Dark Energy and the Accelerating Universe

Abstract

The discovery ten years ago that the expansion of the Universe is accelerating put in place the last major building block of the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark energy. At the same time, it posed one of the most profound mysteries in all of science, with deep connections to both astrophysics and particle physics. Cosmic acceleration could arise from the repulsive gravity of dark energy -- for example, the quantum energy of the vacuum -- or it may signal that General Relativity breaks down on cosmological scales and must be replaced. We review the present observational evidence for cosmic acceleration and what it has revealed about dark energy, discuss the various theoretical ideas that have been proposed to explain acceleration, and describe the key observational probes that will shed light on this enigma in the coming years.

Invited review for Annual Reviews of Astronomy and Astrophysics; 53 pages, 18 figures

References in corpus (134)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• 4D Gravity on a Brane in 5D Minkowski Space
• A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Cosmological Constant - the Weight of the Vacuum
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• The Cosmological Constant
• Exploring the Expansion History of the Universe
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• Is Cosmic Speed-Up Due to New Gravitational Physics?
• Phantom Energy and Cosmic Doomsday
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Cosmological Constraints from the SDSS Luminous Red Galaxies
• Quantization of Four-form Fluxes and Dynamical Neutralization of the Cosmological Constant
• Can the dark energy equation-of-state parameter w be less than -1?
• Type Ia Supernova Explosion Models
• Quintessence and the Rest of the World
• Constraining Cosmological Parameters Based on Relative Galaxy Ages
• Cosmology with the Sunyaev-Zel'dovich Effect
• Cluster Abundance Constraints on Quintessence Models
• Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters
• Cosmology on a Brane in Minkowski Bulk
• Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2
• Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
• The large-scale structure of the Universe
• Cosmic Microwave Background Anisotropies
• Reconstructing Dark Energy
• Jerk, snap, and the cosmological equation of state
• Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
• CDM Models with a Smooth Component
• Detection of weak gravitational lensing distortions of distant galaxies by cosmic dark matter at large scales
• Intrinsic alignment-lensing interference as a contaminant of cosmic shear
• Detection of Weak Gravitational Lensing by Large-scale Structure
• A MaxBCG Catalog of 13,823 Galaxy Clusters from the Sloan Digital Sky Survey
• Precision Determination of the Mass Function of Dark Matter Halos
• Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler
• The Large Scale Structure of f(R) Gravity
• Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
• Cross-correlation Tomography: Measuring Dark Energy Evolution with Weak Lensing
• Probing the dark energy: methods and strategies
• Prospects for probing the dark energy via supernova distance measurements
• Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys
• Is There A Cosmological Constant?
• Systematic Errors in Future Weak Lensing Surveys: Requirements and Prospects for Self-Calibration
• The Cosmological Constant is Back
• Cosmological parameters from lensing power spectrum and bispectrum tomography
• Dark matter maps reveal cosmic scaffolding
• Uncorrelated Estimates of Dark Energy Evolution
• A correlation of the cosmic microwave sky with large scale structure
• Future Supernovae observations as a probe of dark energy
• The ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry
• Parameterization of Dark-Energy Properties: a Principal-Component Approach
• Cosmological Parameter Extraction from the First Season of Observations with DASI
• Cosmology with Weak Lensing Surveys
• How to determine an effective potential for a variable cosmological term
• Improved forecasts for the baryon acoustic oscillations and cosmological distance scale
• Short GRB and binary black hole standard sirens as a probe of dark energy
• A kinematical approach to dark energy studies
• BVRI Light Curves for 29 Type Ia Supernovae
• An inhomogeneous alternative to dark energy?
• Effect of Photometric Redshift Uncertainties on Weak Lensing Tomography
• Type Ia Supernova Explosion: Gravitationally Confined Detonation
• On cosmic acceleration without dark energy
• First cosmic shear results from the Canada-France-Hawaii Telescope Wide Synoptic Legacy Survey
• Dynamical Lambda Models of Structure Formation
• Joint Galaxy-Lensing Observables and the Dark Energy
• Correlated Fluctuations in Luminosity Distance and the (Surprising) Importance of Peculiar Motion in Supernova Surveys
• Weak Lensing and Dark Energy
• Cross-Correlation of the Cosmic Microwave Background with the 2MASS Galaxy Survey: Signatures of Dark Energy, Hot Gas, and Point Sources
• Redshifting Rings of Power
• Dark Synergy: Gravitational Lensing and the CMB
• Self Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum and Mass Measurements
• Early Dark Energy Cosmologies
• The Dynamics of Quintessence, The Quintessence of Dynamics
• Differentiating between Modified Gravity and Dark Energy
• The Integrated Sunyaev-Zeldovich Effect as the Superior Method for Measuring the Mass of Clusters of Galaxies
• A Local Void and the Accelerating Universe
• Early-universe constraints on a Primordial Scaling Field
• Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data
• Measuring Cosmology with Supernovae
• The Impact of Galaxy Formation on the Sunyaev-Zeldovich Effect of Galaxy Clusters
• Potential sources of contamination to weak lensing measurements: constraints from N-body simulations
• A model independent approach to the dark energy equation of state
• Lemaitre-Tolman-Bondi model and accelerating expansion
• The acceleration of the universe and the physics behind it
• Towards a More Standardized Candle Using GRB Energetics and Spectra
• The X-Ray Luminosity--Mass Relation for Local Clusters of Galaxies
• `Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function
• Improved Cosmological Constraints from Gravitational Lens Statistics
• Type Ia Supernovae, Evolution, and the Cosmological Constant
• The Case for an Accelerating Universe from Supernovae
• Two Windows on Acceleration and Gravitation: Dark Energy or New Gravity?
• What Do We Really Know About Cosmic Acceleration?
• Dark Energy Constraints from Weak Lensing Cross-Correlation Cosmography
• Gamma-Ray Burst Hubble Diagram to z=4.5
• Self-Calibration of Cluster Dark Energy Studies: Counts in Cells
• Probing quintessence: reconstruction and parameter estimation from supernovae
• Dust Versus Cosmic Acceleration
• Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey
• Dark Energy Constraints from the CTIO Lensing Survey
• Detection of correlated galaxy ellipticities on CFHT data: first evidence for gravitational lensing by large-scale structures
• Determining the Equation of State of the Expanding Universe: Inverse Problem in Cosmology
• Measuring Dark Energy Clustering with CMB-Galaxy Correlations
• Completeness in Weak Lensing Searches for Clusters
• Shear Selected Cluster Cosmology I: Tomography and Optimal Filtering
• Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models
• Future Evolution of Structure in an Accelerating Universe
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• A Geometrical Test of the Cosmological Energy Contents Using the Lyman-alpha Forest
• Probing Dark Energy with Supernovae: Exploiting Complementarity with the Cosmic Microwave Background
• A New Perspective on DGP Gravity
• Future Evolution of Nearby Large-Scale Structure in a Universe Dominated by a Cosmological Constant
• Global Cosmological Parameters Determined Using Classical Double Radio Galaxies
• Updated Estimates of Global Cosmological Parameters Determined Using Classical Double Radio Galaxies
• The Return of a Static Universe and the End of Cosmology
• Evaluating Dark Energy Probes using Multi-Dimensional Dark Energy Parameters
• Growth Rate of Large Scale Structure as a Powerful Probe of Dark Energy
• Systematic effects in the sound horizon scale measurements
• Cosmological Parameters from the SDSS DR5 Velocity Dispersion Function of Early-Type Galaxies through Radio-Selected Lens Statistics
• Constraints on Dark Energy Models from Galaxy Clusters with Multiple Arcs
• CMB Cluster Lensing: Cosmography with the Longest Lever Arm
• Testing cosmological models and understanding cosmological parameter determinations with metaparameters

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• Five-dimensional generalized $f(R)$ gravity with curvature-matter coupling
• Model selection and constraints from Holographic dark energy scenarios
• The evolution of the [OII], Hβ and [OIII] emission-line luminosity functions over the last nine billions years
• Post-Newtonian parameters and cosmological constant of screened modified gravity
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Dynamics of a parametrized dark energy model in $f(R,T)$ gravity
• Combining cluster number counts and galaxy clustering
• Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles
• Constraints on a $\varphi$CDM model from strong gravitational lensing and updated Hubble parameter measurements
• Characterizing the linear growth rate of cosmological density perturbations in an f(R) model
• Neutrino Oscillations, Lorentz/CPT Violation, and Dark Energy
• Post-Newtonian constraints on Lorentz-violating gravity theories with a MOND phenomenology
• A Synthetic Roman Space Telescope High-Latitude Imaging Survey: Simulation Suite and the Impact of Wavefront Errors on Weak Gravitational Lensing
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• The growth factor of matter perturbations in an f(R) gravity
• Cosmological model-independent test of $\Lambda$CDM with two-point diagnostic by the observational Hubble parameter data
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Holographic Dark Energy with Cosmological Constant
• New Generalizations of Cosmography Inspired by the Pade Approximant
• Induced cosmological constant and other features of asymmetric brane embedding
• On the $c^2$ term in the holographic formula for dark energy
• Probing the dynamics of dark energy with divergence-free parametrizations: A global fit study
• Gravitational waves and geometrical optics in scalar-tensor theories
• The quantum realm of the "Little Sibling" of the Big Rip singularity
• Reconstructing the Properties of Dark Energy using Standard Sirens
• Supernova light-curve fitters and Dark Energy
• Cosmological Constant from Decoherence
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Evolution of Dark Energy Perturbations in Scalar-Tensor Cosmologies
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Umbrella sampling: a powerful method to sample tails of distributions
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Electrostatic accelerometer with bias rejection for Gravitation and Solar System physics
• The solution of the cosmological constant problem from the inhomogeneous equation of state - a hint from modified gravity?
• Remarks on the properties of elliptical galaxies in modified Newtonian dynamics
• Initiation of the detonation in the gravitationally confined detonation model of Type Ia supernovae
• Scalar field and time varying Cosmological constant in $f(R,T)$ gravity for Bianchi type-I Universe
• Accelerating Universe with spacetime torsion but without dark matter and dark energy
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• Loop quantum Brans-Dicke cosmology
• Bianchi Type I model of universe with customized scale factors
• Barotropic fluid compatible parametrizations of dark energy
• Testing the Cosmic Anisotropy with Supernovae Data: Hemisphere Comparison and Dipole Fitting
• The Galactic Center as a laboratory for theories of gravity and dark matter
• Direction Dependence in Supernova Data: Constraining Isotropy
• A comprehensive numerical study on four categories of holographic dark energy models
• Reconstructing the potentials for the quintessence and tachyon dark energy, from the holographic principle
• Wormhole on the Brane with Ordinary Matter: The Broader View
• Exploring the Hubble tension with a late time Modified Gravity scenario
• Background cosmological dynamics in $f(R)$ gravity and observational constraints
• Reconstruction of GR cosmological solutions in modified gravity theories
• Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Radial pulsations, moment of inertia and tidal deformability of dark energy stars
• Proton Mass Decomposition and Hadron Cosmological Constant
• Quantum vacuum, dark matter, dark energy and spontaneous supersymmetry breaking
• Analysing dissipative effects in the $\Lambda$CDM model
• Modeling the Phase-Space Distribution around Massive Halos
• Cosmological Constraints on Variable Warm Dark Matter
• Constraining Logotropic Unified Dark Energy Models
• Distance Measurements from Supernovae and Dark Energy Constraints
• Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces
• Testing the spherical evolution of cosmic voids
• Dark Energy and Dark Matter unification via superfluid Chaplygin gas
• Localized D-dimensional global k-defects
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• Future dark energy constraints from measurements of quasar parallax: Gaia, SIM and beyond
• Stability of Effective Thin-shell Wormholes Under Lorentz Symmetry Breaking Supported by Dark Matter and Dark Energy
• Gravitational lens effect of a holonomy corrected Schwarzschild black hole
• Interacting Ricci-like holographic dark energy
• Producing a BOSS-CMASS sample with DES imaging
• Exact Solution for Chameleon Field, Self-Coupled Through the Ratra-Peebles Potential with n = 1 and Confined Between Two Parallel Plates
• Testing modified gravity via Yukawa potential in two body problem: Analytical solution and observational constraints
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• The Higgs boson -- its implications and prospects for future discoveries
• The Corona Borealis supercluster: connectivity, collapse, and evolution
• Effective four-dimensional loop quantum black hole with a cosmological constant
• Growth of matter overdensities in non-minimal torsion-matter coupling theories
• Next generation design and prospects for CANNEX
• Generalized Holographic Dark Energy and its Observational Constraints
• Model-Independent Reconstruction of the Expansion History of the Universe from Type Ia Supernovae
• Measuring growth index in a universe with sterile neutrinos
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• A global fit study on the new agegraphic dark energy model
• Computing model independent perturbations in dark energy and modified gravity
• Observational Constraints on Dynamical Dark Energy Models
• A search for the variation of speed of light using galaxy cluster gas mass fraction measurements
• Reconstruction of new holographic scalar field models of dark energy in Brans-Dicke Universe
• Prospects for Searching Thermal Effects, Non-Newtonian Gravity and Axion-Like Particles: Cannex Test of the Quantum Vacuum
• Cosmological Constant, Fine Structure Constant and Beyond
• Anthropic versus cosmological solutions to the coincidence problem
• On dark energy models of single scalar field
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• Generalized supersymmetric cosmological term in N=1 Supergravity
• Cosmological tests of an axiverse-inspired quintessence field
• Model independent constraints on mass-varying neutrino scenarios
• Cosmological dynamics of $f(R)$ gravity scalar degree of freedom in Einstein frame
• The impact of baryons on the sensitivity of dark energy measurements
• Vacuum energy and the cosmological constant
• Chandra Follow-Up of the SDSS DR8 redMaPPer Catalog Using the MATCha Pipeline
• Asymptotically Lifshitz black hole solutions in F(R) gravity
• Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Anisotropic quark stars in $f(R,L_m,T)$ gravity
• Perturbations in a scalar field model with virtues of $\Lambda$CDM
• On An Interacting New Holographic Dark Energy Model: observational constraints
• Cosmic slowing down of acceleration using $f_{gas}$
• Using the Topology of Large Scale Structure to constrain Dark Energy
• The Accelerating Universe
• Non-Uniform Cosmological Birefringence and Active Galactic Nuclei
• A search for sterile neutrinos in interacting dark energy models using DESI baryon acoustic oscillations and DES supernovae data
• Spontaneous symmetry breaking in cosmos: The hybrid symmetron as a dark energy switching device
• Boson mixing and flavor vacuum in the expanding Universe: a possible candidate for the dark energy
• Neutron stars in Einstein-$\Lambda$ gravity: the cosmological constant effects
• Constraints on CDM cosmology from galaxy power spectrum, CMB and SNIa evolution
• Scrutinizing Various Phenomenological Interactions In The Context Of Holographic Ricci Dark Energy Models
• Dynamical Systems Analysis of K-essence Model
• Domain wall network evolution in (N+1)-dimensional FRW universes
• An interacting New Holographic Dark Energy in the framework of fractal cosmology
• Dynamics and constraints of the Unified Dark Matter flat cosmologies
• Fixed points and FLRW cosmologies: Flat case
• Estimation of Cosmological Parameters, Stability Analysis and Energy Conditions in Viable Modified Gravity
• Exploring hints for dark energy density evolution in light of recent data
• Globally visible singularity in an astrophysical setup
• The Averaging Problem in Cosmology
• Modeling cosmic acceleration with a generalized varying deceleration parameter
• Note on the Cardoso-Pani-Rico parametrization to test the Kerr black hole hypothesis
• Archimedean-type force in a cosmic dark fluid: I. Exact solutions for the late-time accelerated expansion
• Constraints on Dark Energy and Modified Gravity models by the Cosmological Redshift Drift test
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• Effective Dark Energy Models and Dark Energy Models with Bounce in frames of $F(T)$ Gravity
• Loop Quantum Brans-Dicke Theory
• Asymmetric wormholes in Palatini $f(\mathcal{R})$ gravity: Energy conditions, absorption and quasibound states
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Gravitational Dust Collapse in $f(R)$ Gravity
• Quintessence and tachyon dark energy models with a constant equation of state parameter
• Modified arctan-gravity model mimicking a cosmological constant
• Cosmological constraints from Radial Baryon Acoustic Oscillation measurements and Observational Hubble data
• Post-Newtonian parameters of ghost-free parity-violating gravities
• Galaxy Clusters as a probe of early dark energy
• Effective dark energy equation of state in interacting dark energy models
• Spherical Accretion of Matter by Charged Black Holes on f(T) Gravity
• Constraints on galileons from the positions of supermassive black holes
• Imprints of interacting dark energy on cosmological perturbations
• Searching for systematics in SNIa and galaxy cluster data using the cosmic duality relation
• Study of the charged super-Chandrasekhar limiting mass white dwarfs in the $f(R,\mathcal{T})$ gravity
• PeV IceCube signals and Dark Matter relic abundance in modified cosmologies
• Cosmology in Poincare gauge gravity with a pseudoscalar torsion
• Spherical `Top-Hat' Collapse in general Chaplygin gas dominated universes
• Consistency Test of Dark Energy Models
• Black Hole Formation with an Interacting Vacuum Energy Density
• Cosmological and Solar-System Tests of f(R) Modified Gravity
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• $f(R)$ gravity modifications: from the action to the data
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Can Cosmic Parallax Distinguish Between Anisotropic Cosmologies?
• Archimedean-type force in a cosmic dark fluid: II. Qualitative and numerical study of a multistage Universe expansion
• Probing modified gravity via the mass-temperature relation of galaxy clusters
• The traces of anisotropic dark energy in light of Planck
• de Sitter as a Resonance
• Diagnosing $\Lambda$HDE model with statefinder hierarchy and fractional growth parameter
• Hartle-Hawking boundary conditions as Nucleation by de Sitter Vacuum
• Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2
• Scalar-tensor cosmologies with dust matter in the general relativity limit
• New Scalar Field Quartessence
• Principal components of dark energy with SNLS supernovae: the effects of systematic errors
• Magnification as a Tool in Weak Lensing
• Cosmological model with time varying deceleration parameter in $F(R,G)$ gravity
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• A New Type of Dark Energy Model
• Confronting Tracker Field Quintessence with Data
• Evidence for strong progenitor age dependence of type Ia supernova luminosity standardization process
• More Evidence for the Redshift Dependence of Color from the JLA Supernova Sample Using Redshift Tomography
• Indistinguishability of Warm Dark Matter, Modified Gravity, and Coupled Cold Dark Matter
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• Quintessence versus phantom dark energy: the arbitrating power of current and future observations
• Formation of caustics in Dirac-Born-Infeld type scalar field systems
• $\Lambda (t)$CDM Model as a Unified Origin of Holographic and Agegraphic Dark Energy Models
• $2.6M_{\odot }$ Compact Object and Neutron Stars within Eddington-Inspired Born-Infeld Theory of Gravity
• Observational constraints on scalar field models of dark energy with barotropic equation of state
• Latest data constraint of some parameterized dark energy models
• 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
• Stringent Pulsar Timing Bounds on Light Scalar Couplings to Matter
• Constraints on dark energy models from radial baryon acoustic scale measurements
• Dark matter and dark energy induced by condensates
• Asymmetry in the reconstructed deceleration parameter
• Generalized cosmological term in D=4 supergravity from a new AdS-Lorentz superalgebra
• On exponential modified gravity
• The PAU Survey: A Forward Modeling Approach for Narrow-band Imaging
• The role of curvature in the slowing down acceleration scenario
• Large-scale structure in mimetic Horndeski gravity
• Cosmological constraints on the new holographic dark energy model with action principle
• Observed galaxy power spectrum in cubic Galileon model
• Delta-gravity and Dark Energy
• Geodesics of McVittie Spacetime with a Phantom Cosmological Background
• Evolution of domain wall networks: the PRS algorithm
• Cosmological evolution of thermal relic particles in $f(R)$ gravity
• Reconstruction of late-time cosmology using Principal Component Analysis
• A Test of the Standard Cosmological Model with Geometry and Growth
• Holographic dark energy described at the Hubble length
• Probing dark matter interactions with 21cm observations
• Scalar perturbations in the late Universe: viability of the Chaplygin gas models
• Generalized scalar-tensor theory of gravity reconstruction from physical potentials of a scalar field
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• Cosmological Information from the Small-scale Redshift Space Distortions
• Structure formation in dark energy cosmologies described by PADE parameterization
• The Maxwell-Chern-Simons gravity and its cosmological implications
• Late-time acceleration in Higher Dimensional Cosmology
• Quasinormal Modes and Topological Characteristics of a Schwarzschild Black Hole Surrounded by the Dehnen Type Dark Matter Halo
• Vacuum Solution of a Linear Red-Shift Based Correction in $f(R)$ Gravity
• Late-time acceleration and inflation in a Poincaré gauge cosmological model
• Constraints on the dark matter sound speed from galactic scales: the cases of the Modified and Extended Chaplygin Gas
• Cosmological Probes of Structure Growth and Tests of Gravity
• Type Ia supernovae data with scalar-tensor gravity
• Axionic extension of the Einstein-aether theory
• Spherical collapse in Generalized Dark Matter models
• Gauge theory of the Maxwell and semi-simple extended (anti) de Sitter algebra
• Five-dimensional metric $f(R)$ gravity and the accelerated universe
• Impact of string and monopole-type junctions on domain wall dynamics: implications for dark energy
• Electrodynamics of a Cosmic Dark Fluid
• Can cosmic acceleration be caused by exotic massless particles?
• Properties of the exact analytic solution of the growth factor and its applications
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Comparing dark energy models with current observational data
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Consequences of f(R)-theories of gravity on gravitational leptogenesis
• Revisiting a model-independent dark energy reconstruction method
• Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
• QCD ghost dark energy cannot (even roughly) explain the main features of the accepted cosmological paradigm
• Testing the cosmic conservation of photon number with type Ia supernovae and ages of old objects
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Dependence on supernovae light-curve processing in void models
• Nonminimal Einstein-Maxwell-Vlasov-axion model
• An effective theory of accelerated expansion
• Acceleration from Modified Gravity: Lessons from Worked Examples
• Late time acceleration in a slow moving galileon field
• Exact Cosmological Solutions of $f(R)$ Theories via Hojman Symmetry
• Testing modified gravity at large distances with the HI Nearby Galaxy Survey's rotation curves
• Is dark energy evolving?
• Dark sector unifications: dark matter-phantom energy, dark matter -- constant $w$ dark energy, dark matter-dark energy-dark matter
• The evolution of high-density cores of the BOSS Great Wall superclusters
• MOND as a peculiar case of the SIV theory
• SNe Ia as a cosmological probe
• Observational cosmology and the cosmic distance-duality relation
• Dark Matter as a Non-Relativistic Bose-Einstein Condensate with Massive Gravitons
• Solar System Constraints on Scalar Tensor Theories with Non-Standard Action
• Loop quantum gravity and cosmological constant
• Can Dark Energy emerge from quantum effects in compact extra dimension ?
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• Quintom fields from chiral K-essence cosmology
• Incorporating galaxy cluster triaxiality in stacked cluster weak lensing analyses
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Evolution of Primordial Neutrino Helicities in Cosmic Gravitational Inhomogeneities
• Inference for the dark energy equation of state using Type IA supernova data
• Casimir energy of confining large $N$ gauge theories
• Reconstruction of cosmological matter perturbations in Modified Gravity
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Early dark energy constraints with late-time expansion marginalization
• Time evolution of the local gravitational parameters and gravitational wave polarizations in a relativistic MOND theory
• Searches for New Particles Including Dark Matter with Atomic, Molecular and Optical Systems
• Cosmic acceleration from coupling of baryonic and dark matter components: Analysis and diagnostics
• Dark effects in $f(R,P)$ gravity
• Standardizing the Gamma-ray burst as a standard candle and applying to the cosmological probes: constraints on the two-component dark energy model
• Observational tests of backreaction with recent data
• Constraints on the Phase Plane of the Dark Energy Equation of State
• Time Dependent Geometry in Massive Gravity
• It's a dark, dark world: Background evolution of interacting $\varphi$CDM models beyond simple exponential potentials
• Extension of Loop Quantum Gravity to Metric Theories beyond General Relativity
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Evolution of Spherical Overdensity in Thawing Dark energy Models
• Accelerated expansion of the Universe driven by dynamic self-interaction
• The effective Lagrangian of dark energy from observations
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity in Bianchi-I spacetime
• Gravitational entropy of local cosmic voids
• Dynamically Generated Inflationary Lambda-CDM
• Model Breaking Measure for Cosmological Surveys
• Interacting holographic dark energy models: A general approach
• Parametrization for the Scale Dependent Growth in Modified Gravity
• Evolution of superclusters and supercluster cocoons in various cosmologies
• The Noether Symmetry Approach: Foundation and applications. The case of scalar-tensor Gauss-Bonnet gravity
• Dark Energy and Inflation in a Gravitational Wave Dominated Universe
• Dynamical Dark Energy in Minimally Modified Gravity
• Is $w\ne -1$ evidence for a dynamical dark energy equation of state ?
• Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data
• Dynamical evolutin of quintessence dark energy in collapsing dark matter halos
• Exotic Rotational Correlations in Quantum Geometry
• New Tsallis Agegraphic Dark Energy
• Testing anthropic reasoning for the cosmological constant with a realistic galaxy formation model
• Holographic Dark Energy and Quantum Entanglement
• Solar chameleons: Novel channels
• de Sitter Harmonies: Cosmological Spacetimes as Resonances
• Reconstructing the growth index $\gamma$ with Gaussian Processes
• Testing the consistency between cosmological measurements of distance and age
• Cosmological constraints on Agegraphic dark energy in DGP braneworld gravity
• Measuring Space-Time Geometry over the Ages
• First cosmological constraints on the Superfluid Chaplygin gas model
• TASI Lectures on Cosmic Acceleration
• Observational constraints in Delta Gravity: CMB and supernovas
• Holographic reconstruction of the k-essence and dilaton models
• Observational Constraints on Varying Alpha in $\Lambda (\alpha )$CDM Cosmology
• CMB anisotropies induced by tensor modes in Massive Gravity
• Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory
• Friedmann equations for deformed entropic gravity
• Revisiting dark energy models using differential ages of galaxies
• Constraining Perturbative Early Dark Energy with Current Observations
• Comparison of cosmological parameter inference methods applied to supernovae lightcurves fitted with SALT2
• X-ray Clusters of Galaxies as Cosmological Tools
• Reconstructing a Model for Gravity at Large Distances from Dark Matter Density Profiles
• $D=4$ supergravity from the Maxwell-Weyl superalgebra
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• Loop quantum modified gravity and its cosmological application
• Dynamical system approach to scalar-vector-tensor cosmology
• Inflation with explicit parametric connection between General Relativity and Scalar-Tensor gravity
• Neutrino at different epochs of the Friedmann Universe
• The observational constraints on the flat $\varphi$CDM models
• Dynamical System Analysis of Quintessence Models with Exponential Potential -- Revisited
• Tailoring cosmologies in cubic shift-symmetric Horndeski gravity
• Holographic Λ(t)CDM model in a non-flat universe
• Probing new fundamental fields with Extreme Mass Ratio Inspirals
• Dark energy fingerprints in the nonminimal Wu-Yang wormhole structure
• The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys
• Non-minimally Coupled Tachyon Field in Teleparallel Gravity
• Hair-dressing Horndeski: an approach to hairy solutions in cubic Horndeski gravity
• Cosmology in Delta-Gravity
• Whether an enormously large energy density of the quantum vacuum is catastrophic
• A primer on problems and prospects of dark energy
• Emergent Dark Matter in Late Time Universe on Holographic Screen
• On the stability of the dark energy based on generalized uncertainty principle
• On the emergence of the $\mathbf{\Lambda }$CDM model from self-interacting Brans-Dicke theory in $\mathbf{d}=5$
• Some models of holographic dark energy on the Randall-Sundrum brane and observational data
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Testing a dissipative kinetic k-essence model
• Skewness as a probe of Baryon Acoustic Oscillations
• $\Lambda$CDM as a Noether Symmetry in Cosmology
• Age problem in holographic dark energy
• Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius
• Classification of the FRW universe with a cosmological constant and a perfect fluid of the equation of state $p=w\rho$
• Non-integer (or fractional) power model of a viral spreading: application to the COVID-19
• Application of the Abel Equation of the 1st kind to an inflation analysis of non-exactly solvable cosmological models
• Israel-Stewart approach to viscous dissipative extended holographic Ricci dark energy dominated universe
• Action Principle for Scale Invariance and Applications (Part I)
• Light propagation with non-minimal couplings in a two-component cosmic dark fluid with an Archimedean-type force and unlighted cosmological epochs
• Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
• Particle Physics at the LHC Start
• Thermodynamical analysis on a braneworld scenario with curvature corrections
• The Scale Factor in the Universe with Dark Energy
• Hojman Symmetry in $f(T)$ Theory
• Lightcone Averaging and Precision Cosmology
• Signature flip in deceleration parameter: A thermodynamic phase transition?
• Testing emergent gravity with mass densities of galaxy clusters
• Analytical solutions of the geodesic equation in the space-time of a black hole surrounded by perfect fluid in Rastall theory
• The Nature of Dark Energy and Constraints on Its Hypothetical Constituents from Force Measurements
• Constraining Models of Dark Energy
• Magnetic Seed and Cosmology as Quantum Hall Effect
• New Equation of Nonrelativistic Physics and Theory of Dark Matter
• Two-field cosmological models and large-scale cosmic magnetic fields
• Gravitational Field Equations and Theory of Dark Matter and Dark Energy
• Stress testing the dark energy equation of state imprint on supernova data
• Black Hole Thermodynamics in Harada's inspired theory of gravity: Stability, Phase Structure and Geometrothermodynamics
• Cosmological twinlike models with multi scalar fields
• The Distinguishability of Interacting Dark Energy from Modified Gravity
• High-z Supernova Type Ia Data: non-Gaussianity and Direction Dependence
• Reconstruction from scalar-tensor theory and the inhomogeneous equation of state in f(T) Gravity
• Dynamical analysis of the Tsallis holographic dark energy models with event horizon as cut-off and interaction with matter
• Fundamental Physics and Cosmology with TianQin
• Unbiased acceleration measurements with an electrostatic accelerometer on a rotating platform
• Reconstruction of the dark energy scalar field potential by Gaussian process
• Average Spectral Properties of Type Ia Supernova Host Galaxies
• Dark Energy and Dark Matter Interaction: Kernels of Volterra Type and Coincidence Problem
• Covariant gauge invariant theory of Scalar Perturbations in $f(R)$-gravity: a brief review
• Dark energy from instantons
• Imprints of dynamical dark energy on weak-lensing measurements
• Generalized entropic gravity from modified Unruh temperature
• Electrodynamic phenomena induced by a dark fluid: Analogs of pyromagnetic, piezoelectric, and striction effects
• Graviton mass due to dark energy as a superconducting medium: theoretical and phenomenological aspects
• Study on the mapping of halo clustering from real space to redshift space
• Deflection and Gravitational lensing of null and timelike signals in the Kiselev black hole spacetime in the weak field limit
• Probing departures from $\Lambda$CDM by late-time datasets
• Generalized particle dynamics: modifying the motion of particles and branes
• Connection Dynamics for Higher Dimensional Scalar-Tensor Theories of Gravity
• Phantom crossing or dark interaction?
• Non-adiabatic perturbations in Ricci dark energy model
• Emulating dark energy models with known equation of state via the created cold dark matter scenario
• Modeling galaxy clustering on small scales to tighten constraints on dark energy and modified gravity
• The Weight of Vacuum Fluctuations
• Null geodesics and observational cosmology
• The role of domain wall junctions in Carter's pentahedral model
• Cosmological Inference from Host-Selected Type Ia Supernova Samples
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Dark Gravitational Field on Riemannian and Sasaki Spacetime
• Precessing Binary Black Holes as Better Dark Sirens
• Investigating the $w$CDM Model with Latest DESI BAO Observations
• Beyond $\Lambda$CDM: Exploring a Dynamical Cosmological Constant Framework Consistent with Late-Time Observations
• Holographic reconstruction of k-essence model with Tsallis and the most generalized Nojiri-Odintsov version of holographic dark energy
• cp3-bench: A tool for benchmarking symbolic regression algorithms tested with cosmology
• Self-calibrating optical galaxy cluster selection bias using cluster, galaxy, and shear cross-correlations
• Toward a more stringent test of gravity with redshift space power spectrum: simultaneous probe of growth and amplitude of large-scale structure
• Interacting dark matter and cosmic acceleration
• Measuring the distances to quasars at high redshifts with strong lensing
• Optimizing galaxy samples for clustering measurements in photometric surveys
• Statistical analysis with cosmic-expansion-rate measurements and two-point diagnostics
• Gauss-Bonnet dark energy on Hořava-Lifshitz cosmology
• Dark Energy and Dark Matter From Hidden Symmetry of Gravity Model with a Non-Riemannian Volume Form
• Sampling the Probability Distribution of Type Ia Supernova Lightcurve Parameters in Cosmological Analysis
• Temperature Structure and Mass-Temperature Scatter In Galaxy Clusters
• Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
• Gravitational instability of the primordial plasma: anisotropic evolution of structure seeds
• Studies on dark energy evolution
• Dynamics of entropy perturbations in assisted dark energy with mixed kinetic terms
• New holographic Chaplygin gas model of dark energy
• Holographic dark information energy: Predicted dark energy measurement
• Quintessential Inflation, Unified Dark Energy and Dark Matter, and Higgs Mechanism
• Sudden Future Singularities in Quintessence and Scalar-Tensor Quintessence Models
• Tachyon field non-minimally coupled to massive neutrino matter
• The Scale Invariant Vacuum Paradigm: Main Results and Current Progress Review (Part II)
• Chi-square versus median statistics in SNIa data analysis
• Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
• Realistic f(T) model describing the de Sitter epoch of the dark energy dominated universe
• Simulation studies of dark energy clustering induced by the formation of dark matter halos
• Beyond the Standard Model of Physics with Astronomical Observations
• Statefinder analysis of the superfluid Chaplygin gas model
• The SM and SUSY after the 2011 LHC results
• Effective Low-Energy Potential for Slow Dirac Fermions in Einstein-Cartan Gravity with Torsion and Chameleon
• Interaction of the axionic dark matter, dynamic aether, spinor and gravity fields as an origin of oscillations of the fermion effective mass
• Novel aspects of C-theories in Cosmology
• Some Adventures in the Search for a Modified Gravity Explanation for Cosmic Acceleration
• Cosmological consequences of a scalar field with oscillating equation of state. III. Unifying inflation with dark energy and small tensor-to-scalar ratio
• Observational constraints on the unified dark matter and dark energy model based on the quark bag model
• The Sun and stars: Giving light to dark matter
• Dynamics of Potentials in Bianchi Type Scalar-Tensor Cosmology
• Chiral Symmetry in Dirac Equation and its Effects on Neutrino Masses and Dark Matter
• Coincidence problem within dark energy as a coupled self-interacting Bose-Einstein gas
• Quasi-spherical superclusters
• The Shared Causal Pasts and Futures of Cosmological Events
• Centenary of Alexander Friedmann's Prediction of the Universe Expansion and the Quantum Vacuum
• Investigating the Possibility of a Turning Point in the Dark Energy Equation of State
• Study of Thermodynamics in Generalized Holographic and Ricci Dark Energy Models
• Constraining Neutrinos and Dark Energy with Galaxy Clustering in the Dark Energy Survey
• Gravitational Forces on a Codimension-2 Brane
• Testing Lambert$W$ equation of state with observational Hubble parameter data
• Cosmological consequences of a scalar field with oscillating equation of state. IV. Primordial nucleosynthesis and the deuterium problem
• Entanglement production in Einstein-Cartan theory
• New Nonrelativistic Quantum Theory of Cold Dark Matter
• Expressing the equation of state parameter in terms of the three dimensional cosmic shear
• Probing Lambda-DGP Braneworld Model
• A Locally Anisotropic Metric for Matter in an Expanding Universe: I. The Ansatz and the Modified Newton Law
• Initial Conditions of Inhomogeneous Universe and the Cosmological Constant Problem
• Conceptual Problems in Cosmology
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)
• Brane cosmology in the Horava-Witten heterotic M-Theory on $S^1/Z_2$
• Electromagnetic Casimir densities for a cylindrical shell on de Sitter space
• Elucidating the Dark Energy and Dark Matter Phenomena Within the Scale-Invariant Vacuum (SIV) Paradigm
• How Much NEC Breaking Can the Universe Endure?
• Observational constraints on nonlinear matter extensions of general relativity: Separable trace power models
• Testing Gravity and Predictions Beyond the Standard Model at Short Distances: The Casimir Effect
• Transient dark energy, cosmological constant boundary crossing and dark energy $w(z)$ data fits
• The coincidence problem in $f(R)$ gravity models
• Effect of some modified models of gravity on the radial velocity of binary systems
• A High Throughput Workflow Environment for Cosmological Simulations
• Production of primordial gravitational waves in a simple class of running vacuum cosmologies
• Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes
• Does nonlocal gravity yield divergent gravitational energy-momentum fluxes?
• Interacting dark energy: the role of microscopic feedback in the dark sector
• Cosmological Study in Myrzakulov $F(R,T)$ Quasi-dilaton Massive Gravity
• The Matter Power Spectrum of Dark Energy Models and the Harrison-Zel'dovich Prescription
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• Gauging the Maxwell extended $\mathcal{G}\mathcal{L}\left(n,\mathbb{R}\right)$ and $\mathcal{SL}\left(n+1,\mathbb{R}\right)$ algebras
• Tsallis holographic dark energy model with event horizon cutoff in modified gravity
• Misinterpreting Modified Gravity as Dark Energy: a Quantitative Study
• Can the NANOGrav observations constrain the geometry of the universe?
• Implementation of cosmological bounce inflation with Nojiri-Odintsov generalized holographic dark fluid
• Viability of general relativity and modified gravity cosmologies using high-redshift cosmic probes
• Euclid: Photometric redshift calibration with self-organising maps
• Holographic connection of f(G) gravity through Barrow and a generalized version of holographic dark fluid
• A comprehensive analysis of Barrow holographic Chaplygin gas model reconstruction and its cosmological consequences
• Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff
• Flat Galactic Rotation Curves from Geometry in Weyl Gravity
• Vacuum Structure and Dark Energy
• Possible use of self-calibration to reduce systematic uncertainties in determining distance-redshift relation via gravitational radiation from merging binaries
• Linear dark energy equation of state revealed by supernovae?
• The Big Trip and Wheeler-DeWitt equation
• Framework Confirmation by Newtonian Abduction
• An Accelerating Universe without Lambda: Delta~Gravity Using Monte Carlo
• Bounding f(R,T) gravity by particle creation
• Dark energy from a renormalization group flow
• Generalized particle dynamics in anti de Sitter spaces: A source for dark energy
• Scaling Hydrodynamical Evolution of a Gravitating Dark-fluid Universe
• Revisiting metric perturbations in tensor-vector-scalar theory
• Inflationary Constraints on the Van der Waals Equation of State
• Dark Energy and Inflation from Gravitational Waves
• Why is Universe so dark ?
• Navigating permanent underdetermination in dark energy and inflationary cosmology
• Constraints on dark energy evolution
• On the Number of Cosmic Strings
• The Dark Components of the Universe Are Slowly Clarified
• Cosmological application of the Maxwell gravity
• Anisotropic power-law inflation for a generalized model of two scalar and two vector fields
• Recent Developments in Degenerate Higher Order Scalar Tensor Theories
• A simple Hubble-like law in lieu of dark energy
• Why the mean anomaly at epoch is not used in tests of non-Newtonian gravity?
• Analysis of regular inflationary cosmological models with two torsion functions in Poincare gauge theory of gravity
• Peripheral, ultrarelativistic production of particles in heavy ion collisions
• Probing Cosmic Acceleration by Using Model-Independent Parametrizations and Three Kinds of Supernova Statistics Techniques
• Late evolution of relic gravitational waves in coupled dark energy models
• Is scalar-tensor gravity consistent with polytropic stellar models?
• Probing dark fluids and modified gravity with gravitational lensing
• Quantum Theory of Cold Dark Matter Halos
• Mass Varying Neutrinos in Supernovae
• Dark Energy from Topology
• Dark energy and spontaneous mirror symmetry breaking
• Geometrical constraints on curvature from galaxy-lensing cross-correlations
• Influence of the correlation prior on reconstruction of the dark energy equation of state
• Re-evaluation of ${\Omega }_k$ of the normalised Friedmann-Lema\^ıtre-Robertson-Walker model: Implications for Hubble constant determinations
• Is the Cosmological Constant of Topological Origin?
• Inflation constraints for classes of f(R) models
• Super-light baryphotons, Weak Gravity Conjecture and Exotic instantons in Neutron-Antineutron transitions
• The Vacuum and the Cosmological Constant Problem
• A Dynamic Dark Information Energy Consistent with Planck Data
• Gravity with free initial conditions: a solution to the cosmological constant problem testable by CMB B-mode polarization
• An Exploration of Heterogeneity in Supernova Type Ia Samples
• Holographic unification of dark matter and dark energy
• A Post-Newtonian Analysis of Regularized 4D-EGB Theory: Complete Set of PPN Parameters and Observational Constraints
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Evolution of perturbations in the model of Tsallis holographic dark energy
• Neutrino Dark Energy in Grand Unified Theories
• On the effect of image denoising on galaxy shape measurements
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• Exploring the expansion of the universe using the Grüneisen parameter
• Anisotropic cosmology in Bumblebee gravity theory
• The inhomogeneous equation of state and the road towards the solution of the cosmological constant problem
• To theory of gravitational interaction
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• FLRW Cosmology of Induced Dark Energy Model and Open Universe
• Assessing the viability of successful reconstruction of the dynamics of dark energy using varying fundamental couplings
• Maxwell-Modified Metric Affine Gravity
• Growth of Perturbations using Lambert$W$ Equation of State
• The $\kappa$-model, a minimal model alternative to dark matter. Application to the galactic rotation problem
• Current observational constraints on holographic dark energy model
• Quark-Novae Ia in the Hubble diagram: Implications For Dark Energy
• Schwinger's Approach to Einstein's Gravity and Beyond
• Astrophysical evidence for an extra dimension: phenomenology of a Kaluza Klein theory
• Evaluating the effect of stellar multiplicity on the PSF of space-based weak lensing surveys
• Quantum gravity and the holographic dark energy cosmology
• Repulsive gravity induced by a conformally coupled scalar field implies a bouncing radiation-dominated universe
• Symplectic realization of two interacting spin-two fields in three dimensions
• Higher order mimetic gravity after GW170817
• Exoplanetary Interiors
• Dark matter fluid constraints from galaxy rotation curves
• Is cosmic dynamics self-regulating?
• Cosmological Constant, Inflaton, and Dark Matter all Naturally Originated from Poincaré Gauge Gravity
• Numerical analysis of cosmological models for accelerating Universe in Poincare gauge theory of gravity
• Generation of effective massive Spin-2 fields through spontaneous symmetry breaking of scalar field
• The Universe according to DESI results
• A cosmic speed-trap: a gravity-independent test of cosmic acceleration using baryon acoustic oscillations
• Potential of constraining the Fifth Force Using the Earth as a Spin and Mass Source from space
• Matter Creation Cosmologies and Accelerated Expansion
• A sub-ppm upper limit on the cosmological variations of the fine structure constant alpha
• Cybersusy Solves the Cosmological Constant Problem
• The cosmological constant emerging from a symmetry invariant
• Signatures of Solar Chameleons in the Earth's Magnetic Field
• Possible Relation between the Cosmological Constant and Standard Model Parameters
• Gravity Beyond Einstein? Yes, but in Which Direction?
• Cosmological Constant from Boundary Condition and Its Implications beyond the Standard Model
• Cosmological Implications of a Neutrino Mass Detection
• Varying Alpha Generalized Dirac-Born-Infeld Models
• Dynamical behavior of the Universe: an entropic force scenario
• Phantom Domain Walls
• Coupled Dark Energy field variation
• Single scale factor for the universe from the creation of radiation and matter till the present
• A bound system in the expanding universe with modified holographic Ricci dark energy and dark matter
• Orbifold Branes in the $M_D\times M_{d^{+}}\times M_{d^{-}}$ Compactification of type II string on $S^1/Z_2$ and their cosmological applications
• The inhomogeneous equation of state and the speed of convergence to a small cosmological constant
• Physics and Cosmology : the Milli-Electron-Volt Scale
• Mass Determination of New Particle States
• Compact Objects in 4D Einstein Gauss Bonnet Gravity A Data Based Perspective
• Cluster optical depth and pairwise velocity estimation using machine learning
• Exploring Cosmological Implications of the Modified Raychaudhuri Equation in Non-Gravitating Vacuum Energy Theory
• A Model For Intergalactic Filaments and Galaxy Formation During the First Gigayear
• Dark Energy from Time Crystals
• Gravitational Waves with Dark Energy
• Cosmology of Quasi-Dilaton Massive Gravity with Non-minimal Kinetic Coupling
• The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
• Is it possible to separate baryonic from dark matter within the $\Lambda$-CDM formalism?
• Bose-Einstein condensates in microgravity and fundamental tests of gravity
• Modified Friedmann Equations from Maxwell-Weyl Gauge Theory
• Stability of Differentially Rotating Disks in $f(T)$ Theory
• Concluding Talk: A Theorist Overview on Particle Physics
• Testing of Dark Energy and a Solution of the Cosmological Constant Problem
• Inference of cosmological models with principal component analysis
• Dark energy from a geometrical gauge scalar-tensor theory of gravity
• Dynamical dark energy from extra dimensions
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Phenomenological aspects of supergravity theories in de Sitter vacua
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• Perspectives for studying the dark energy at z>2 with galaxy surveys
• A new approach to modified-gravity models
• Confronting Einstein Yang Mills Higgs Dark Energy in light of observations
• Extremal cosmological black holes in Horndeski gravity and the anti-evaporation regime
• Current Status of LHC Physics: Precision Theory View
• Exploring the Latest Pantheon SNIa Dataset by Using Three Kinds of Statistics Techniques
• Cosmology via Metric-Independent Volume-Form Dynamics
• Some remarks on axion dark matter, dark energy and energy of the quantum vacuum
• Observations of General Relativity at strong and weak limits
• A transient phase in cosmological evolution : A multi-fluid approximation for a quasi-thermodynamics equilibrium
• Expansion of a spherical dust gas -- the cosmological conundrum
• Cosmological constraints from supernova data set with corrected redshift
• Cosmic Dark Energy Emerging from Gravitationally Effective Vacuum Fluctuations
• Ads spacetime in Lorentz covariant gauges
• Inflation and Linear Expansion in the Radiation Dominated era in Jordan-Brans-Dicke Cosmology
• A novel mechanism for the distance-redshift relation
• Nonrelativistic Dark-Energy Fluid in a Baby Universe
• Dark Energy After DESI DR2: Observational Status, Reconstructions, and Physical Models
• Cosmic acceleration and the challenge of modifying gravity
• The peculiar case of the Viaggiu holographic dark energy
• Deparametrization and quantization of scalar-tensor gravity and its cosmological model
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• The holographic principle and the cosmological constant
• Viaggiu holographic dark energy in light of DESI DR2
• Epoch Dependent Dark Energy
• Lorentz-covariant quantum transport and the origin of dark energy
• Avoiding unrealistic priors: the case of dark energy constraints from the time variation of the fine-structure constant
• Non-minimally coupled dark fluid in Schwarzschild spacetime
• Effective dark energy from decoherence
• Beyond LCDM: Bits join the Dark Side
• Dark Matter and Dark Energy
• Mathematical Models in Isotropic Cosmology
• Halos of dark energy
• Monte Carlo study of NLO correction to QCD evolution kernel induced by the change of the factorization scale
• GUP-corrected $\Lambda$CDM cosmology
• Phase space analysis of Bianchi III Universe with $f(R,T)$ gravity theory
• Intermediate evolution using SNIa, and BAO
• Phase space analysis and cosmography of a two-fluid cosmological model
• Search for dark matter in the framework of Einstein-Cartan gravity at the International Linear Collider (ILC)
• The Concept of an Emergent Cosmographic Vacuum
• Axion boson stars with wormhole topology
• Cosmological aspects of cubic Galileon massive gravity
• Gravitational Lensing Effect from The Revised Deser-Woodard Nonlocal Gravity
• Search for an exotic parity-odd spin- and velocity-dependent interaction using a magnetic force microscope
• Pathology of the Unified Dark Sectors in Modified General Relativity
• Perturbations In Some Dark Energy Models
• Cylindrical cosmological simulations with StePS
• Bayesian Inference of Neutron Star Properties in $f(Q)$ Gravity Using NICER Observations
• UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
• Coupling dark-baryonic matter density profile for vacuum decay scenarios
• The creation of radiation and the relic of inflaton potential
• Analysis of some classical and quantum aspects of black holes
• Statistical Mechanics of the L-Distance Minimal Dominating Set problem
• Scalar perturbation of the viscosity dark fluid cosmological model
• Scalar-field potential for viable models in $f(R)$ theory
• How Holographic is the Dark Energy? A Spline Nodal reconstruction approach
• General Relativistic Thick Disks in the Accelerating Expanding Universe Dominated By Dark Energy
• Flavour Condensate and the Dark Sector of the Universe
• Self-interaction in a cosmic dark fluid: The four-kernel rheological extension of the equations of state
• Scalar-Field Reconstruction of Ricci--Gauss--Bonnet Dark Energy in Hořava--Lifshitz Cosmology
• The Riddle of Gravitation
• Chiral Bargmann-Wigner Equations for Spin-1 Massive Fields
• Has the density of sources of gamma-ray burts been constant over the last ten billion years ?
• Running vacuum model versus $\Lambda$CDM -- a Bayesian analysis
• An analysis of Born-Infeld boson compact objects
• Inductive rectilinear frame dragging and local coupling to the gravitational field of the universe
• Use of Redshifts as Evidence of Dark Energy