Quintom evolution in power-law potentials
• Exploring hints for dark energy density evolution in light of recent data
• Complementary constraints from FR IIb radio galaxies and X-ray gas mass fractions in clusters on non-standard cosmological models
• Modified gravity and coupled quintessence
• Observational constraints on the dark energy density evolution
• Suppressed cosmic growth in coupled vector-tensor theories
• Scale-dependent power spectrum from initial excited-de Sitter modes
• Neutrino Condensate as Origin of Dark Energy
• Cosmology with variable parameters and effective equation of state for Dark Energy
• Strong Gravitational Lensing and Dynamical Dark Energy
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• Spherical collapse in the extended quintessence cosmological models
• The general form of the coupled Horndeski Lagrangian that allows cosmological scaling solutions
• Dynamics and constraints of the Unified Dark Matter flat cosmologies
• Phase Transitions of Quintessential AdS Black Holes in M-theory/Superstring Inspired Models
• A new extended quintessence
• Dilatation symmetry in higher dimensions and the vanishing of the cosmological constant
• Constraining the Dark Universe
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Do cosmological data rule out $f(\mathcal{R})$ with $w\ne -1$?
• Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature
• Dark Energy, A Cosmological Constant, and Type Ia Supernovae
• Coupled vector dark energy
• Probing for the Cosmological Parameters with PLANCK Measurement
• Cosmic acceleration and extra dimensions: constraints on modifications of the Friedmann equation
• Dark Matter-baryon segregation in the non-linear evolution of coupled Dark Energy model
• Renormalization Ambiguities and Conformal Anomaly in Metric-Scalar Backgrounds
• Moduli evolution in the presence of flux compactifications
• Fierz-Pauli theory reloaded: from a theory of a symmetric tensor field to linearized massive gravity
• Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity
• Instability of Chaplygin gas trajectories in unified dark matter models
• Interacting modified holographic Ricci dark energy model and statefinder diagnosis in flat universe
• Thermodynamics of Spinor Quintom
• Dirac Neutrinos, Dark Energy and Baryon Asymmetry
• Fitting and forecasting non-linear coupled dark energy
• Lunar Laser Ranging constraints on nonminimally coupled dark energy and standard sirens
• Asymptotic Scale Invariance and its Consequences
• Inherently stable effective field theory for dark energy and modified gravity
• Route to Lambda in conformally coupled phantom cosmology
• Cosmological evolution of interacting dark energy in Lorentz violation
• Spontaneous Conformal Symmetry Breaking in Fishnet CFT
• Cosmology With Non-Minimally Coupled K-Field
• Parametrization of K-essence and Its Kinetic Term
• Thawing models in the presence of a generalized Chaplygin gas
• Dilaton Coupled Quintessence Model in the $\omega -{\omega }^{\prime }$ Plane
• From Asymptotic Safety to Dark Energy
• Hodge Duality and Cosmological Constant
• Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
• Parameterizing and Measuring Dark Energy Trajectories from Late-Inflatons
• A new pressure-parametrization unified dark fluid model
• On the covariant formalism of the effective field theory of gravity and its cosmological implications
• Born-Infeld Type Phantom Model in the $\omega -{\omega }^{\prime }$ Plane
• Moduli Evolution in Heterotic Scenarios
• Trace anomaly and infrared cutoffs
• Coupled dark energy and dark matter from dilatation anomaly
• Dark Energy and Dark Matter in General Relativity with local scale invariance
• Hidden and explicit quantum scale invariance
• Holographic dark energy with the sign-changeable interaction term
• Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity
• Age of the Universe in the Cardassian Model
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• Traversable holographic dark energy wormholes constrained by astronomical observations
• Rip/singularity free cosmology models with bulk viscosity
• Neutrino Lump Fluid in Growing Neutrino Quintessence
• Casimir Dark Energy, Stabilization of the Extra Dimensions and Gauss-Bonnet Term
• Networks of cosmological histories, crossing of the phantom divide line and potentials with cusps
• Non-minimal kinetic coupling and Chaplygin gas cosmology
• Symmetric Scalars
• Probing the speed of gravity with LVK, LISA, and joint observations
• Gauge coupling unification without leptoquarks
• Mass freezing in growing neutrino quintessence
• Fitting oscillating string gas cosmology to supernova data
• Cosmological acceleration
• Acceleration of the Universe
• Semi-analytic galaxy formation in early dark energy cosmologies
• Sounds of instability from generalized QCD ghost dark energy
• The Gravitational Horizon for a Universe with Phantom Energy
• Could the black hole singularity be a field singularity?
• A Model of Dark Energy and Dark Matter
• Inflation and Quintessence: Theoretical Approach of Cosmological Reconstruction
• Combined constraints on Cardassian models from supernovae, CMB and large-scale structure observations
• Effective Action for Cosmological Scalar Fields at Finite Temperature
• Improved Energy-Momentum Currents in Metric-Affine Spacetime
• Schrödinger-Wheeler-DeWitt equation in chaplygin gas FRW cosmological model
• Two scalar field cosmology from coupled one-field models
• Constraints on the cosmic equation of state: age conflict versus phantom energy. Age-redshift relations in an accelerated universe
• Cosmological bounds on oscillating dark energy models
• Isocurvature Perturbations of Dark Energy and Dark Matter from the Swampland Conjecture
• An exact model of conformal quintessence
• Logarithmic corrected $F(R)$ gravity in the light of Planck 2015
• Partial rip scenario - a cosmology with a growing cosmological term
• Cosmological implications of interacting polytropic gas dark energy model in non-flat universe
• Self-interacting holographic dark energy
• A New Type of Dark Energy Model
• Direct Detection Rates of Dark Matter Coupled to Dark Energy
• Phantom Instability of Viscous Dark Energy in Anisotropic Space-Time
• The general property of dynamical quintessence field
• Linear Perturbation constraints on Multi-coupled Dark Energy
• Proper Matter Collineations of Plane Symmetric Spacetimes
• Cosmological Scaling Solutions for Multiple Scalar Fields
• Chaplygin gas may prevent big trip
• Observational Constraints on a Variable Dark Energy Model
• Machine Learning and cosmographic reconstructions of quintessence and the Swampland conjectures
• CFT data and spontaneously broken conformal invariance
• Accretion of Chaplygin gas upon black holes: Formation of faster outflowing winds
• Inhomogeneous cosmologies, the Copernican principle and the cosmic microwave background: More on the EGS theorem
• New scaling solutions in cubic Horndeski theories
• New Scalar Field Quartessence
• Parametrization of Tachyon Field
• Limits on the parameters of the equation of state for interacting dark energy
• Unified picture for Dirac neutrinos, dark matter, dark energy and matter-antimatter asymmetry
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Constraints on Quintessence From Using Cosmological Data
• Cosmological Implications of 5-dimensional Brans-Dicke Theory
• Discrimination between Lambda-CDM, quintessence, and modified gravity models using wide area surveys
• Tracing the Nature of Dark Energy with Galaxy Distribution
• Suppression of matter couplings with a vector field in generalized Proca theories
• Most general cubic-order Horndeski Lagrangian allowing for scaling solutions and the application to dark energy
• Dilaton dominance in the early Universe dilutes Dark Matter relic abundances
• Perturbations in the relaxation mechanism for a large cosmological constant
• Dilaton-assisted generation of the Fermi scale from the Planck scale
• Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE
• Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy
• Mass Varying Neutrinos, Quintessence, and the Accelerating Expansion of the Universe
• Disformally Coupled Quintessence
• Fifth forces and broken scale symmetries in the Jordan frame
• Shadows of magnetically charged rotating black holes surrounded by quintessence
• Dark energy, curvature, and cosmic coincidence
• Prospects for Dark Energy Evolution: a Frequentist Multi-Probe Approach
• Dark energy and inflation invoked in CCGG by locally contorted space-time
• Cosmology-informed neural networks to solve the background dynamics of the Universe
• Reconstructing the properties of dark energy from recent observations
• General dynamical properties of cosmological models with nonminimal kinetic coupling
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Inverse Power Law Quintessence with Non-Tracking Initial Conditions
• Nonlinear matter spectra in growing neutrino quintessence
• Power-law entropy-corrected HDE and NADE in Brans-Dicke cosmology
• Interacting Tsallis holographic dark energy in higher dimensional Cosmology
• A simple parametrisation for coupled dark energy
• A Comment or two on Holographic Dark Energy
• Is Trans-Planckian Censorship a Swampland Conjecture?
• An Inverse $f(R)$ Gravitation for Cosmic Speed up, and Dark Energy Equivalent
• The Ultimate Fate of Life in an Accelerating Universe
• Theoretical Limits on Agegraphic Quintessence from Weak Gravity Conjecture
• Observed galaxy power spectrum in cubic Galileon model
• Power Spectrum with Auxiliary Fields in de Sitter Space
• From model dynamics to oscillating dark energy parameterisation
• Properties of scalar wave emission in a scalar-tensor theory with kinetic screening
• Quintessential inflation with a trap and axionic dark matter
• Coupling dark energy to dark matter inhomogeneities
• Parametrizations for tests of gravity
• Baryogenesis after Hyperextended Inflation
• The role of curvature in the slowing down acceleration scenario
• Future supernova probes of quintessence
• Properties of cosmologies with dynamical pseudo Nambu-Goldstone bosons
• On the effect of the degeneracy between w_0 and w_a
• Bouncing Universe with Non-minimally Coupled Quintom Matter
• Common Origin of Visible and Dark Universe
• Dark D-Brane Cosmology: from background evolution to cosmological perturbations
• Gaussian-process reconstructions and model building of quintom dark energy from latest cosmological observations
• Dark Energy and Neutrino CPT Violation
• Constraints on Dark Energy from the Observed Expansion of our Cosmic Horizon
• Competing bounds on the present-day time variation of fundamental constants
• Forecasts on interacting dark energy with standard sirens
• Transient acceleration from a hybrid Chaplygin gas
• Three dimensional dilatonic gravity's rainbow: exact solutions
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Inflation in gauge theory of gravity with local scaling symmetry and quantum induced symmetry breaking
• Cosmological Implications of a Scale Invariant Standard Model
• Cosmic acceleration and de Sitter expansion in hybrid mass varying neutrino model
• Importance of being nonminimally coupled: Scalar Hawking radiation from regular black holes
• Improved cosmological constraints on the curvature and equation of state of dark energy
• Quantum matter bounce with a dark energy expanding phase
• A comparison between axion-like and power law potentials in cosmological background
• Cosmological neutrino mass limit and the dynamics of dark energy
• Conformal GUT inflation, proton lifetime and non-thermal leptogenesis
• Gauss-Bonnet Dark Energy and the Speed of Gravitational Waves
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Evolution of perturbations in distinct classes of canonical scalar field models of dark energy
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• Small scale structures in coupled scalar field dark matter
• On detecting interactions in the dark sector with H(z) data
• Probing a cosmological model with a $\Lambda ={\Lambda }_0+3\beta H^2$ decaying-vacuum
• Coupling dark energy with Standard Model states
• Testing scale-invariant inflation against cosmological data
• Constraints on the Cosmological Constant due to Scale Invariance
• Imprints of non-standard Dark Energy and Dark Matter Models on the 21cm Intensity Map Power Spectrum
• Cosmology from pregeometry
• Quintessence as k-essence
• Sub-Quantum Dark Energy
• Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld
• Generalized Scalar Field Cosmologies: A Global Dynamical Systems Formulation
• Stability of a modified Jordan-Brans-Dicke theory in the dilatonic frame
• Einstein static universe on the brane supported by extended Chaplygin gas
• Is Thick Brane Model Consistent with the Recent Observations?
• Supernova constraints on Multi-coupled Dark Energy
• Exact quantum conformal symmetry, its spontaneous breakdown, and gravitational Weyl anomaly
• Testing gravity with gravitational wave friction and gravitational slip
• DESI constraints on $\alpha$-attractor inflationary models
• The tension on the cosmological parameters from different observational data
• Emergent Universe in the Braneworld Scenario
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• Matter Power Spectrum for Convex Quartessence
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• R\' enyi Holographic Dark Energy in Higher Dimension Cosmology
• Nonlinear growing neutrino cosmology
• Towards a Dark Sector Model from String Theory
• Unimodular Supergravity
• Long time black hole evaporation with bounded Hawking flux
• Anomaly-free scale symmetry and gravity
• Termination of the Phase of Quintessence by Gravitational Back-Reaction
• Studying the Intervention of an Unusual Term in $f(T)$ Gravity via Noether Symmetry
• Phase-space analysis of the cosmological 3-fluid problem: Families of attractors and repellers
• De-Sitter nonlinear sigma model and accelerating universe
• Who's Afraid of the Supersymmetric Dark? The Standard Model vs Low-Energy Supergravity
• Cosmological Perturbations and the Running Cosmological Constant Model
• Galileons, phantom fields, and the fate of the Universe
• Decoupling Dark Energy from Matter
• Impact of early dark energy on the Planck SZ cluster sample
• Can Strong Gravitational Lensing Constrain Dark Energy?
• Everpresent Lambda - II: Structural Stability
• A Dark Energy Model in Lyra Manifold
• Interacting Ghost Dark Energy in Complex Quintessence Theory
• Sesame: A power spectrum emulator pipeline for beyond-$\Lambda$CDM models
• Cosmological stability in $f(\varphi ,\mathcal{G})$ gravity
• Scalar field damping at high temperatures
• The effects on CMB power spectra and bispectra from the polarization rotation and its correlations with temperature and E-polarization
• Distinguishing cosmologies using the turn-around radius near galaxy clusters
• Cosmological constraints from low-redshift data
• Interacting Dark Energy: Dynamical System Analysis
• Interacting Quintessence in a New Scalar-Torsion Gravity
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Galaxy clusters and structure formation in quintessence versus phantom dark energy universe
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• On Dark Energy and Accelerated Reference Frames
• Investigating clustering dark energy with 3d weak cosmic shear
• Generalized Self-similar Scalar-Tensor Theories
• Twister quintessence scenario
• Hybrid dark energy
• Holographic dark energy with time varying $c^2$ parameter
• $H(z)$ diagnostics on the nature of dark energy
• Scalar field dark energy perturbations and the Integrated Sachs Wolfe effect
• Simulations of structure formation in interacting dark energy cosmologies
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Duality invariance and cosmological dynamics
• A gauge-invariant approach to interactions in the dark sector
• Holographic dark energy with time depend gravitational constant in the non-flat Ho$\check{r}$ava-Lifshitz cosmology
• Tracking Quintessence and Cold Dark Matter Candidates
• Possible evidence for "dark radiation" from Big Bang Nucleosynthesis Data
• Imprint of thawing scalar fields on large scale galaxy overdensity
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Scalar-tensor cosmologies without screening
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• The cosmological constant and higher dimensional dilatation symmetry
• Marginalized Fisher Forecast for Horndeski Dark Energy Models
• The fine tuning of the cosmological constant in a conformal model
• Combined cosmological tests of a bivalent tachyonic dark energy scalar field model
• Cosmological Constant in a Model with Superstring-Inspired E_6 Unification and Shadow Theta-Particles
• Constraining thawing and freezing models with cluster number counts
• Scaling Dark Energy
• Variable cosmological term $\Lambda (t)$
• Scale Invariant Gravity and Black Hole Ringdown
• Quintom fields from chiral K-essence cosmology
• Cosmological Evolution of Einstein-Aether Models with Power-law-like Potential
• Model Independent Analysis of Supernova Data, Dark Energy, Trans-Planckian Censorship and the Swampland
• $Om$ Diagnostic for Dilaton Dark Energy
• Power-law solutions and accelerated expansion in scalar-tensor theories
• Cosmological Models and Renormalization Group Flow
• Dark Energy Scaling from Dark Matter to Acceleration
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• The cosmological constant problem in codimension-two brane models
• Ultraviolet complete dark energy model
• Cosmic acceleration from coupling of baryonic and dark matter components: Analysis and diagnostics
• Renormalization Group for Non-minimal ${\varphi }^{2}R$ Couplings and Gravitational Contact Interactions
• The interaction of neutrinos with Phantom, Quintessence, and Quintum scalar fields and its effect on the formation of structures in the early Universe
• Cosmological Scaling Solutions with Tachyon:Modified Gravity Model
• The $k$-essence scalar field in the context of Supernova Ia Observations
• Reconstructing the interaction between the dark matter and holographic dark energy
• Interacting new agegraphic Phantom model of dark energy in non-flat universe
• Simplified Quartessence Cosmology
• Conformal $\alpha$-attractor Inflation with Weyl Gauge Field
• Holographic dark energy in Barrow cosmology with Granda-Oliveros IR cutoff
• Neutrino Dark Energy and Baryon Asymmetry from Higgs Sector
• Ellipsoidal configurations in the de Sitter spacetime
• Exponential Potentials and Attractor Solution of Dilatonic Cosmology
• Quasiattractor in models of new and chaotic inflation
• Scaling solutions and geodesics in moduli space
• Structure formation in the new Deser-Woodard nonlocal gravity model
• Unified Dark Matter, Dark Energy and Baryogenesis via a "Cosmological Wetting Transition''
• Cosmological dynamics of scalar fields with O(N) symmetry
• Stable de Sitter Vacua in 4 Dimensional Supergravity Originating from 5 Dimensions
• Interacting entropy-corrected holographic scalar field models in non-flat universe
• Quantizing the Eisenhart Lift
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• Anisotropic Scalar Field Dark Energy with a Disformally Coupled Yang-Mills Field
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• Gravitational Contact Interactions and the Physical Equivalence of Weyl Transformations in Effective Field Theory
• Dynamics of the scalar field in 5-dimensional Kaluza-Klein theory
• Neutrino generated dynamical dark energy with no dark energy field
• Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models
• Detecting dark energy in long baseline neutrino oscillations
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Interacting holographic dark energy models: A general approach
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• How CMB and large-scale structure constrain chameleon interacting dark energy
• Dark energy as a remnant of inflation and electroweak symmetry breaking
• Testing the nature of Dark Energy with Precision Cosmological constraints
• Light mass galileon and late time acceleration of the Universe
• Cosmology with the Square Kilometre Array by SKA-Japan
• DBI Galileon and Late time acceleration of the universe
• Dark Energy Perturbations Revisited
• The kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity
• Investigation of the fundamental constants stability based on the reactor Oklo burn-up analysis
• The evolution of the universe from noncompact Kaluza-Klein theory
• Dark Matter & Dark Energy from a single scalar field: CMB spectrum and matter transfer function
• A study on Cubic Galileon Gravity Using N-body Simulations
• Irreversible thermodynamics of dark energy on entropy-corrected apparent horizon
• Neutrino Phenomenology, Dark Energy and Leptogenesis from pseudo-Nambu-Goldstone Bosons
• Observational Constraints on Axions as Quintessence in String Theory
• Cosmology with a long range repulsive force
• Decaying dark matter mimicking time-varying dark energy
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions
• Dark Energy and Dark Matter in Galaxy Halos
• Dark Energy, Dark Matter and Baryogenesis from a Model of a Complex Axion Field
• First cosmological constraints on the Superfluid Chaplygin gas model
• Holographic dilatonic model of dark energy
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• The effect of inhomogeneities on dark energy constraints
• Wiggly cosmic strings accrete dark energy
• Baryogenesis and the New Cosmology
• The Hierarchy Problem and the Cosmological Constant Problem Revisited -- A new view on the SM of particle physics
• Emergent Cosmos in Einstein-Cartan Theory
• Solar chameleons: Novel channels
• Wolfgang Priester: from the big bounce to the Lambda-dominated universe
• Virialization of matter overdensities within dark energy subsystems: special cases
• Noether Symmetry Approach in "Cosmic Triad" Vector Field Scenario
• Deformation of Axion Potentials: Implications for Spontaneous Baryogenesis, Dark Matter, and Isocurvature Perturbations
• Supergravity Brane Cosmologies
• Cosmological Condensation of Scalar Fields -- Making a dark energy
• Null tests with Gaussian Process
• Gravitational Origin of Phantom Dark Energy and Late Cosmic Acceleration
• Quintessential early dark energy
• Strong lensing, cosmology and lensing halos
• Constraints on kinematic parameters at $z\ne 0$
• Primordial flat frame -- a new view on inflation
• WMAP Constraints on Quintessence
• Power suppression from disparate mass scales in effective scalar field theories of inflation and quintessence
• Mass-Varying Massive Gravity with k-essence
• Dilaton dominance relaxes LHC and cosmological constraints in supersymmetric models
• Gif Lectures on Cosmic Acceleration
• Applications to cosmological models of a complex scalar field coupled to a U(1) vector gauge field
• Polytropic gas scalar field models of dark energy
• Vacuum energy sequestering and conformal symmetry
• Confronting quintessence models with recent high-redshift supernovae data
• First-order formalism for the quintom model of dark energy
• Wave dynamics of phantom scalar perturbation in the background of Schwarzschild black hole
• On the holographic dark energy in chameleon scalar-tensor cosmology
• Early universe in quantum gravity
• General parametrization for energy density of quintessence field
• The Dark Energy Cosmic Clock: A New Way to Parametrise the Equation of State
• Phenomemology of a Realistic Accelerating Universe Using Tracker Fields
• Tachyon model of Tsallis holographic dark energy
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• Cosmography using strong lensing systems and cosmic chronometers
• Warping with dilatation symmetry and self-tuning of the cosmological constant
• The B-L Phase Transition: Implications for Cosmology and Neutrinos
• The non-minimal coupling constant and the primordial de Sitter state
• Interacting holographic tachyon model of dark energy
• Cosmological Constant, Gauge Hierarchy and Warped Geometry
• Non-linear cosmological collapse of quintessence
• The dynamics of coset dimensional reduction
• Late-time acceleration with steep exponential potentials
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
• Imprints of screened dark energy on nonlocal quantum correlations
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• Cosmon Lumps and Horizonless Black Holes
• Covariance of dark energy parameters and sound speed constraints from large HI surveys
• Evolution of magnetic component in Yang-Mills condensate dark energy models
• Leptonic Dark Energy and Baryogenesis
• Inhomogeneous cosmologies with Q-matter and varying $\Lambda$
• Observational constraints upon quintessence models arising from moduli fields
• Cosmological Coincidence without Fine Tuning
• Mirror World with Broken Mirror Parity, E(6) Unification and Cosmology
• Quintessence models with an oscillating equation of state and their potentials
• Dark Energy on Astrophysical Scales and Its Detection in the Milky Way
• A new logotropic model based on a complex scalar field with a logarithmic potential
• The cosmological constant as a boundary term
• Can our Universe be inhomogeneous on large sub-horizon scales ?
• A way to get rid of cosmological constant and zero point energy problems of quantum fields through metric reversal symmetry
• The accelerated scaling attractor solution of the interacting agegraphic dark energy in Brans-Dicke theory
• Extension of non-minimal derivative coupling theory and Hawking radiation in black-hole spacetime
• The Extended Analysis On New Generalized Chaplygin Gas
• A Universe with a generalized ghost dark energy and Van der Waals fluid interacting with a fluid
• Chameleon Fragmentation
• Semi-analytic galaxy formation in coupled dark energy cosmologies
• Testing a dissipative kinetic k-essence model
• Classifying the behavior of noncanonical quintessence
• Viable dark energy models using pseudo-Nambu-Goldstone bosons
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Absence of solid angle deficit singularities in beyond-generalized Proca theories
• Late time cosmic acceleration from natural infrared cutoff?
• First and second order cosmological perturbations in light mass Galileon models
• Ghost dark energy with sign-changeable interaction term
• Effect of low anisotropy on cosmological models by using supernova data
• Exploring evidence of interaction between dark energy and dark matter
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• Non-locality and late-time cosmic acceleration from an ultraviolet complete theory
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Do Bound Structures Brake Cosmic Acceleration?
• A new take on the inflationary quintessence
• The Coincidence Problem and the Swampland Conjectures in the Ijjas-Steinhardt Cyclic Model of the Universe
• General Markovian Equation for Scalar Fields in a Slowly Evolving Background
• Mixed fluid cosmological model in $f(R,T)$ gravity
• Shadows and Optical Appearances of Black Holes in $R^2$ Gravity
• Exit from inflation and a paradigm for vanishing cosmological constant in self-tuning models
• Generalized Model of Interacting Dark Energy and Dark Matter : Phase Portrait Analysis of Evolving Universe
• Qualitative Properties of Magnetic Fields in Scalar Field Cosmology
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Quadratic integrals of a multi-scalar cosmological model
• Exact general solutions for cosmological scalar field evolution in a background-dominated expansion
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• Nonsingular Chaplygin gas cosmologies in universes connected by wormhole
• Standard Model with Cosmologically Broken Quantum Scale Invariance
• Reconstruction of the dark energy scalar field potential by Gaussian process
• Imprints of dynamical dark energy on weak-lensing measurements
• Late-time acceleration in the coupled Cubic Galileon models
• Homogeneous and Isotropic Charge Densities to Accelerate the Universe
• Phantom shell around black hole and global geometry
• Late-time-accelerated expansion arisen from gauge fields in an anisotropic background and a fruitful trick for Noether's approach
• Freezing Out Early Dark Energy
• Scalar field evolution at background and perturbation levels for a broad class of potentials
• The Nature of Dark Energy and Constraints on Its Hypothetical Constituents from Force Measurements
• Gravitational Field Equations and Theory of Dark Matter and Dark Energy
• Non-adiabatic perturbations in Ricci dark energy model
• Mass varying neutrinos with different quintessence potentials
• (An)Isotropic models in scalar and scalar-tensor cosmologies
• Stars disformally coupled to a shift-symmetric scalar field
• The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
• How Slowly can the Early Universe Expand?
• The Universality of Seesaws
• Deformation of the quintom cosmological model and its consequences
• A minimal scale invariant axion solution to the strong CP-problem
• A Parameterized Variable Dark Energy Model: Structure Formation and Observational Constraints
• Degravitation of the Cosmological Constant in Bigravity
• Cosmological Higgs fields
• Non-local scalar fields inflationary mechanism in light of Planck $2013$
• Spherical collapse and cluster number counts in dark energy models disformally coupled to dark matter
• Cosmological constraints on superconducting dark energy models
• Consistency of Cubic Galileon Cosmology: Model-Independent Bounds from Background Expansion and Perturbative Analyses
• Fundamental Cosmology from Precision Spectroscopy: II. Synergies with supernovae
• Constraints on Late Time Violations of the Equivalence Principle in the Dark Sector
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• Scalar Field Kantowski--Sachs Solutions in Teleparallel $F(T)$ Gravity
• Thermodynamical description of modified generalized Chaplygin gas model of dark energy
• Spacetime and Planck mass generation from scale-invariant degenerate gravity
• Accelerating expansion of the universe may be caused by inhomogeneities
• Non-local dilaton coupling to dark matter: cosmic acceleration and pressure backreaction
• Cosmology with higher-derivative matter fields
• Effective scalar potential in asymptotically safe quantum gravity
• Scalar field inflation and Shan-Chen fluid models
• FeynMG: a FeynRules extension for scalar-tensor theories of gravity
• Quintessential inflation and nonlinear effects of the tachyonic trap mechanism
• APPLIED COSMOGRAPHY: A Pedagogical Review
• Astrophysical and electromagnetic emissivity properties of black holes surrounded by a quintessence type exotic fluid in the Scalar-Vector-Tensor Modified Gravity
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Frozen-in fermionic singlet dark matter in non-standard cosmology with a decaying fluid
• Early dark energy constraints on growing neutrino quintessence cosmologies
• High-precision spectra for dynamical Dark Energy cosmologies from constant-w models
• Left-Right Symmetric Model of Neutrino Dark Energy
• A particle's perspective on screening mechanisms
• Old Dark Energy
• On the Effective Equation of State of Dark Energy
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• The Hamiltonian formalism for scalar fields coupled to gravity in a cosmological background
• On Dark Energy Isocurvature Perturbation
• A possible role for the merger of clusters/voids in the cosmological expansion
• "Expansion" around the vacuum: how far can we go from Lambda?
• Dynamical evolution of phantom scalar perturbation in the background of Schwarzschild black String spacetime
• Interacting dark energy collapse with matter components separation
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Scaling solution for field-dependent gauge couplings in quantum gravity
• The effect of curvature in thawing models
• The entangled accelerating universe
• Mass varying dark matter in effective GCG scenarios
• The variation of the electromagnetic coupling and quintessence
• High accuracy power spectra including baryonic physics in dynamical Dark Energy models
• Statefinder analysis of the superfluid Chaplygin gas model
• Bianchi {VI}${}_0$ in Scalar and Scalar-Tensor Cosmologies
• Complementarity of Future Dark Energy Probes
• The Spin Alignments in Galaxy Pairs as a Test of Bouncing Coupled Dark Energy
• Chameleon gravity on cosmological scales
• Novel aspects of C-theories in Cosmology
• Observational constraints on G-corrected holographic dark energy using a Markov chain Monte Carlo method
• Dark Energy from holographic theories with hyperscaling violation
• Probing Quintessence Potential with Future Cosmological Surveys
• Inflation driven by q-de Sitter
• Quintessence and phantom emerging from the split-complex field and the split-quaternion field
• Curvature Singularity in f(R) Theories of Gravity
• A cosmological model of the early universe based on ECG with variable $\Lambda$-term in Lyra geometry
• Crossing of the Cosmological Constant Boundary - an Equation of State Description
• Friedmann-Robertson-Walker Models with Late-Time Acceleration
• The unphysical character of dark energy fluids
• Cosmological cancellation of the vacuum energy density
• From Swampland to Phenomenology and Back
• Nonlinear structure formation in Bound Dark Energy
• Reconstruction and exact solutions for cosmological perturbations from a generalized gravity theory
• Dark matter and Standard Model reheating from conformal GUT inflation
• Dark Matter and Dark Energy from a Kaluza-Klein inspired Brans-Dicke Gravity with Barotropic Fluid
• The Grand Canonical Multiverse and the Small Cosmological Constant
• Electroweak symmetry breaking by gravity
• Sensitivity of quintessence perturbations to initial conditions
• Phase-space analysis of torsion-coupled dilatonic ghost condensate
• Dynamical system analysis in modified Galileon cosmology
• Cosmological Dynamics in Interacting Scalar-Torsion f(T,$\varphi$) Gravity: Investigating Energy and Momentum Couplings
• Cosmic superstrings in large volume compactifications: PTAs, LISA and time-varying tension
• Supersymmetric Models For Gauge Inflation
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Scalar field source Teleparallel Robertson-Walker F(T)-gravity solutions
• Probing extra dimensions through cosmological observations of dark energy
• $\Lambda$ is Coming: Parametrizing Freezing Fields
• Observational constraints on the unified dark matter and dark energy model based on the quark bag model
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Backreaction in Growing Neutrino Quintessence
• New holographic Chaplygin gas model of dark energy
• Interacting Three Fluid System and Thermodynamics of the Universe Bounded by the Event Horizon
• Dynamics of entropy perturbations in assisted dark energy with mixed kinetic terms
• Cosmological acceleration from a gas of strings
• Dark Energy with a Fine-toothed Comb
• The Matrix Reloaded - on the Dark Energy Seesaw
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• Constraints for warped branes
• Cosmic Evolution with Early and Late Acceleration Inspired by Dual Nature of the Ricci Scalar Curvature
• Fate of homogeneous ${\mathbb{Z}}_2$-symmetric scalar condensates
• The Matter Power Spectrum of Dark Energy Models and the Harrison-Zel'dovich Prescription
• Gauge Invariant Perturbation Analysis for Quintessence with an Exponential Potential
• The torsion cosmology in Kaluza-Klein theory
• DBI analog of a decaying vacuum cosmology
• Is Quintessence an Indication of a Time-Varying Gravitational Constant?
• Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
• Phenomenological models of Universe with varying $G$ and $\Lambda$
• The coincidence problem in $f(R)$ gravity models
• A scalar field dark matter model and its role in the large scale structure formation in the Universe
• Observational constraints using Bayesian statistics and Deep Learning in $f(Q)$ gravity
• Variable $G$ Correction for Dark Energy Model in Higher Dimensional Cosmology
• Non-Gaussianity of the density distribution in accelerating universes
• Accretion of Holographic Dark Energy : Dependency only upon Horizon Radius of Expanding Universe
• Dynamics of Multi-Component, Multi-Field Quintessence
• Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
• Slow-Roll Inflation in the Presence of a Dark Energy Coupling
• Interacting Viscous Dark Energy in Bianchi Type-III Universe
• Big bang nucleosynthesis as a probe of fundamental "constants"
• A new generic and structurally stable cosmological model without singularity
• Joint constraint on primordial gravitational waves and polarization rotation angle with current CMB polarization data
• Mimicking the LCDM model with Stealths
• Cosmology and the Hubble Constant: On the Megamaser Cosmology Project (MCP)
• Fine Tuning Problem of the Cosmological Constant in a Generalized Randall-Sundrum Model
• Nature of Dark Energy and Polarization Measurements
• $f(R)$ Dual Theories of Quintessence : Expansion-Collapse Duality
• Non-Linearly Interacting Ghost Dark Energy in Brans-Dicke Cosmology
• Estimations of the cosmological parameters from the observational variation of the fine structure constant
• Cosmological Unification, Dark Energy and the Origin of Neutrino Mass
• Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff
• Constraints on Holographic cosmologies from strong lensing systems
• Naturalness and stability of the generalized Chaplygin gas in the seesaw cosmon scenario
• Cyclic universe due to phantom and quintessence
• Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
• The Quadratic Approximation for Quintessence with Arbitrary Initial Conditions
• Constraining the runaway dilaton and quintessential dark energy
• D-bound and Bekenstein bound for McVittie solution surrounded by dark energy cosmological fields
• Teleparallel Gravity and Quintessence: The Role of Nonminimal Boundary Couplings
• Spinor quintom cosmology with intrinsic spin
• Entropic considerations on the Universe and Universe-Black Hole Systems
• Realizing the phantom-divide crossing with vector and scalar fields
• Pseudo Newtonian Potential For a Rotating Kerr Black Hole Embedded in Quintessence
• Analytic Study of Cosmological Perturbations in a Unified Model of Dark Matter and Dark Energy with a Sharp Transition
• Dark Energy Accretion onto Van der Waal's Black Hole
• Bifurcated symmetry breaking in scalar-tensor gravity
• Compactifications of conformal gravity
• Early dark energy in the pre- and post-recombination epochs
• From inflation to dark energy in scalar-tensor cosmology
• Avoiding parameter fine-tuning in mass varying neutrino models of DE?
• Higgs-dilaton model revisited: can dilaton act as QCD axion?
• Non-linear Matter Spectrum for a Variable Equation of State
• Theory of interacting vector dark energy and fluid
• Scaling attractors for quintessence in flat universe with cosmological term
• Hamiltonian study of the Generalized scalar-tensor theory with potential in a Bianchi type I model
• Variational symmetries and superintegrability in multifield cosmology
• A Kaluza-Klein Inspired Brans-Dicke Gravity with Dark Matter and Dark Energy Model
• Crossing the Big Bang singularity
• Transient weak gravity in scalar-tensor theories
• No-scale Brans-Dicke Gravity -- ultralight scalar boson & heavy inflaton
• Observational constraints on a Yang-Mills condensate dark energy model
• Analytical considerations about the cosmological constant and dark energy
• Effective field theory of coupled dark energy and dark matter
• Diagnostic Approaches for Interacting generalized holographic Ricci Dark Energy Models
• Spinor gravity and diffeomorphism invariance on the lattice
• Inflation is the generic feature of phantom field-not the big-rip
• Raychaudhuri-based reconstruction of anisotropic Einstein-Maxwell equation in 1+3 covariant formalism of $f(R)$-gravity
• Cosmology: a bird's eye view
• Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
• Dynamical system analysis in descending dark energy model
• Neutrino Lorentz invariance violation from the CPT-even SME coefficients through a tensor interaction with cosmological scalar fields
• Mimetic Weyl geometric gravity
• Rigorous derivation of dark energy and inflation as geometry effects in Covariant Canonical Gauge Gravity
• Dilaton-induced variations in Planck constant and speed of light: An alternative to Dark Energy
• Lectures on Naturalness, String Landscape and Multiverse
• Preheating and Dark Sector of Universe
• Stabilizing dark matter with quantum scale symmetry
• Power-law solutions for TeVeS
• Coupling active and sterile neutrinos in the cosmon plus seesaw framework
• Time dependent dark energy and the thermodynamics of many-body systems
• D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole
• Runaway potentials and a massive goldstino
• Cosmic scalar fields with flat potential
• Top-Hat Spherical Collapse with Clustering Dark Energy. I. Radius Evolution and Critical Contrast Density
• Dark Energy from pNGB Mediated Dirac Neutrino Condensate
• Coupling q-deformed dark energy to dark matter
• Relating the cosmological constant and slow roll to conformal symmetry breaking
• The Electroweak Axion, Dark Energy, Inflation and Baryonic Matter
• Complex supergravity quintessence models confronted with Sn Ia data
• Non-relativistic matter and Dark energy in a quantum conformal model
• Observed Cosmological Reexpansion in Minimal QFT with Bose and Fermi Fields
• A quantized frequency reference in the short-ranged gravity potential and its application for dark matter and dark energy searches
• Classical and quantum quintessence cosmology
• The expansion of the universe observed with supernovae
• Phenomenologically varying $\Lambda$ and a toy model for the Universe
• G-corrected holographic dark energy model
• A Model of Large Quintessence Isocurvature Fluctuations and Low CMB Quadrupole
• Bimodal/Schizophrenic Neutrino As a Bridge between Inflation and Dark Energy
• (Non-) geodesic motion in chameleon Brans Dicke model
• Axions in Cold Dark Matter and Inflation Models
• Phenomenology of Hybrid Scenarios of Neutrino Dark Energy
• The electromagnetic coupling and the dark side of the Universe
• Potentials of Coupled Quintessence Based on a Dilaton
• B-L-symmetric Baryogenesis with Leptonic Quintessence
• Phantom scalar emission in the Kerr black hole spacetime
• The Fourth Gravity Test and Quintessence Matter Field
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Vacuum Energy and Renormalization of the Field-Independent Term
• Neutrino Dark Energy in Grand Unified Theories
• Screening fifth forces in scalar-vector-tensor theories
• Observational constraints on thawing quintessence scalar field model
• Cosmological volume acceleration in dust epoch: using scaling solutions and variable cosmological term $\Lambda (t)$ within an anisotropic cosmological model
• Gravitational relaxation of electroweak hierarchy problem
• Dilatons for Dense Hadronic Matter
• Observational constraints and differential diagnosis for cosmic evolutionary models
• Tackling tangledness of cosmic strings by knot polynomial topological invariants
• Quantum tunneling driven by quintessence and the role of GUP
• A new single-dynamical-scalar-field model of dark energy
• Coupled Dark Energy field variation
• On possible composite structure of scalar fields in expanding universe
• Toy models of Universe with an Effective varying $\Lambda$-Term in Lyra Manifold
• Can Chameleon fields be the source of both the dark energy dipole and the CMB dipole?
• On Conformal Transformation with Multiple Scalar Fields and Geometric Property of Field Space with Einstein-like Solutions
• Impact of inhomogeneities on slowly rolling Quintessence: implications for the local variations of the fine-structure constant
• Single scalar cosmology
• Evolution of perturbations in a universe with exotic solid-like matter
• The nature of cosmological singularities in isotropic universes and braneworlds
• Interacting dark fluid in the universe bounded by event horizon : A non-equilibrium prescription
• A mechanism to generate varying speed of light via Higgs-dilaton coupling: Theory and cosmological applications
• Supergravity models of Quintessence and Supersymmetry breaking
• Dark energy from conformal symmetry breaking
• DESI constraints on two-field quintessence with exponential potentials
• Exact solution and exotic fluid in cosmology
• New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
• Dark Energy in vector-tensor theories of gravity
• Phenomenological aspects of dark energy dominated cosmologies
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• On the F-term problem and quintessence supersymmetry breaking
• Dark energy without fine tuning
• Quintessence, Supersymmetry and Inflation
• Interacting Models of Generalised Chaplygin Gas and Modified Chaplygin Gas with Barotropic Fluid
• Cosmological viability of a double field unified model from warm inflation
• Higgs potential near-criticality from a de Sitter swampland-like condition
• How does Inflation Depend Upon the Nature of Fluids Filling Up the Universe in Brane World Scenario
• Interaction between Tachyon and Hessence (or Hantom) dark energies
• Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature
• Scalar field dark energy and Cosmic Microwave Background
• Interacting Dark Energy and Its Implications for Unified Dark Sector
• An effective description of dark energy: from theory to phenomenology
• Early Tracking Behavior in Small-field Quintessence Models
• Characterising Dark Energy through supernovae
• f(R) cosmological solutions with varying speed of light
• UV-complete and stable Quintom Dark Energy models in the light of DESI DR2
• Dynamics of scalar fields in an expanding/contracting cosmos at finite temperature
• Impact of a Rapid Diluted Energy Density on the halo mass function
• A new approach to modified-gravity models
• K-Inflation with a Dark Energy Coupling
• Cosmic Acceleration Caused by the Extra-Dimensional Evolution in a Generalized Randall-Sundrum Model
• Scalar field models for an accelerating universe
• Parameterization and Reconstruction of Quasi Static Universe
• Effect of Moduli Redefinitions on Fibre Inflation
• Renormalization Group Approach to Generalized Cosmological models
• Dark energy constraints in light of theoretical priors
• Higgs-Induced Screening Mechanisms in Scalar-Tensor Theories
• Perturbations of Einstein--Maxwell--phantom spacetime: Instabilities of charged Ellis--Bronnikov wormholes and quasinormal modes of black holes
• Dynamical dark energy in the no-scale Brans-Dicke gravity
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Scalar Field Static Spherically Symmetric Solutions in Teleparallel $F(T)$ Gravity
• Is the cosmological dark sector better modeled by a generalized Chaplygin gas or by a scalar field?
• Tracking through equality
• Theory Challenges of the Accelerating Universe
• Structure Formation in Dynamical Dark Energy Models
• Gravity of Cosmological Perturbations in the CMB
• Gravity and induced matter on Nearly Kahler Manifolds
• Quintessence and false vacuum: Two sides of the same coin?
• Agegraphic dark energy from entropy of the anti-de Sitter black hole
• Can dark energy explain a high growth index?
• Non-linear structure formation in the "Running FLRW" cosmological model
• Evolution of the horizons for dark energy universe
• Can a pseudo-symmetry solve the cosmological constant problem?
• Galileon versus Quintessence: A comparative phase space analysis and late-time cosmic relevance
• Can Moduli Fields parametrize the Cosmological Constant?
• A Jacobian generalization of the pseudo Nambu-Goldstone bosons potential
• What is the SUSY mass scale?
• Generic autonomous system approach to interacting dark energy models
• Phase space of multi-fluid universe in $F(T)$-gravity and some enhancements for the oscillating interaction model
• Pure Natural Quintessential Inflation and Dark Energy
• Dark Energy Simulations
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• An introduction to axions and their detection
• Semi-holographic model revisited
• Acceleration of the universe in matter dominant era by conformal symmetry breaking
• Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics
• An analogy between four parametrizations of the dark energy equation of state onto Physical DE Models
• Scaling Cosmologies from Duality Twisted Compactifications
• Electroweak Phase Transitions in Einstein's Static Universe
• Dark Energy: relating the evolution of the universe from the past to the future
• Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology
• Chaplygin and Polytropic gases Teleparallel Robertson-Walker $F(T)$ gravity solutions
• Braneworld wormholes supported by astrophysical observations
• Perturbations In Some Dark Energy Models
• Signature Change in $f(R,T_{\varphi })$ Theory
• Scaling solutions in three-form cosmology
• Neutrino Condensate Dark Energy from TeV Scale Extra Dimensions
• Cosmic evolution of scalar fields with multiple vacua: generalized DBI and quintessence
• Electroweak Quintessence Axion as Dark Energy
• The Limits of Quintessence
• Dynamical dark energy and variation of fundamental "constants"
• Very Light Cosmological Scalar Fields from a Tiny Cosmological Constant
• The Higgs boson, naturalness, and the Universe
• Chaplygin gas halos
• Higgs-Dilaton Inflation in Einstein-Cartan gravity
• Phantom Crossing with Quintom Models
• Linearized Treatment of Scalar perturbations in the Asymptotic Cosmological Model
• Post-Newtonian Constraints on Scalar-Tensor Gravity
• VADER - A Satellite Mission Concept For High Precision Dark Energy Studies
• Constraints on Energy Conditions in $f(R,L_m)$ Gravity
• Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
• Cosmological test of a length-preserving biconnection gravity
• Parametrization of Born-Infeld Type Phantom Dark Energy Model
• On curvature coupling and quintessence fine-tuning
• Power-law and Logarithmic Entropy Corrected Holographic Dark Energy Models in Brans-Dicke Cosmology with Granda-Oliveros Cut-Off
• Bayesian evidence and model selection approach for time-dependent dark energy
• After the Dark Ages
• Observational Constraints and Cosmological Dynamics of Interacting Fractional Holographic Dark Energy in Light of DESI DR2
• Curvature-Assisted Dynamical Compactification in a Pre-Inflationary Higher-Dimensional Universe
• Cosmology in the presence of diffeomorphism-violating, nondynamical background fields
• The creation of radiation and the relic of inflaton potential