Dark Energy

Abstract

We review the problem of dark energy, including a survey of theoretical models and some aspects of numerical studies.

185 pages, 29 figures, 8 tables, more references added. We will continue to update this article, comments and suggestions are welcome

References in corpus (304)

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• Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
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• CfA3: 185 Type Ia Supernova Light Curves from the CfA
• G-inflation: inflation driven by the Galileon field
• A Holographic Dark Energy Model from Ricci Scalar Curvature
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• On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter
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• Constraining f(R) Gravity as a Scalar Tensor Theory
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• The Hubble Diagram to Redshift >6 from 69 Gamma-Ray Bursts
• The morphology of HII regions during reionization
• Large Scale Structure as a Probe of Gravitational Slip
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• Observational constraints on $f(T)$ theory
• f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis
• Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
• The Hubble Constant: A Summary of the HST Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
• High resolution CMB power spectrum from the complete ACBAR data set
• Galileon Cosmology
• Cosmology with Weak Lensing Surveys
• De Sitter Space and Eternity
• Phantom scalar dark energy as modified gravity: understanding the origin of the Big Rip singularity
• A kinematical approach to dark energy studies
• Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
• The future evolution and finite-time singularities in $F(R)$-gravity unifying the inflation and cosmic acceleration
• Holographic dark energy models: A comparison from the latest observational data
• A general test of the Copernican Principle
• Interacting holographic generalized Chaplygin gas model
• Cuscuton: A Causal Field Theory with an Infinite Speed of Sound
• Non-linear Evolution of f(R) Cosmologies III: Halo Statistics
• Observational Tests of Modified Gravity
• Cosmology and Astrophysical Constraints of Gauss-Bonnet Dark Energy
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Detection of the ISW and SZ effects from the CMB-Galaxy correlation
• Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy
• Matter instability in modified gravity
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Solar System tests DO rule out 1/R gravity
• The 2dF-SDSS LRG and QSO Survey: QSO clustering and the L-z degeneracy
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• Nonparametric Dark Energy Reconstruction from Supernova Data
• Growth factor in f(T) gravity
• Observational information for f(T) theories and Dark Torsion
• A Singularity Problem with f(R) Dark Energy
• Confronting Lemaitre-Tolman-Bondi models with Observational Cosmology
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Testing LCDM with the Growth Function δ(a): Current Constraints
• Non-linear evolution of f(R) cosmologies II: power spectrum
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• The 2dF-SDSS LRG and QSO Survey: The LRG 2-Point Correlation Function and Redshift-Space Distortions
• The Dynamics of Quintessence, The Quintessence of Dynamics
• Reconstruction of the deceleration parameter and the equation of state of dark energy
• The Measure Problem in Cosmology
• Evolution of the 21 cm signal throughout cosmic history
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Reconstructing holographic quintessence
• Cosmological Constraints on New Agegraphic Dark Energy
• Relativistic stars in f(R) gravity, and absence thereof
• Potential sources of contamination to weak lensing measurements: constraints from N-body simulations
• X-ray and Sunyaev-Zel'dovich Effect Measurements of the Gas Mass Fraction in Galaxy Clusters
• Systematic Bias in Cosmic Shear: Beyond the Fisher Matrix
• Exact solution to the averaging problem in cosmology
• Holographic probabilities in eternal inflation
• Dark Energy and QCD Ghost
• The matter power spectrum in f(R) gravity
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• A Cosmology-Independent Calibration of Gamma-Ray Burst Luminosity Relations and the Hubble Diagram
• Time drift of cosmological redshifts as a test of the Copernican principle
• Statefinder Diagnosis for Ricci Dark Energy
• The dark matter halos of massive, relaxed galaxy clusters observed with Chandra
• Inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills-$F(R)$ gravity and non-minimal vector-$F(R)$ gravity
• Instability of holographic dark energy models
• Instability of agegraphic dark energy models
• Observational constraints on self-accelerating cosmology
• Weak Lensing Probes of Modified Gravity
• The acceleration of the universe and the physics behind it
• Constraining Interactions in Cosmology's Dark Sector
• On the growth of linear perturbations
• Interacting Agegraphic Dark Energy
• A Test of the Copernican Principle
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• Cosmological Constraints on f(R) Acceleration Models
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Ghosts, Instabilities, and Superluminal Propagation in Modified Gravity Models
• `Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function
• The No-Boundary Measure of the Universe
• Nonparametric Reconstruction of the Dark Energy Equation of State
• On causality and superluminal behavior in classical field theories. Applications to k-essence theories and MOND-like theories of gravity
• Interacting Vector-like Dark Energy, the First and Second Cosmological Coincidence Problems
• A litmus test for Lambda
• CMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe
• The cosmological constant from the ghost. A toy model
• Bouncing Cosmologies in Palatini $f(R)$ Gravity
• Statefinder diagnosis for the interacting model of holographic dark energy
• Mapping the Cosmological Expansion
• Observational constraints on Galileon cosmology
• Living in a Void: Testing the Copernican Principle with Distant Supernovae
• Interacting holographic dark energy
• Matter density perturbations in interacting quintessence models
• Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
• Non-linear Evolution of Matter Power Spectrum in Modified Theory of Gravity
• Dynamical Masses in Modified Gravity
• Large-Scale Tests of the DGP Model
• A cosmic vector for dark energy
• Parametrizations of the Dark Energy Density and Scalar Potentials
• The Growth of Structure in Interacting Dark Energy Models
• Cuscuton Cosmology: Dark Energy meets Modified Gravity
• Reconstructing the Distortion Function for Nonlocal Cosmology
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• A no-go theorem for polytropic spheres in Palatini f(R) gravity
• Density perturbations in general modified gravitational theories
• The dispersion of growth of matter perturbations in f(R) gravity
• Simultaneous Falsification of LCDM and Quintessence with Massive, Distant Clusters
• Constraining dark energy with cross-correlated CMB and Large Scale Structure data
• Cosmic Calibration: Constraints from the Matter Power Spectrum and the Cosmic Microwave Background
• Predicting the Cosmological Constant from the Causal Entropic Principle
• Looking the void in the eyes - the kSZ effect in LTB models
• Axions as Quintessence in String Theory
• Thermodynamics in $F(R)$ gravity with phantom crossing
• $f(T)$ Theories and Varying Fine Structure Constant
• Ghost conditions for Gauss-Bonnet cosmologies
• Top ten accelerating cosmological models
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• Observational constraints on the linear fluctuation growth rate
• Can we avoid dark energy?
• Age Problem in the Holographic Dark Energy Model
• Gauge-invariant analysis of perturbations in Chaplygin gas unified models of dark matter and dark energy
• Power-laws f(R) theories are cosmologically unacceptable
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• DBI-essence
• Some Issues Concerning Holographic Dark Energy
• Eternal Inflation: The Inside Story
• Cosmological implications of Karolyhazy uncertainty relation
• Predicting the cosmological constant with the scale-factor cutoff measure
• Precision cosmology defeats void models for acceleration
• Constraints on the Sound Speed of Dynamical Dark Energy
• Growth factor parametrization and modified gravity
• Dark Energy Model with Spinor Matter and Its Quintom Scenario
• Backreaction: directions of progress
• Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
• On holographic dark-energy models
• Relic gravitational waves and their detection
• Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test
• Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
• The behavior of $f(R)$ gravity in the solar system, galaxies and clusters
• Present and future evidence for evolving dark energy
• Effects of dark sectors' mutual interaction on the growth of structures
• Relic Gravitational Waves in the Accelerating Universe
• Dynamical and Gravitational Instability of Oscillating-Field Dark Energy and Dark Matter
• Can higher curvature corrections cure the singularity problem in f(R) gravity?
• Scale dependence of cosmological backreaction
• Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae
• Are We Typical?
• Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
• Secondary anisotropies of the CMB
• Entropy-Corrected Holographic Dark Energy
• The Possibility of Cosmic Acceleration via Spatial Averaging in Lemaitre-Tolman-Bondi Models
• Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• Delicate f(R) gravity models with disappearing cosmological constant and observational constraints on the model parameters
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• Cosmic Acceleration, Dark Energy and Fundamental Physics
• Populating the Landscape: A Top Down Approach
• Bounding the mass of the graviton with gravitational waves: Effect of higher harmonics in gravitational waveform templates
• Curvature singularities, tidal forces and the viability of Palatini f(R) gravity
• Re-examination of Polytropic Spheres in Palatini f(R) Gravity
• Cosmological constraints from COMBO-17 using 3D weak lensing
• On the curvature of the present-day Universe
• Inflation with Holographic Dark Energy
• Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
• Growth Index of DGP Model and Current Growth Rate Data
• Lookback time as a test for brane cosmology
• Luminosity distance in "Swiss cheese" cosmology with randomized voids: I. Single void size
• Comparison of Standard Ruler and Standard Candle constraints on Dark Energy Models
• The influence of structure formation on the cosmic expansion
• The Cosmic Microwave Background in an Inhomogeneous Universe - why void models of dark energy are only weakly constrained by the CMB
• Physics of dark energy particles
• The effect of modified gravity on weak lensing
• Dark Energy in Practice
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• Dark Energy: Recent Developments
• Quintessence reconstructed: new constraints and tracker viability
• Distance, Growth Factor, and Dark Energy Constraints from Photometric Baryon Acoustic Oscillation and Weak Lensing Measurements
• Reconciling the local void with the CMB
• Analytic spectrum of relic gravitational waves modified by neutrino free streaming and dark energy
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• From Cavendish to PLANCK: Constraining Newton's Gravitational Constant with CMB Temperature and Polarization Anisotropy
• Reconstructing the Cosmic Expansion History up to Redshift z=6.29 with the Calibrated Gamma-Ray Bursts
• An exact analytic spectrum of relic gravitational waves in an accelerating universe
• 2-loop Quantum Yang-Mills Condensate as Dark Energy
• Measuring deviations from a cosmological constant: a field-space parameterization
• Revisit of cosmic age problem
• Fitting the Constitution SNIa Data with Redshift Binned Parameterization Method
• Cheng-Weyl Vector Field and its Cosmological Application
• Growth factor parametrization in curved space
• Yang-Mills condensate dark energy coupled with matter and radiation
• Cosmological perturbations in the DGP braneworld: numeric solution
• (No) Eternal Inflation and Precision Higgs Physics
• Systematic effects in the sound horizon scale measurements
• Ruling out the Modified Chaplygin Gas Cosmologies
• Cosmic Parallax: possibility of detecting anisotropic expansion of the universe by very accurate astrometry measurements
• Scalar Field Dark Energy Perturbations and their Scale Dependence
• The LambdaCDM model on the lead -- a Bayesian cosmological models comparison
• Realizing Scale-invariant Density Perturbations in Low-energy Effective String Theory
• Dark energy, the colored anti-de Sitter vacuum, and LHC phenomenology
• Cosmic age problem revisited in the holographic dark energy model
• Dynamically avoiding fine-tuning the cosmological constant: the "Relaxed Universe"
• Is Our Universe Decaying at an Astronomical Rate?
• Invariance under complex transformations, and its relevance to the cosmological constant problem
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• The Cosmic Microwave Background for Pedestrians: A Review for Particle and Nuclear Physicists
• Speed of Sound in the Mass Varying Neutrinos Scenario
• Eternal inflation predicts that time will end
• De Sitter brane-world, localization of gravity, and the cosmological constant
• Narrowing Constraints with Type Ia Supernovae: Converging on a Cosmological Constant
• Holographic Gas as Dark Energy
• Constraining the evolution of dark energy with type Ia supernovae and gamma-ray bursts
• Remarks on Dynamical Dark Energy Measured by the Conformal Age of the Universe
• Spectral Energy Distributions and Age Estimates of 39 Globular Clusters in M31
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• Exploring the Latest Union2 SNIa Dataset by Using Model-Independent Parametrization Methods
• Cosmological Constant from Decoherence
• Constraining DGP Gravity from Observational Data
• Evolution of Dark Energy Perturbations in Scalar-Tensor Cosmologies
• Gamma-ray burst afterglows
• Gamma-Ray Bursts are Produced Predominately in the Early Universe
• Is the Dynamics of Tracking Dark Energy Detectable?
• Modifications by QCD transition and $e^{+}{e}^{-}$ annihilation on analytic spectrum of relic gravitational waves in accelerating universe
• Three-Point Correlations in f(R) Models of Gravity
• Supernovae and Cosmology
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• Structure Formation, Backreaction and Weak Gravitational Fields
• Crossing of Phantom Divide in $F(R)$ Gravity
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• Searching for modified gravity with baryon oscillations: from SDSS to wide field multiobject spectroscopy (WFMOS)
• Unparticle dark energy
• Indistinguishable Macroscopic Behaviour of Palatini Gravities and General Relativity
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• Metric gravity theories and cosmology:II. Stability of a ground state in f(R) theories
• Constraining the interacting dark energy models from weak gravity conjecture and recent observations
• PHotometry Assisted Spectral Extraction (PHASE) and identification of SNLS supernovae
• Eternal Chaotic Inflation is Prohibited by Weak Gravity Conjecture
• Can cosmic acceleration be caused by exotic massless particles?
• No resonant tunneling in standard scalar quantum field theory
• Probing the course of cosmic expansion with a combination of observational data
• Measuring Baryon Acoustic Oscillations with Millions of Supernovae
• Signatures of the Baryon Acoustic Oscillations on 21cm Emission Background
• Typicality Derived
• Data analysis methods for the cosmic microwave background
• The Hubble constant and dark energy from cosmological distance measures
• Can the Copernican principle be tested by cosmic neutrino background?
• The warping of extra spaces accelerates the expansion of the universe
• Backreaction of superhorizon perturbations in scalar field cosmologies
• Self-gravitating darkon fluid with anisotropic scaling
• Current cosmological constraints on the curvature, dark energy and modified gravity
• Eternal inflation and localization on the landscape

Cited by in corpus (531)

• Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• f(T) teleparallel gravity and cosmology
• Beyond the Cosmological Standard Model
• WIMP dark matter candidates and searches - current status and future prospects
• Holographic Dark Energy
• Extended Gravity Cosmography
• Cosmology with the Laser Interferometer Space Antenna
• Dark energy two decades after: Observables, probes, consistency tests
• Reconstruction of $f(T)$ gravity: Rip cosmology, finite-time future singularities and thermodynamics
• Bounce cosmology from $F(R)$ gravity and $F(R)$ bigravity
• Cosmography and constraints on the equation of state of the Universe in various parametrizations
• Cosmographic analysis of the equation of state of the universe through Padé approximations
• FRW Cosmology in F(R,T) gravity
• Reconstructing $f(R,T)$ gravity from holographic dark energy
• Early and late universe holographic cosmology from a new generalized entropy
• Barrow entropic dark energy: A member of generalized holographic dark energy family
• The $H_0$ tension in light of vacuum dynamics in the Universe
• Thermodynamics of cosmological horizons in $f(T)$ gravity
• Generalized second law of thermodynamics in f(T) gravity
• A Generalization to the Rastall Theory and Cosmic Eras
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Higher dimensional charged $f(R)$ black holes
• Entropic cosmology for a generalized black-hole entropy
• Phantom Cosmology without Big Rip Singularity
• Inflation, Cosmic Perturbations and Non-Gaussianities
• Noether Symmetry in $f(T)$ Theory
• Wormholes without exotic matter in Einstein-Cartan theory
• Nonlinear structure formation in the Cubic Galileon gravity model
• Weak Gravitational lensing by phantom black holes and phantom wormholes using the Gauss-Bonnet theorem
• Dynamics of Teleparallel Dark Energy
• Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
• Scaling attractors in interacting teleparallel dark energy
• Planck Constraints on Holographic Dark Energy
• Dark goo: Bulk viscosity as an alternative to dark energy
• Matter Bounce Loop Quantum Cosmology from $F(R)$ Gravity
• Dynamics of Inflation and Dark Energy from $F(R,\mathcal{G})$ Gravity
• Linear perturbations in Galileon gravity models
• $f(T)$ cosmology via Noether symmetry
• Generalizing the running vacuum energy model and comparing with the entropic-force models
• Future Cosmological Constraints from Fast Radio Bursts
• Selected topics in scalar-tensor theories and beyond
• Holographic Scalar Fields Models of Dark Energy
• Generalized Second Law of Thermodynamics in $f(T)$ Gravity with Entropy Corrections
• Revisiting Generalized Chaplygin Gas as a Unified Dark Matter and Dark Energy Model
• Matter creation and cosmic acceleration
• Distance Priors from Planck and Dark Energy Constraints from Current Data
• Observational Viability and Stability of Nonlocal Cosmology
• Evolution of the universe in entropic cosmologies via different formulations
• Cosmokinetics: A joint analysis of Standard Candles, Rulers and Cosmic Clocks
• Kerr-Newman-AdS Black Hole Surrounded by Perfect Fluid Matter in Rastall Gravity
• Future singularities and Teleparallelism in Loop Quantum Cosmology
• Disformal couplings and the dark sector of the universe
• Cosmic history of viable exponential gravity: Equation of state oscillations and growth index from inflation to dark energy era
• Cosmological dynamics of tachyonic teleparallel dark energy
• Note on the Evolution of the Gravitational Potential in Rastall Scalar Field Theories
• Cosmological Applications of Pade Approximant
• On the stability of scalar-vacuum space-times
• Bouncing cosmologies with dark matter and dark energy
• Holographic dark energy in the DGP braneworld with GO cutoff
• The parameter space in Galileon gravity models
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Galileon inflation evades the no-go for PBH formation in the single-field framework
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Bianchi Type I Cosmology in Generalized Saez-Ballester Theory via Noether Gauge Symmetry
• A new null diagnostic customized for reconstructing the properties of dark energy from BAO data
• Observational constraints on Rastall's cosmology
• Updated constraints on $f(\mathcal{R})$ gravity from cosmography
• Cosmological Fluids with Logarithmic Equation of State
• Ghost-free $F(R)$ bigravity and accelerating cosmology
• Constraints on barotropic dark energy models by a new phenomenological $q(z)$ parameterization
• Observational constraints on interacting Tsallis holographic dark energy models
• Effect of Varying Bulk Viscosity on Generalized Chaplygin Gas
• The evidence of cosmic acceleration and observational constraints
• Scalar dark energy models mimicking $\Lambda$CDM with arbitrary future evolution
• Revisit of the interacting holographic dark energy model after Planck 2015
• Correspondence between $f(G)$ Gravity and Holographic Dark Energy via Power-law Solution
• Accretion disks around black holes in modified strong gravity
• Constraining f(R) gravity in solar system, cosmology and binary pulsar systems
• Cosmological Perturbations in Unimodular Gravity
• Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations
• Gravitational Lensing by Phantom Black holes
• General form of entropy on the horizon of the universe in entropic cosmology
• Pilgrim Dark Energy in $f(T,T_G)$ cosmology
• Unification of a Bounce with a Viable Dark Energy Era in Gauss-Bonnet Gravity
• Turbulence and Little Rip Cosmology
• Post-$Planck$ constraints on interacting vacuum energy
• Domain Wall Brane in Eddington Inspired Born-Infeld Gravity
• Reconstruction and constraining of the jerk parameter from OHD and SNe Ia observations
• Cosmological observational constraints on the power law $f(Q)$ type modified gravity theory
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Correspondence of cosmology from non-extensive thermodynamics with fluids of generalized equation of state
• Connecting early and late universe by $f(R)$ gravity
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Modified Chaplygin Gas as a Unified Dark Matter and Dark Energy Model and Cosmic Constraints
• Matter Non-conservation in the Universe and Dynamical Dark Energy
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Thermodynamic Behavior of particular $f(R,T)$ Gravity Models
• Nonlinear Chaplygin Gas Cosmologies
• A New Class of Parametrization for Dark Energy without Divergence
• Constraining $f(T)$ Theories with the Varying Gravitational Constant
• Modified cosmology from the thermodynamics of apparent horizon
• Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
• Extended Spherical Collapse and the Accelerating Universe
• Non-adiabatic-like accelerated expansion of the late universe in entropic cosmology
• Holographic f(T)-gravity model with power-law entropy correction
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Interacting Ricci Dark Energy with Logarithmic Correction
• Towards equation of state of dark energy from quasar monitoring: Reverberation strategy
• Exploring uncertainties in dark energy constraints using current observational data with Planck 2015 distance priors
• Gravitational wave constraints on Lorentz and parity violations in gravity: high-order spatial derivative cases
• Constraints on the Nieh-Yan modified teleparallel gravity with gravitational waves
• Geometrization of light bending and its application to SdSw spacetime
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Extended Birkhoff's Theorem in the f(T) Gravity
• Primordial non-Gaussianity from ultra slow-roll Galileon inflation
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• The cosmology in f(R,T) gravity without dark energy
• Unified description of the dynamics of quintessential scalar fields
• Constraining interacting dark energy with CMB and BAO future surveys
• The transient acceleration from time-dependent interacting dark energy models
• Null test for interactions in the dark sector
• Entropic cosmology in a dissipative universe
• Early dark energy in $k$-essence
• Cosmic acceleration from modified gravity with Palatini formalism
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Holographic realization from inflation to reheating in generalized entropic cosmology
• On the road to percent accuracy V: the non-linear power spectrum beyond $\Lambda$CDM with massive neutrinos and baryonic feedback
• $\Lambda$CDM Bounce Cosmology without $\Lambda$CDM: the case of modified gravity
• Holographic dark matter and dark energy with second order invariants
• Constructing a cosmological model-independent Hubble diagram of type Ia supernovae with cosmic chronometers
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Singularity Problem in Teleparallel Dark Energy Models
• Unified Dark Fluid with Constant Adiabatic Sound Speed and Cosmic Constraints
• Teleparallel Dark Energy with Purely Non-minimal Coupling to Gravity
• Possible antigravity regions in $F(R)$ theory?
• Reissner-Nordström Black Holes in Mimetic $F(R)$ Gravity
• Apparent horizon and gravitational thermodynamics of the Universe: Solutions to the temperature and entropy confusions, and extensions to modified gravity
• Statefinder hierarchy model for the Barrow holographic dark energy
• Growth of matter perturbations in clustered holographic dark energy cosmologies
• Notes on teleparallel cosmology with nonminimally coupled scalar field
• Probing cosmic opacity at high redshifts with gamma-ray bursts
• Testing dark energy models with a new sample of strong-lensing systems
• Generalized second law of thermodynamics in scalar-tensor gravity
• Direct Probe of Dark Energy through Gravitational Lensing Effect
• Constraining the Asymptotically Safe Cosmology: cosmic acceleration without dark energy
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• The generalized second law of gravitational thermodynamics on the apparent horizon in f(R)-gravity
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Superbounce and Loop Quantum Cosmology Ekpyrosis from Modified Gravity
• Holographic thermalization and gravitational collapse in the spacetime dominated by quintessence dark energy
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Back-Reaction of Super-Hubble Cosmological Perturbations Beyond Perturbation Theory
• Beyond-one-loop quantum gravity action yielding both inflation and late-time acceleration
• Quasi-Rip: A New Type of Rip Model without Cosmic Doomsday
• New Graviton Mass Bound from Binary Pulsars
• QCD ghost f(T)-gravity model
• A Comparative Study of Dark Energy Constraints from Current Observational Data
• Cosmological Hysteresis and the Cyclic Universe
• Cosmic evolution of dark energy in a generalized Rastall gravity
• Post-Newtonian parameters and cosmological constant of screened modified gravity
• Confronting the relaxation mechanism for a large cosmological constant with observations
• Realisation of the ultra-slow roll phase in Galileon inflation and PBH overproduction
• Constraints on a $\varphi$CDM model from strong gravitational lensing and updated Hubble parameter measurements
• Binary Black Hole merger in f(R) theory
• Generalized holographic dark energy model described at the Hubble length
• Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
• Confronting dark energy models mimicking $\Lambda$CDM epoch with observational constraints: future cosmological perturbations decay or future Rip?
• Viscous Dark Energy In Bianchi Type V Space-Time
• Exact spherically-symmetric inhomogeneous model with n perfect fluids
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• Holographic Dark Energy with Cosmological Constant
• Cosmological model-independent test of $\Lambda$CDM with two-point diagnostic by the observational Hubble parameter data
• Tsallis holographic dark energy in Fractal Universe
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Dynamical dark energy
• Bianchi Type $I$ Cosmology in $f(R,T)$ Gravity
• A Note on Schwarzschild de Sitter Black Holes in Mimetic $F(R)$ Gravity
• Consistency of Modified Gravity with a decreasing $G_{\mathrm{eff}}(z)$ in a $\Lambda$CDM background
• New Generalizations of Cosmography Inspired by the Pade Approximant
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Cosmological implications of an interacting model of dark matter \& dark energy
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Universal thermodynamics in different gravity theories: Modified entropy on the horizons
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Tsallis holographic dark energy for inflation
• Evidence for cosmic acceleration with next-generation surveys: A model-independent approach
• Mass varying neutrinos, symmetry breaking, and cosmic acceleration
• Holographic, new agegraphic and ghost dark energy models in fractal cosmology
• Thermodynamics and dark energy
• Post-Planck Dark Energy Constraints
• A comprehensive numerical study on four categories of holographic dark energy models
• Testing the Cosmic Anisotropy with Supernovae Data: Hemisphere Comparison and Dipole Fitting
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• A comprehensive investigation on the slowing down of cosmic acceleration
• Domain wall solution in $F(R)$ gravity and variation of the fine structure constant
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Bayesian evidence for $\alpha$-attractor dark energy models
• Bianchi type I cosmological models in Eddington-inspired Born-Infeld gravity
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Constraining Logotropic Unified Dark Energy Models
• Cosmological Constraints on Variable Warm Dark Matter
• Uncertainty on w from large-scale structure
• Stability of accelerating cosmology in two scalar-tensor theory: Little Rip versus de Sitter
• Evolution of spherical overdensities in holographic dark energy models
• Large fluctuations and Primordial Black Holes
• Non-parametric dark energy reconstruction using the tomographic Alcock-Paczynski test
• A systematic procedure to build the beyond generalized Proca field theory
• Holographic realization of constant roll inflation and dark energy: An unified scenario
• When is the growth index constant?
• Detecting the cosmic acceleration with current data
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Probing the physical and mathematical structure of $f(R)$ gravity by PSR $J0348+0432$
• Planar Symmetry in f(T) gravity
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• Global behavior of cosmological dynamics with interacting Veneziano ghost
• Searching for a matter bounce cosmology with low redshift observations
• Fractional dark energy
• A global fit study on the new agegraphic dark energy model
• Dark Energy and Equation of State Oscillations with Collisional Matter Fluid in Exponential Modified Gravity
• How universe evolves with cosmological and gravitational constants
• Generalized Holographic Dark Energy and its Observational Constraints
• Growth Index after the Planck Results
• Cosmological Constant, Fine Structure Constant and Beyond
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• On dark energy models of single scalar field
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Strong gravitational lensing constraints on holographic dark energy
• A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short $\gamma$-ray bursts
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• On An Interacting New Holographic Dark Energy Model: observational constraints
• Reconstruction of an Observationally Constrained $f(R,T)$ gravity model
• Reconstructing the History of Energy Condition Violation from Observational Data
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Cuscuton kinks and branes
• Cosmic slowing down of acceleration using $f_{gas}$
• Weak-field limit of f(R)-gravity in three and more spatial dimensions
• Asymptotically Lifshitz black hole solutions in F(R) gravity
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Phenomenological models for Unified Dark Matter with fast transition
• Cosmological dark energy effects from entanglement
• Scrutinizing Various Phenomenological Interactions In The Context Of Holographic Ricci Dark Energy Models
• Spherical collapse in the extended quintessence cosmological models
• An interacting New Holographic Dark Energy in the framework of fractal cosmology
• Effective Dark Energy Models and Dark Energy Models with Bounce in frames of $F(T)$ Gravity
• Interacting modified holographic Ricci dark energy model and statefinder diagnosis in flat universe
• A new holographic dark energy model in Brans-Dicke theory with logarithmic scalar field
• A note on interacting holographic dark energy with a Hubble-scale cutoff
• Statefinder diagnosis for the extended holographic Ricci dark energy model without and with interaction
• Constraints on dark energy from the Lyα forest baryon acoustic oscillations measurement of the redshift 2.3 Hubble parameter
• Methodological Reflections on the MOND/Dark Matter Debate
• Onset of acceleration in a Universe initially filled by dark and baryonic matters in nonminimally coupled teleparallel model
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Effective dark energy equation of state in interacting dark energy models
• Gravitational Dust Collapse in $f(R)$ Gravity
• Generation of large-scale magnetic fields from inflation in teleparallelism
• A solution of the dark energy and its coincidence problem based on local antigravity sources without fine-tuning or new scales
• Quantum deformation of quantum cosmology: A framework to discuss the cosmological constant problem
• Post-Newtonian parameters of ghost-free parity-violating gravities
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• Little Rip cosmological models with time-dependent equation of state
• Thermodynamical description of the ghost dark energy model
• Anisotropic $k$-essence
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Cosmological aspects of $f(R,T)$ gravity in a simple model with a parametrization of $q$
• Cosmological perturbations and dynamical analysis for interacting quintessence
• $f(R)$ gravity modifications: from the action to the data
• Strong lensing modeling in galaxy clusters as a promising method to test cosmography I. Parametric dark energy models
• Cosmological Constant Problem and Renormalized Vacuum Energy Density in Curved Background
• Cosmology in Poincare gauge gravity with a pseudoscalar torsion
• Cosmography of interacting generalized QCD ghost dark energy
• Black Hole Formation with an Interacting Vacuum Energy Density
• Cosmological evolution of equation of state for dark energy in G-essence models
• Bianchi type II models in the presence of perfect fluid and anisotropic dark energy
• Vainshtein mechanism in Gauss-Bonnet gravity and Galileon aether
• Cosmological model with time varying deceleration parameter in $F(R,G)$ gravity
• Robust constraints on dark energy and gravity from galaxy clustering data
• Loop Quantum Cosmology Matter Bounce Reconstruction from $F(R)$ Gravity Using an Auxiliary Field
• Equation-of-state formalism for dark energy models on the brane and the future of brane universes
• Diagnosing $\Lambda$HDE model with statefinder hierarchy and fractional growth parameter
• Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2
• The general property of dynamical quintessence field
• Constraints on the exponential $f(R)$ model from latest Hubble parameter measurements
• New Scalar Field Quartessence
• More Evidence for the Redshift Dependence of Color from the JLA Supernova Sample Using Redshift Tomography
• Latest data constraint of some parameterized dark energy models
• Anisotropic cosmological models with two fluids
• The unified history of the viscous accelerating universe and phase transitions
• Model-Independent Measurements of Cosmic Expansion and Growth at z=0.57 Using the Anisotropic Clustering of CMASS Galaxies From the Sloan Digital Sky Survey Data Release 9
• Indistinguishability of Warm Dark Matter, Modified Gravity, and Coupled Cold Dark Matter
• The generalized second law of thermodynamics for interacting $f(R)$ gravity
• Late Time Cosmological Evolution in f(R) theories with Ordinary and Collisional Matter
• Natural Braneworld Inflation in Light of Recent Results from Planck and BICEP2
• Maximum turnaround radius in $f(R)$ gravity
• Cosmological constant Petrov type-N space-time in Ricci-inverse gravity
• On the effect of the degeneracy between w_0 and w_a
• Alcock-Paczynski Test with the Evolution of Redshift-Space Galaxy Clustering Anisotropy
• Interacting Tsallis holographic dark energy in higher dimensional Cosmology
• Cosmological constraints on the new holographic dark energy model with action principle
• Coupling dark energy to dark matter inhomogeneities
• Constraining Thawing Quintessence
• A critical assessment of some inhomogeneous pressure Stephani models
• Thawing Versus. Tracker Behaviour: Observational Evidence
• Cosmological Models Coupled with Dark Matter in a Dissipative Universe
• On Bianchi type III Cosmological Model with Quadratic EoS in Lyra Geometry
• Constraints to Holographic Dark Energy Model via Type Ia Supernovae, Baryon Acoustic Oscillation and WMAP
• Generalized Galileon Model -- cosmological reconstruction and the Vainshtein mechanism --
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• Constraints on the dark matter sound speed from galactic scales: the cases of the Modified and Extended Chaplygin Gas
• On detecting interactions in the dark sector with H(z) data
• Birkhoff's Theorem in f(T) Gravity up to the Perturbative Order
• R\' enyi Holographic Dark Energy in Higher Dimension Cosmology
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Estimating the uncorrelated dark energy evolution in the Planck era
• Comparing dark energy models with current observational data
• Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
• Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
• Holographic Dark Energy Characterized by the Total Comoving Horizon and Insights to Cosmological Constant and Coincidence Problem
• The tension on the cosmological parameters from different observational data
• Constraints on Dark Energy Models Using Late Universe Probes
• Multi-component DHOST analysis in galaxy clusters
• A Dark Energy Model in Lyra Manifold
• Periodic Cosmological Evolutions of Equation of State for Dark Energy
• Exact Cosmological Solutions of $f(R)$ Theories via Hojman Symmetry
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• Singular Accelerated Evolution in Massive $F(R)$ Bigravity
• Thawing quintessence from the inflationary epoch to today
• The redshift dependence of Alcock-Paczynski effect: cosmological constraints from the current and next generation observations
• A Born-Infeld-like f(R) gravity
• Cosmological constraints from low-redshift data
• Holographic Dark Energy Model Characterized by the Conformal-age-like Length
• Cosmological constraints on holographic dark energy models under the energy conditions
• Kriging Interpolating Cosmic Velocity Field
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Constraining f(R) theories with cosmography
• Observing the dark sector
• Cosmography with the Sunyaev-Zeldovich effect and X-ray data
• Universal thermodynamics in different gravity theories: Conditions for generalized second law of thermodynamics and thermodynamical equilibrium on the horizons
• Global properties of the growth index of matter inhomogeneities in the universe
• New holographic dark energy model inspired by the DGP braneworld
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• Reconstructing a non-linear interaction in the dark sector with cosmological observations
• Neutrino generated dynamical dark energy with no dark energy field
• Dark effects in $f(R,P)$ gravity
• Observational tests of backreaction with recent data
• Statefinder diagnostic of logarithmic entropy corrected holographic dark energy with Granda-Oliveros IR cut-off
• Varying constants entropic--$\Lambda$CDM cosmology
• Generalized second law of thermodynamics in QCD ghost f(G) gravity
• A Study of Universal Thermodynamics in Brane World Scenario
• Interacting generalized ghost dark energy in non-flat universe
• (m,n)-type holographic dark energy models
• Causality Problem in a Holographic Dark Energy Model
• Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology
• Interacting holographic dark energy models: A general approach
• It's a dark, dark world: Background evolution of interacting $\varphi$CDM models beyond simple exponential potentials
• Study of QCD generalized ghost dark energy in FRW universe
• Revisiting the Cosmological Constant Problem within Quantum Cosmology
• Figure of Merit and Different Combinations of Observational Data Sets
• Can Back-Reaction Prevent Eternal Inflation?
• Hubble-rate-dependent Dark Energy in Brans-Dicke Cosmology
• Null tests with Gaussian Process
• Quantum computational complexity, Einstein's equations and accelerated expansion of the Universe
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• Interacting dark energy in the dark $SU(2{)}_R$ model
• Holographic Dark Energy and Quantum Entanglement
• Global properties of the growth index: mathematical aspects and physical relevance
• Cosmological Constraint and Analysis on Holographic Dark Energy Model Characterized by the Conformal-age-like Length
• DBI Galileon and Late time acceleration of the universe
• Stable phantom-divide crossing in two scalar models with matter
• Observational Constraints on Axions as Quintessence in String Theory
• Cosmological Model of Interacting Tachyon Field
• Observational Constraints on Varying Alpha in $\Lambda (\alpha )$CDM Cosmology
• Interacting viscous entropy-corrected holographic scalar field models of dark energy with time-varying G in modified FRW cosmology
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Unified dark matter and dark energy description in a chiral cosmological model
• Data-driven and Almost Model-independent Reconstruction of Modified Gravity
• Holographic Λ(t)CDM model in a non-flat universe
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• Dark Energy on Astrophysical Scales and Its Detection in the Milky Way
• On the emergence of the $\mathbf{\Lambda }$CDM model from self-interacting Brans-Dicke theory in $\mathbf{d}=5$
• The cosmological constant filter without big bang singularity
• Running vacuum model in non-flat universe
• Entanglement inside the cosmological apparent horizon
• Kriging interpolating cosmic velocity field. II. Taking anistropies and multistreaming into account
• Nonlinearities in modified gravity cosmology. II. Impacts of modified gravity on the halo properties
• Dynamical System of Scalar Field from 2-Dimension to 3-D and its Cosmological Implication
• Application of the Abel Equation of the 1st kind to an inflation analysis of non-exactly solvable cosmological models
• Dynamical reconstruction of the $\Lambda$CDM model in hybrid metric-Palatini gravity
• Power Law Entropy Corrected New-Agegraphic Dark Energy in Hořava-Lifshitz Cosmology
• Hojman Symmetry in $f(T)$ Theory
• Knot Universes in Bianchi Type I Cosmology
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Constraints on thawing scalar field models from fundamental constants
• Thermodynamical analysis on a braneworld scenario with curvature corrections
• Non-minimally Coupled Tachyon Field in Teleparallel Gravity
• Late time cosmic acceleration from natural infrared cutoff?
• Fundamental Physics and Cosmology with TianQin
• Thermodynamic analysis of universes with the initial and final de-Sitter eras
• Cosmological implications of different baryon acoustic oscillation data
• Probing departures from $\Lambda$CDM by late-time datasets
• Clustering GCG: a viable option for unified dark matter-dark energy?
• Dark energy in thermal equilibrium with the cosmological horizon?
• Cosmological evolutions in Tsujikawa model of $f(R)$ Gravity
• Turbulence Accelerating Cosmology from an Inhomogeneous Dark Fluid
• Electrodynamic phenomena induced by a dark fluid: Analogs of pyromagnetic, piezoelectric, and striction effects
• The Distinguishability of Interacting Dark Energy from Modified Gravity
• Reconstruction of the equation of state for the cyclic universes in homogeneous and isotropic cosmology
• Holographic dark energy in the DGP model
• Study on the mapping of halo clustering from real space to redshift space
• Dark Energy and Cosmological Horizon Thermal Effects
• Nonstandard approach to gravity for the dark sector of the Universe
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• There is no vacuum zero-point energy in our universe for massive particles within the scope of relativistic quantum mechanics
• Cosmological and Particle Physics Constraints on a New Non-Abelian SU(3) Gauge Model for Ordinary/Dark Matter Interaction
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Sampling the Probability Distribution of Type Ia Supernova Lightcurve Parameters in Cosmological Analysis
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Spinor Walls in Five-Dimensional Warped Spacetime
• Ricci Flow Approach to The Cosmological Constant Problem
• A numerical approach to model independently reconstruct $f(R)$ functions through cosmographic data
• Thermodynamical description of modified generalized Chaplygin gas model of dark energy
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Toward a more stringent test of gravity with redshift space power spectrum: simultaneous probe of growth and amplitude of large-scale structure
• Gauss-Bonnet dark energy on Hořava-Lifshitz cosmology
• Observational constraints on Tsallis holographic dark energy with Ricci horizon cutoff
• Investigating the Possibility of a Turning Point in the Dark Energy Equation of State
• Chi-square versus median statistics in SNIa data analysis
• Observational constraints to a unified cosmological model
• Holographic Dark Energy from the Anti-de Sitter Black Hole
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Fourier space analysis
• Gödel and Gödel-type solutions in the Palatini $f(R,T)$ gravity theory
• Limit on the dark matter mass from its interaction with photons
• Scalar-Torsion Mode in a Cosmological Model of the Poincaré Gauge Theory of Gravity
• Singularity problem in f(R) model with non-minimal coupling
• Generalized Ghost Dark Energy in DGP Model
• Observational constraints on the unified dark matter and dark energy model based on the quark bag model
• On the consistency of the expansion with the perturbations
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• $\sigma$CDM coupled to radiation. Dark energy and Universe acceleration
• Cosmic acceleration from quantum Friedmann equations
• Dark Energy from Ratio Gravity
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
• Entanglement production in Einstein-Cartan theory
• Dark Energy and Inflation with Volume Normalized Action
• Interacting and Non-interacting Reńyi Holographic Dark Energy Models in DGP Braneworld
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Inflation in non-local hybrid metric-Palatini gravity
• Dark energy effects on realistic neutron stars
• Elucidating the Dark Energy and Dark Matter Phenomena Within the Scale-Invariant Vacuum (SIV) Paradigm
• Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?
• Brane cosmology from observational surveys and its comparison with standard FRW cosmology
• A New Exponential Gravity
• An observational signal of the void shape correlation and its link to the cosmic web
• The coincidence problem in $f(R)$ gravity models
• Interacting dark energy: the role of microscopic feedback in the dark sector
• Effect of dark energy sound speed and equation of state on CDM power spectrum
• Estimations of the cosmological parameters from the observational variation of the fine structure constant
• Structure Formation in the Effective Field Theory of Holographic Dark Energy
• Analysis on a General Class of Holographic Type Dark Energy Models
• The optimal Padé polynomial for reconstruction of luminosity distance based on 10-fold cross-validation
• The Big Trip and Wheeler-DeWitt equation
• Analytic Study of Cosmological Perturbations in a Unified Model of Dark Matter and Dark Energy with a Sharp Transition
• A new analytical approximation of luminosity distance by optimal HPM-Padé technique
• Constraining self-interactions of a massive scalar field using scalar gravitational waves from stellar core collapse
• Implementation of cosmological bounce inflation with Nojiri-Odintsov generalized holographic dark fluid
• A class of regular bouncing cosmologies
• Flat Galactic Rotation Curves from Geometry in Weyl Gravity
• Unified dark matter: constraints from galaxies and clusters
• Influence of the correlation prior on reconstruction of the dark energy equation of state
• Noncommutative cosmological models induced by a symplectic formalism coupled to phantom fluids
• Dark Matter in a bi-metric universe
• Neutrino Lorentz invariance violation from the CPT-even SME coefficients through a tensor interaction with cosmological scalar fields
• Time variation of the Equation of State for Dark Energy
• Assessing the viability of successful reconstruction of the dynamics of dark energy using varying fundamental couplings
• Asymptotic Cosmological Behavior of Scalar-Torsion Mode in Poincare Gauge Theory
• Growth of matter perturbations for realistic $F(R)$ models
• Towards p-Adic Matter in the Universe
• Coupling q-deformed dark energy to dark matter
• Viscous coupled fluids in terms of a log-corrected equation of state
• Probing Cosmic Acceleration by Using Model-Independent Parametrizations and Three Kinds of Supernova Statistics Techniques
• Constraining the swiss-cheese IR-fixed point cosmology with cosmic expansion
• Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection
• Tomographic Alcock-Paczynski Method with Redshift Errors
• Matter Creation Cosmologies and Accelerated Expansion
• Phantom Domain Walls
• Gravitational particle production of superheavy massive particles in Quintessential Inflation: A numerical analysis
• Ferromagnetic instability in PAAI in the sky
• Astrophysical evidence for an extra dimension: phenomenology of a Kaluza Klein theory
• Gravitational wave propagation in generalized hybrid metric-Palatini gravity
• Large Hierarchy from Non-minimal Coupling
• K-essential covariant holography
• Geometric sigma model of the Universe
• A bound system in the expanding universe with modified holographic Ricci dark energy and dark matter
• Neutrino Interactions with perturbed Rastall Gravity: A Novel Approach to Reducing the Hubble Tension
• Light propagation around a Kerr-like black hole immersed in an inhomogeneous anisotropic plasma in Rastall gravity: Analytical solutions to the equations of motion
• Quantum gravity and the holographic dark energy cosmology
• Energy conditions and constraints on the generalized non-local gravity model
• Higher order mimetic gravity after GW170817
• Universal Entanglement and an Information-Complete Quantum Theory
• Exploring the Latest Pantheon SNIa Dataset by Using Three Kinds of Statistics Techniques
• A Note on Gravitational Memory in F(R)-theories and their Equivalent Scalar-Tensor Theories
• Rényi Holographic Dark Energy Models In Multidimensional Universe
• Dark energy with oscillatory tracking potential: Observational Constraints and Perturbative effects
• The Effects of Spatial Curvature on Cosmic Evolution
• $\Lambda$CDM-like evolution in Einstein-scalar-Gauss-Bonnet gravity
• Game Theory in Cosmology
• Tensor stability in Born-Infeld determinantal gravity
• Gravitational wave from cosmic inflation in a gravity with two small four-derivative corrections
• Cuscuta-Galileon Braneworlds
• Halos of dark energy
• Study of Tachyonic Field and its statefinder diagnostics in Various Scenarios of The Anisotropic Universe
• Avoiding unrealistic priors: the case of dark energy constraints from the time variation of the fine-structure constant
• Cosmological constraints from the density gradient weighted correlation function
• Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
• Cosmological Implications of Thermodynamic Split Conjecture
• On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
• Non-minimally coupled quintessential inflation
• Mystery of the Cosmological Constant
• Thermodynamic Split Conjecture and an Observational Test for Cosmological Entropy
• Future Dark Energy Constraints from Atomic Clocks
• Phase space analysis and cosmography of a two-fluid cosmological model
• Modified Cosmology from Mass-to-Horizon Relation: Background Evolution
• Acceleration from a clustering environment
• On Gauge Theories and Covariant Derivatives in Metric Spaces
• Quintessence reconstruction of interacting HDE in a non-flat universe
• Phantom BTZ Black Holes: Thermal Properties Under Perturbative Corrections
• Scalar perturbations of Galileon cosmologies in the mechanical approach within the late Universe
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions