Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

Abstract

We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration. These objects, discovered during the course of the GOODS ACS Treasury program, include 6 of the 7 highest-redshift SNe Ia known, all at z>1.25, and populate the Hubble diagram in unexplored territory. The luminosity distances to these and 170 previous SNe Ia are provided. A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at z=0.46 +/- 0.13. The data are consistent with the cosmic concordance model of Omega_M ~ 0.3, Omega_Lambda~0.7 (chi^2_dof=1.06), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy. For a flat Universe with a cosmological constant. When combined with external flat-Universe constraints we find w=-1.02 + 0.13 - 0.19 (and $<-0.76atthe95$w_0$, and its time evolution, dw/dz, are a factor of ~8 more precise than its first estimate and twice as precise as those without the SNe Ia discovered with HST. Our constraints are consistent with the static nature of and value of w expected for a cosmological constant (i.e., w_0 = -1.0, dw/dz = 0), and are inconsistent with very rapid evolution of dark energy. We address consequences of evolving dark energy for the fate of the Universe.

Accepted Astrophysical Journal, to Appear June 2004 72 pages, 17 Figures

References in corpus (65)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• The Cosmological Constant and Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Exploring the Expansion History of the Universe
• Phantom Energy and Cosmic Doomsday
• Cosmological Results from High-z Supernovae
• The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
• Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
• The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Cur vature of the Universe Using Type Ia Supernovae
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• A method for optimal image subtraction
• Accelerated Universe from Gravity Leaking to Extra Dimensions
• Supernova Limits on the Cosmic Equation of State
• A Precise Distance Indicator: Type Ia Supernova Multicolor Light Curve Shapes
• BVRI Light Curves for 22 Type Ia Supernovae
• The Absolute Luminosities of the Calan/Tololo Type Ia Supernovae
• 23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at z>0.7
• A median redshift of 2.4 for galaxies bright at submillimetre wavelengths
• A new catalog of photometric redshifts in the Hubble Deep Field
• The case for dynamical dark energy revisited
• Type Ia Supernovae: Influence of the Initial Composition on the Nucleosynthesis, Light Curves, Spectra and Consequences for the Determination of Omega_M & Lambda
• Using SN Ia Light Curve Shapes to Measure The Hubble Constant
• K-corrections and Extinction Corrections for Type Ia Supernovae
• Dust and Extinction Curves in Galaxies with z>0: The Interstellar Medium of Gravitational Lens Galaxies
• The Hubble Diagram of the Calan/Tololo Type Ia Supernovae and the value of Ho
• The Risetime of Nearby Type Ia Supernovae
• A Search for Environmental Effects on Type Ia Supernovae
• Measuring and Understanding the Universe
• Intergalactic Dust and Observations of Type Ia Supernovae
• A large sample of spectroscopic redshifts in the ACS-GOODS region of the HDF-N
• Future supernovae data and quintessence models
• The evolution of field early-type galaxies to z~0.7
• Do SNe Ia Provide Direct Evidence for Past Deceleration of the Universe?
• Type Ia Supernovae, Evolution, and the Cosmological Constant
• The Case for an Accelerating Universe from Supernovae
• The Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology
• Dust Versus Cosmic Acceleration
• Extinction and the Radial Distribution of Supernova Properties in Their Parent Galaxies
• The Redshift Distribution and Luminosity Functions of Galaxies in the Hubble Deep Field
• Creating Spectral Templates from Multicolor Redshift Surveys
• Spectral Templates from Multicolor Redshift Surveys
• High Redshift Supernovae in the Hubble Deep Field
• Lensing and high-z supernova surveys
• Observational Bounds on Cosmic Doomsday
• The evolution of the Tully-Fisher relation of spiral galaxies
• A novel image reconstruction method applied to deep Hubble Space Telescope Images
• The Flat Spectrum Radio Luminosity Function, Gravitational Lensing, Galaxy Ellipticities and Cosmology
• A Fundamental Test of the Nature of Dark Matter
• Importance of Supernovae at z>1.5 to Probe Dark Energy
• Identification of Type Ia Supernovae at Redshift 1.3 and Beyond with the Advanced Camera for Surveys on HST
• Measuring the properties of extragalactic dust and implications for the Hubble diagram
• The magnification of SN 1997ff, the farthest known Supernova
• Discovery of Two Distant Type Ia Supernovae in the Hubble Deep Field North with the Advanced Camera for Surveys
• Optical Spectra of Type Ia Supernovae at z=0.46 and z=1.2
• Dark Energy and the Fate of the Universe
• Vacuum effects of ultra-low mass particle account for Recent Acceleration of Universe
• Gravitational lensing of the farthest known supernova SN1997ff
• Was SN1997ff at z~1.7 magnified by gravitational lensing?
• Cosmological Acceleration Through Transition to Constant Scalar Curvature
• Einstein's Biggest Blunder? High-Redshift Supernovae and the Accelerating Universe
• Q-LET - Quick Lensing Estimation Tool - An application to SN2003es
• Sub-millimeter emission from type Ia supernova host galaxies at z=0.5

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• Constraining Dark Energy with X-ray Galaxy Clusters, Supernovae and the Cosmic Microwave Background
• Notes on $f(T)$ Theories
• Exact Solutions of Bianchi Types $I$ and $V$ Spacetimes in $f(R)$ Theory of Gravity
• A New Method to Calibrate the Magnitudes of Type Ia Supernovae at Maximum Light
• LXCDM: a cosmon model solution to the cosmological coincidence problem?
• Density perturbations in general modified gravitational theories
• Cosmology with a Variable Chaplygin Gas
• Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter
• A parametric reconstruction of the deceleration parameter
• Bianchi Type-$V$ cosmology in $f(R,T)$ gravity with $\Lambda (T)$
• The Rise and Fall of Type Ia Supernova Light Curves in the SDSS-II Supernova Survey
• Density perturbations in f(R) gravity theories in metric and Palatini formalisms
• The Chemical Abundances of Tycho G in Supernova Remnant 1572
• Generalizing the generalized Chaplygin gas
• The Carnegie Supernova Project: First Near-Infrared Hubble Diagram to z~0.7
• Scant evidence for thawing quintessence
• Gauss-Bonnet cosmologies: crossing the phantom divide and the transition from matter dominance to dark energy
• Effect on cosmic microwave background polarization of coupling of quintessence to pseudoscalar formed from the electromagnetic field and its dual
• Interacting Quintessence, Cosmic Acceleration and the Coincidence Problem
• String-inspired cosmology: Late time transition from scaling matter era to dark energy universe caused by a Gauss-Bonnet coupling
• Observational $H(z)$ Data and Cosmological Models
• Deflection Angle and Shadow Behaviors of Quintessential Black Holes in arbitrary Dimensions
• Constraining dark energy with cross-correlated CMB and Large Scale Structure data
• Quintom model with O($N$) symmetry
• Polarization of gravitational waves in symmetric teleparallel theories of gravity and their modifications
• Dark Energy Models in the w - w' Plane
• Dark energy from a quintessence (phantom) field rolling near potential minimum (maximum)
• Dark Energy Constraints from the CTIO Lensing Survey
• Stability of the Einstein static Universe in $f(R,T)$ gravity
• The Absolute Magnitudes of Type Ia Supernovae in the Ultraviolet
• A String-Inspired Quintom Model Of Dark Energy
• CDM Accelerating Cosmology as an Alternative to LCDM model
• The Dark Universe
• Torsion Cosmology and the Accelerating Universe
• Condensates in Quantum Chromodynamics and the Cosmological Constant
• Cosmological Signatures of Interacting Neutrinos
• VAST: An ASKAP Survey for Variables and Slow Transients
• Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
• Cosmo-dynamics and dark energy with non-linear equation of state: a quadratic model
• Fundamental limitations on "warp drive" spacetimes
• Hilltop Quintessence
• The phase space view of f(R) gravity
• Avocado: Photometric Classification of Astronomical Transients with Gaussian Process Augmentation
• The Effect of Inhomogeneities on the Luminosity Distance-Redshift Relation: is Dark Energy Necessary in a Perturbed Universe?
• Cosmology with Photometrically-Classified Type Ia Supernovae from the SDSS-II Supernova Survey
• Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results
• A Sudden Gravitational Transition
• Can superhorizon cosmological perturbations explain the acceleration of the universe?
• Constraining Isocurvature Initial Conditions with WMAP 3-year data
• Correlating the CMB with Luminous Red Galaxies : The Integrated Sachs-Wolfe Effect
• Gravitational Waves in Modified Teleparallel Theories
• Supernova cosmology: legacy and future
• Model Independent Reconstruction of the Expansion History of the Universe and the Properties of Dark Energy
• The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses
• Observing Dark Energy Dynamics with Supernova, Microwave Background and Galaxy Clustering
• Constraining Inverse Curvature Gravity with Supernovae
• Interacting models of soft coincidence
• Constraints on Oscillating Quintom from Supernova, Microwave Background and Galaxy Clustering
• Evolution of linear cosmological perturbations and its observational implications in Galileon-type modified gravity
• Cosmographic Hubble fits to the supernova data
• Parameterized Post-Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• Age Problem in the Holographic Dark Energy Model
• Anisotropic strange star with Tolman-Kuchowicz metric under $f(R,T)$ gravity
• Some Issues Concerning Holographic Dark Energy
• Modified TOV in gravity's rainbow: properties of neutron stars and dynamical stability conditions
• Likelihood-Free Cosmological Inference with Type Ia Supernovae: Approximate Bayesian Computation for a Complete Treatment of Uncertainty
• On type Ia supernovae and the formation of single low-mass white dwarfs
• Using Line Profiles to Test the Fraternity of Type Ia Supernovae at High and Low Redshifts
• Exactly Solvable SFT Inspired Phantom Model
• Constraining f(R) gravity in the Palatini formalism
• Hubble expansion and structure formation in the "running FLRW model" of the cosmic evolution
• Cosmological parameters from strong gravitational lensing and stellar dynamics in elliptical galaxies
• Hints of FLRW Breakdown from Supernovae
• Nonlinear Structure Formation and "Apparent" Acceleration: an Investigation
• FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space
• No realistic wormholes from ghost-free scalar-tensor phantom dark energy
• Future Cosmological Constraints from Fast Radio Bursts
• The Extended Hubble Space Telescope Supernova Survey: The Rate of Core Collapse Supernovae to z~1
• Breaking the Degeneracies Between Cosmology and Galaxy Bias
• Constraints on the Sound Speed of Dynamical Dark Energy
• Confronting Braneworld Cosmology with Supernova data and Baryon Oscillations
• Can we be tricked into thinking that w is less than -1?
• Statefinders, higher-order energy conditions and sudden future singularities
• Higher order gravity theories and their black hole solutions
• Dark Energy Model with Spinor Matter and Its Quintom Scenario
• Exact solutions of f(R) gravity coupled to nonlinear electrodynamics
• Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Anisotropic cosmological models in $f(R,T)$ gravity with variable deceleration parameter
• Cosmology in $f(R,L_m)$ gravity
• The Outermost Ejecta of Type Ia Supernovae
• Signature of the interaction between dark energy and dark matter in observations
• Bouncing and Accelerating Solutions in Nonlocal Stringy Models
• f(R) Gravity with Torsion: The Metric-Affine Approach
• The Holographic dark energy reexamined
• Bayesian evidence as a tool for comparing datasets
• Physical Characteristics and Maximum Allowable Mass of Hybrid Star in the Context of $f(Q)$ Gravity
• Energy Conditions and Cosmic Acceleration
• Lower limits on the Hubble Constant from models of Type Ia Supernovae
• Cosmographic Constraints and Cosmic Fluids
• Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
• Testing the Isotropy of the Universe with Type Ia Supernovae
• Noether symmetry approach in phantom quintessence cosmology
• On holographic dark-energy models
• Can a matter-dominated model with constant bulk viscosity drive the accelerated expansion of the universe?
• Impact of the Rastall parameter on perfect fluid spheres
• The supernova Hubble diagram for off-center observers in a spherically symmetric inhomogeneous universe
• Some exact solutions of F(R) gravity with charged (a)dS black hole interpretation
• Observational constraints on phantom-like braneworld cosmologies
• Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
• Hybrid modified gravity unifying local tests, galactic dynamics and late-time cosmic acceleration
• Primordial Neutrinos
• Dark Fluid: a complex scalar field to unify dark energy and dark matter
• Probing the curvature and dark energy
• Model independent analysis of dark energy I: Supernova fitting result
• Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
• Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test
• Present and future evidence for evolving dark energy
• Interacting dark energy in $f(R)$ gravity
• Some Anisotropic Dark Energy Models in Bianchi Type-V Space-time
• Reddening, Absorption, and Decline Rate Corrections for a Complete Sample of Type Ia Supernovae leading to a Fully Corrected Hubble Diagram to v<30,000kms-1
• Kerr-Newman-AdS Black Hole In Quintessential Dark Energy
• Dynamics of Interacting Quintessence Models: Observational Constraints
• Tension and Systematics in the Gold06 SnIa Dataset
• Dark matter and dark energy as a effects of Modified Gravity
• Effects of dark sectors' mutual interaction on the growth of structures
• Measuring the cosmic evolution of dark energy with baryonic oscillations in the galaxy power spectrum
• Some Bianchi Type-V Models of Accelerating Universe with Dark Energy
• Generalized holographic dark energy and the IR cutoff problem
• Vacuum Fluctuations of Energy Density can lead to the observed Cosmological Constant
• Photometric selection of high-redshift type Ia supernovae
• Dark energy models from a parametrization of $H$: A comprehensive analysis and observational constraints
• The Extended HST Supernova Survey: The Rate of SNe Ia at z>1.4 Remains Low
• Constraints on the sound speed of dark energy
• Some remarks on the dynamical systems approach to fourth order gravity
• Exploring a matter-dominated model with bulk viscosity to drive the accelerated expansion of the Universe
• Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey
• Modified Chaplygin Gas Cosmology
• On the Geometry of Dark Energy
• Exploring the Properties of Dark Energy Using Type Ia Supernovae and Other Datasets
• Solar System Constraints on Gauss-Bonnet Mediated Dark Energy
• f(R) theories of gravity in Palatini approach matched with observations
• Relativistic Krori-Barua Compact Stars in $f(R,T)$ Gravity
• Can higher curvature corrections cure the singularity problem in f(R) gravity?
• Cosmography by GRBs
• Evolution of the universe in entropic cosmologies via different formulations
• The Cosmology of Ricci-Tensor-Squared Gravity in the Palatini Variational Approach
• Evolving Newton's Constant, Extended Gravity Theories and SnIa Data Analysis
• Dark energy exponential potential models as curvature quintessence
• Phantom stars and topology change
• Cosmokinetics: A joint analysis of Standard Candles, Rulers and Cosmic Clocks
• Two-Fluid Scenario for Dark Energy Models in an FRW Universe-Revisited
• Bulk and Brane Decay of a (4+n)-Dimensional Schwarzschild-De-Sitter Black Hole: Scalar Radiation
• Constraining alternative theories of gravity by gravitational waves from precessing eccentric compact binaries with LISA
• Kerr-Newman-AdS Black Hole Surrounded by Perfect Fluid Matter in Rastall Gravity
• The Foundation Supernova Survey: Measuring Cosmological Parameters with Supernovae from a Single Telescope
• Improved constraints on cosmological parameters from SNIa data
• Which cosmological model with dark energy -- phantom or LambdaCDM
• Einstein static Universe in hybrid metric-Palatini gravity
• Axion-Like Particles, Cosmic Magnetic Fields and Gamma-Ray Astrophysics
• Voids as a Precision Probe of Dark Energy
• Constraints on kinematic models from the latest observational data
• Observational constraints on the acceleration of the Universe
• Early-type Host Galaxies of Type Ia Supernovae. II. Evidence for Luminosity Evolution in Supernova Cosmology
• Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields
• Dark matters on the scale of galaxies
• Modified gravity and the stability of de Sitter space
• Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
• Magnetic Neutron Stars in f(R) gravity
• Photon-axion conversion as a mechanism for supernova dimming: Limits from CMB spectral distortion
• Thermodynamical properties of the Universe with dark energy
• General analytic formulae for attractor solutions of scalar-field dark energy models and their multi-field generalizations
• Status of Dark Matter in the Universe
• Non-linear Structure Formation in Cosmologies with Early Dark Energy
• Measuring cosmological parameters with Gamma-Ray Bursts
• Anisotropic Quintessence stars
• Dynamical dark energy or variable cosmological parameters?
• Bayesian model selection and isocurvature perturbations
• Bulk Viscosity, Decaying Dark Matter, and the Cosmic Acceleration
• Constraints on dark energy with the LOSS SN Ia sample
• On the co-existence of matter dominated and accelerating solutions in f(G)-gravity
• Cosmological Applications of Pade Approximant
• Lightest Neutralino in Extensions of the MSSM
• Improved Measurements of the CMB Power Spectrum with ACBAR
• SNLS Spectroscopy: Testing for Evolution in Type Ia Supernovae
• Cosmologies with a time dependent vacuum
• Supernova limits on brane world cosmology
• Non-minimal coupling, exponential potentials and the $w<-1$ regime of dark energy
• Interpretation of the Hubble diagram in a nonhomogeneous universe
• Thermal history of the plasma and high-frequency gravitons
• A new perspective on Dark Energy modeling via Genetic Algorithms
• If Gauss-Bonnet interaction plays the role of dark energy
• Internal space structure generalization of the quintom cosmological scenario
• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter
• Constraints on backreaction in dust universes
• A divergence free parametrization of deceleration parameter for scalar field dark energy
• Correlated Primordial Perturbations in Light of CMB and LSS Data
• Cosmological evolution in R^2 gravity
• Braneworld models with a non-minimally coupled phantom bulk field: a simple way to obtain the -1-crossing at late times
• Non-minimally Coupled Quintom Model Inspired by String Theory
• Sudden future singularities in FLRW cosmologies
• Testing Models of Intrinsic Brightness Variations in Type Ia Supernovae, and their Impact on Measuring Cosmological Parameters
• Metallicity effect in multi-dimensional SNIa nucleosynthesis
• Searching for a holographic connection between dark energy and the low-l CMB multipoles
• The Art of Lattice and Gravity Waves from Preheating
• The Holographic Model of Dark Energy and Thermodynamics of Non-Flat Accelerated Expanding Universe
• Constraining the Dark Energy Equation of State with Cosmic Voids
• A Note on Crossing the Phantom Divide in Hybrid Dark Energy Model
• Gravity on codimension 2 brane worlds
• Comparison of Approaches to Quantum Correction of Black Hole Thermodynamics
• Charting the Landscape of Modified Gravity
• The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914
• The Effect of Large-Scale Inhomogeneities on the Luminosity Distance
• Vacuum energy in Einstein-Gauss-Bonnet AdS gravity
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• Supernovae in the Subaru Deep Field: An Initial Sample, and Type Ia Rate, out to Redshift 1.6
• Supernovae constraints on models of dark energy revisited
• Dynamics in Nonlocal Cosmological Models Derived from String Field Theory
• Modified equation of state, scalar field, and bulk viscosity in Friedmann universe
• Cosmic Acceleration, Dark Energy and Fundamental Physics
• z~7 galaxy candidates from NICMOS observations over the HDF South and the CDF-S and HDF-N GOODS fields
• Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
• Kerr-Anti-De-Sitter/De-Sitter Black Hole In Perfect Fluid Dark Matter Background
• Dynamical dark energy with a constant vacuum energy density
• Dark energy transition between quintessence and phantom regimes - an equation of state analysis
• Consistency among distance measurements: transparency, BAO scale and accelerated expansion
• K-Chameleon and the Coincidence Problem
• Reconstruction of cosmic history from a simple parametrization of H
• Dark energy perturbations and cosmic coincidence
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• N-Body Simulations of Alternate Gravity Models
• Properties of the ultraviolet flux of type Ia supernovae: an analysis with synthetic spectra of SN 2001ep and SN 2001eh
• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• Expansion, Geometry, and Gravity
• Observational Evidence of the Accelerated Expansion of the Universe
• Noether Symmetry Approach in $f(\mathcal{G},T)$ Gravity
• Bayesian Estimation Applied to Multiple Species: Towards cosmology with a million supernovae
• Reconstruction of general scalar-field dark energy models
• Holographic principle and dark energy
• Cosmological bounds on the equation of state of dark matter
• Short distance and initial state effects in inflation: stress tensor and decoherence
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Constraints on Distance Duality Relation from Sunyaev Zel'dovich Effect and Chandra X-ray measurements
• Dynamics of f(R)-cosmologies containing Einstein static models
• Central Density Dependent Anisotropic Compact Stars
• Type II-P Supernovae from the SDSS-II Supernova Survey and the Standardized Candle Method
• A model independent null test on the cosmological constant
• On using the CMB shift parameter in tests of models of dark energy
• Constraint on the Post-Newtonian Parameter gamma on Galactic Size Scales
• Constraints on f(R) Cosmology in the Palatini Formalism
• Two photon annihilation of Kaluza-Klein dark matter
• Evaluating backreaction with the peak model of structure formation
• Phantom Dark Energy, Cosmic Doomsday, and the Coincidence Problem
• Direct reconstruction of the quintessence potential
• Microlensing of Lensed Supernovae
• Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
• A Note on Agegraphic Dark Energy
• Plane Symmetric Solutions in f(R) Gravity
• Late-time Inhomogeneity and Acceleration Without Dark Energy
• Kination Dominated Reheating and Cold Dark Matter Abundance
• Non-Vacuum Bianchi Types I and V in f(R) Gravity
• Probing the cosmographic parameters to distinguish between dark energy and modified gravity models
• Time Lumps in Nonlocal Stringy Models and Cosmological Applications
• Holographic Dark Energy in Braneworld Models with Moving Branes and the w=-1 Crossing
• Phantom Dark Energy Models with a Nearly Flat Potential
• Photometry of the Type Ia Supernovae 1999cc, 1999cl, and 2000cf
• Determination of the Hubble constant, the intrinsic scatter of luminosities of Type Ia SNe, and evidence for non-standard dust in other galaxies
• Can Gamma-Ray Bursts Be Used to Measure Cosmology? A Further Analysis
• Quintessential Kination and Cold Dark Matter Abundance
• A new null diagnostic customized for reconstructing the properties of dark energy from BAO data
• Constraining cosmic deceleration-acceleration transition with type Ia supernova, BAO/CMB and H(z) data
• Dual interacting cosmologies and late accelerated expansion
• Gamma-ray burst prompt correlations: selection and instrumental effects
• A New Perspective on DGP Gravity
• Some Exact Solutions in $f(\mathcal{G},T)$ Gravity via Noether Symmetries
• Pseudo-Newtonian and general relativistic barotropic tori in Schwarzschild-de Sitter spacetimes
• The Cauchy problem of f(R) gravity
• The past and future dynamics of quintom dark energy models
• Cosmological model with energy transfer
• Paramerization of deceleration parameter in $f(Q)$ gravity
• A new framework for studying spherically symmetric static solutions in f(R) gravity
• A new method optimized to use Gamma Ray Bursts as cosmic rulers
• $\Lambda \alpha$DM: Observational constraints on unified dark matter with constant speed of sound
• Falsifying Paradigms for Cosmic Acceleration
• Analysis of the Yukawa gravitational potential in $f(R)$ gravity II: relativistic periastron advance
• Probing kinematics and fate of the Universe with linearly time-varying deceleration parameter
• Mass Varying Neutrinos in the Sun
• Measurement of Ω_m, Ω_Λ from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe
• Non-local SFT Tachyon and Cosmology
• Light Propagation and Large-Scale Inhomogeneities
• Beyond the perfect fluid hypothesis for dark energy equation of state
• Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
• Improved WIMP-search reach of the CDMS II germanium data
• Do spectra improve distance measurements of Type Ia supernovae?
• The blackness of the cosmic microwave background spectrum as a probe of the distance-duality relation
• Hint for Quintessence-like Scalars from Holographic Dark Energy
• Magnetized CMB observables: a dedicated numerical approach
• Scientific Potential of DECIGO Pathfinder and Testing GR with Space-Borne Gravitational Wave Interferometers
• Growth Index of DGP Model and Current Growth Rate Data
• Nonlinear growth in modified gravity theories of dark energy
• Neutrino mixing as a source of dark energy
• Constraining $f(R)$ gravity by the Large Scale Structure
• Bi-galileon theory II: phenomenology
• Anisotropic Fluid and Bianchi Type III Model in f(R) Gravity
• The impact of Early Dark Energy on non-linear structure formation
• De Sitter Universe in Nonlocal Gravity
• ESC observations of SN 2005cf: II. Optical Spectroscopy and the high velocity features
• Photon-axion conversion in intergalactic magnetic fields and cosmological consequences
• Black hole entropy in scalar-tensor and f(R) gravity: an overview
• Review of Observational Evidence for Dark Matter in the Universe and in upcoming searches for Dark Stars
• Analyze This! A Cosmological Constraint Package for CMBEASY
• Constraints on the Dark Side of the Universe and Observational Hubble Parameter Data
• The relativistic Feynman-Metropolis-Teller theory for white-dwarfs in general relativity
• Observational constraints on interacting Tsallis holographic dark energy models
• Constraints on barotropic dark energy models by a new phenomenological $q(z)$ parameterization
• Cosmological Evolution in f(R,T) theory with Collisional Matter
• New agegraphic dark energy model with generalized uncertainty principle
• Spherical collapse model with shear and angular momentum in dark energy cosmologies
• Interacting Phantom Energy and Avoidance of the Big Rip Singularity
• Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy
• Comparison of Standard Ruler and Standard Candle constraints on Dark Energy Models
• The reliability of the AIC method in Cosmological Model Selection
• Gamma-ray bursts as dark energy-matter probes in the context of the generalized Chaplygin gas model
• Observational constraints on the deceleration parameter in a tilted universe
• A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys
• Initial state of matter fields and trans-Planckian physics: Can CMB observations disentangle the two?
• Energy conditions and current acceleration of the universe
• Cosmological evolution in vector-tensor theories of gravity
• Energy Conditions and Supernovae Observations
• On the progenitors of super-Chandrasekhar mass type Ia supernovae
• Comparison of an X-ray selected sample of massive lensing clusters with the MareNostrum Universe LCDM simulation
• Reconstruction of $\Lambda$CDM Universe in $f(Q)$ Gravity
• We do not live in the R_h = c t universe
• Genetic Algorithms and Supernovae Type Ia Analysis
• Constraining dark energy models using the lookback time to galaxy clusters and the age of the universe
• Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem
• A WISE measurement of the ISW effect
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Gravitational lensing in fourth order gravity
• Cosmological scaling solutions in generalised Gauss-Bonnet gravity theories
• Mimicking Lambda with a spin-two ghost condensate
• Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate
• On the Stability of Phantom K-essence Theories
• SO(1,1) dark energy model and the universe transition
• Cosmological Constraints on a Power Law Universe
• Invariant solutions and Noether symmetries in Hybrid Gravity
• The Limits of Extended Quintessence
• Test of the cosmic evolution using Gaussian processes
• An Interacting Two-Fluid Scenario for Dark Energy in FRW Universe
• Reconstructing the dark energy equation of state with varying couplings
• Spectroscopy of High-Redshift Supernovae from the ESSENCE Project: The First Two Years
• The Weak Energy Condition and the Expansion History of the Universe
• Kaluza-Klein cosmological model in $f(R,T)$ gravity with $\Lambda (T)$
• The effect of an expanding universe on massive objects
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• General form of entropy on the horizon of the universe in entropic cosmology
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Cosmic acceleration and crossing of w=-1 barrier in non-local Cubic Superstring Field Theory model
• Dark Energy: Recent Developments
• Dark Energy Model in Anisotropic Bianchi Type-III Space-Time with Variable EoS Parameter
• The Jebsen-Birkhoff theorem in alternative gravity
• Cosmology of neutrinos and extra light particles after WMAP3
• Generalized Chaplygin Gas Models tested with SNIa
• ALMA Lensing Cluster Survey: $HST$ and $Spitzer$ Photometry of 33 Lensed Fields Built with CHArGE
• Dependence of the non-linear mass power spectrum on the equation of state of dark energy
• Accelerated Cosmological Models in Modified Gravity tested by distant Supernovae SNIa data
• Quintessence reconstructed: new constraints and tracker viability
• Modified Gravity with a Non-minimal Gravitational Coupling to Matter
• Large-Scale Bulk Motions Complicate the Hubble Diagram
• Off-center explosions of Chandrasekhar-mass white dwarfs: an explanation of super-bright type Ia supernovae?
• Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data
• Neutron stars in $f(\mathtt{R},{\mathtt{L}}_{\mathtt{m}})$ gravity with realistic equations of state: joint-constrains with GW170817, massive pulsars, and the PSR J0030+0451 mass-radius from $NICER$ data
• Kinetic k-essence ghost dark energy model
• Age of High Redshift Objects - a Litmus Test for the Dark Energy Models
• The baryonic mass function of galaxies
• Neutron stars in $f(\mathcal{R},\mathcal{T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
• In search of the dark matter dark energy interaction: a kinematic approach
• Faraday rotation, stochastic magnetic fields and CMB maps
• The mass-radius relation for neutron stars in $f(R)=R+\alpha R^2$ gravity: a comparison between purely metric and torsion formulations
• Model-independent reconstruction of $f(T)$ teleparallel cosmology
• The Fundamental Metallicity Relation Reduces Type Ia SN Hubble Residuals More Than Host Mass Alone
• Dark energy and particle mixing
• Did the Universe loiter at high redshifts ?
• Cosmic Equation of state from Strong Gravitational Lensing Systems
• Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study
• Reconstruction and constraining of the jerk parameter from OHD and SNe Ia observations
• Emergent Universe Scenario in the Einstein-Gauss-Bonnet Gravity with Dilaton
• 6+1 lessons from f(R) gravity
• Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• A review of type Ia supernova spectra
• First-Year Spectroscopy for the SDSS-II Supernova Survey
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• Constraining Lorentz violation with cosmology
• Constraining Van der Waals quintessence by observations
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• The Impact of Cosmic Dust on Supernova Cosmology
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Squeezing the window on isocurvature modes with the Lyman-alpha forest
• Constraints on the dark energy equation of state from recent supernova data
• Phantom energy mediates a long-range repulsive force
• Gravastars in $f(\mathbb{T},\mathcal{T})$ gravity
• The cosmic snap parameter in f(R) gravity
• Density Perturbations for Running Cosmological Constant
• Liouville Cosmology at Zero and Finite Temperatures
• Energy Conditions and Segre Classification of Phantom Fields
• Isocurvature, non-gaussianity and the curvaton model
• Connecting early and late universe by $f(R)$ gravity
• Phase space geometry in scalar-tensor cosmology
• Current constraints on the epoch of cosmic acceleration
• Supernova constraints on decaying vacuum cosmology
• Cosmology with decaying tachyon matter
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• Information-theoretic model selection applied to supernovae data
• Constraining the Cosmological Parameters and Transition Redshift with Gamma-Ray Bursts and Supernovae
• Observational constraint on generalized Chaplygin gas model
• Reconciling the local void with the CMB
• Redshift-Independent Distances in the NASA/IPAC Extragalactic Database: Methodology, Content and Use of NED-D
• On the determination of the deceleration parameter from Supernovae data
• Making sense of the bizarre behaviour of horizons in the McVittie spacetime
• Higher-order gravity and the cosmological background of gravitational waves
• Relaxing Nucleosynthesis Constraints on Brans-Dicke Theories
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Bayesian analysis of Friedmannless cosmologies
• When did cosmic acceleration start? How fast was the transition?
• Forecasting the Bayes factor of a future observation
• The WIMP of a Minimal Technicolor Theory
• Looking for an extra dimension with tomographic cosmic shear
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• Determining the Neutrino Mass Hierarchy with Cosmology
• Dilatonic black holes in gravity's rainbow with a nonlinear source: the effects of thermal fluctuations
• The Relevance of the Cosmological Constant for Lensing
• Curvature constraints from Large Scale Structure
• Towards inflation and dark energy cosmologies from modified Gauss-Bonnet theory
• The Velocity Field of the Local Universe from Measurements of Type Ia Supernovae
• Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
• Generalized Chaplygin Gas in a modified gravity approach
• Matter Non-conservation in the Universe and Dynamical Dark Energy
• A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies
• Accelerating dark energy models in bianchi Type-V space-time
• Interacting entropy-corrected agegraphic-tachyon dark energy
• Thermodynamical Structure of AdS Black Holes in Massive Gravity with Stringy Gauge-Gravity Corrections
• Tight coupling expansion and fully inhomogeneous magnetic fields
• Dynamical Relaxation of Dark Energy: A Solution to Early Inflation, Late-time Acceleration and the Cosmological Constant Problem
• The imprint of the interaction between dark sectors in galaxy clusters
• Could the cosmic acceleration be transient? A cosmographic evaluation
• How clustering dark energy affects matter perturbations
• Supernova Brightening from Chameleon-Photon Mixing
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• On Precision Measurement of the Mean Curvature
• Accelerating universe from gravitational leakage into extra dimensions: confrontation with SNeIa
• The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies
• Stability analysis for cosmological models in $f(R)$ gravity using dynamical system analysis
• Constraints on a generalized deceleration parameter from cosmic chronometers
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• Phantom Dark Energy Models with Negative Kinetic Term
• Limiting the dimming of distant type Ia supernovae
• Mid- to Far-IR Emission and Star Formation in Early-Type Galaxies
• Effect of the quintessential dark energy on weak deflection angle by Kerr-Newmann Black hole
• Bayesian Single-Epoch Photometric Classification of Supernovae
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• Cosmological dynamics with propagating Lorentz connection modes of spin zero
• Cosmological model with non-minimally coupled fermionic field
• Challenging bulk viscous unified scenarios with cosmological observations
• Acceleration of the universe: a reconstruction of the effective equation of state
• Star Models with Dark Energy
• On the relativistic Thomas-Fermi treatment of compressed atoms and compressed nuclear matter cores of stellar dimensions
• Cosmology with moving dark energy and the CMB quadrupole
• Constraints on SN Ia progenitor time delays from high-z SNe and the star formation history
• Constraints on Scalar-Field Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift
• Non-adiabatic-like accelerated expansion of the late universe in entropic cosmology
• Exact dark energy star solutions
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• Spectra of High-Redshift Type Ia Supernovae and a Comparison with their Low-Redshift Counterparts
• Which cosmological models -- with dark energy or modified FRW dynamics?
• Phantom-like behaviour in dilatonic brane-world scenario with induced gravity
• The Internal Shear of Type Ia Supernova Progenitors During Accretion and Simmering
• Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
• Expansion of magnetic neutron stars in an energy (in)dependent spacetime
• Constrained $f(Q,T)$ gravity accelerating cosmological model and its dynamical system analysis
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• Non-trivial black hole solutions in $f(R)$ gravitational theory
• Modified gravity with $f(R)=\sqrt{R^2-R_0^2}$
• The cosmological constant as an eigenvalue of f(R)-gravity Hamiltonian constraint
• From neutron stars to quark stars in mimetic gravity
• Black Hole Formation from Collapsing Dust Fluid in a Background of Dark Energy
• Cosmological model with interactions in the dark sector
• Cosmological dynamics in f(R) gravity
• Some Aspects of Tachyon Field Cosmology
• Generation of Magnetic Field in the Pre-recombination Era
• Remarks on the formulation of the cosmological constant/dark energy problems
• Structure formation in cosmologies with oscillating dark energy
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Dark energy, matter creation and curvature
• On compatibility of string effective action with an accelerating universe
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• Dark Energy Evolution and the Curvature of the Universe from Recent Observations
• Probing the curvature of the Universe from supernova measurement
• Hints of Isocurvature Perturbations in the Cosmic Microwave Background?
• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
• 2-loop Quantum Yang-Mills Condensate as Dark Energy
• Noether Symmetry Approach in multiple scalar fields Scenario
• On the Past Asymptotic Dynamics of Non-minimally Coupled Dark Energy
• Peculiar motions, accelerated expansion and the cosmological axis
• Spectroscopy of High-Redshift Supernovae from the ESSENCE Project: The First Four Years
• A Simple Model for Quintessential Inflation
• Accelerating cosmologies tested by distance measures
• Restframe I-band Hubble diagram for type Ia supernovae up to redshift z ~0.5
• Unexorcized ghost in DGP brane world
• Studying the decay of the vacuum energy with the observed density fluctuation spectrum
• Cosmological Horizon Modes and Linear Response in de Sitter Spacetime
• How to Distinguish Dark Energy and Modified Gravity?
• Implication of Dark Energy Parametrizations on the Determination of the Curvature of the Universe
• K-inflationary Power Spectra at Second Order
• Current Observational Constraints on Cosmic Doomsday
• Large-scale inhomogeneities in modified Chaplygin gas cosmologies
• Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
• Consistency of $f(R)=\sqrt{R^2-R_0^2}$ Gravity with the Cosmological Observations in Palatini Formalism
• Determining Cosmological Parameters with Latest Observational Data
• Cheng-Weyl Vector Field and its Cosmological Application
• On the equation of state of Dark Energy
• Cosmological Constraints from Hubble Parameter on f(R) Cosmologies
• Bayesian Analysis and Constraints on Kinematic Models from Union SNIa
• Measuring Dark Energy with Gamma-Ray Bursts and Other Cosmological Probes
• Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy
• Dark Energy and Right-Handed Neutrinos
• The First Type Ia Supernovae: An Empirical Approach to Taming Evolutionary Effects In Dark Energy Surveys from SNe Ia at z>2
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Unified dark fluid in Brans-Dicke theory
• Comparison between different methods of model selection in cosmology
• Dissipative or Conservative cosmology with dark energy ?
• Photometric Supernova Cosmology with BEAMS and SDSS-II
• Bayesian Analysis of the (Generalized) Chaplygin Gas and Cosmological Constant Models using the 157 gold SNe Ia Data
• Entropy perturbations and large-scale magnetic fields
• The Alcock-Paczynski test in redshifted twenty one centimeter maps
• The Hubble diagram extended to z>>1: the gamma-ray properties of GRBs confirm the Lambda-CDM model
• How close can an Inhomogeneous Universe mimic the Concordance Model?
• Transient cosmic acceleration from interacting fluids
• Reconstruction of the Primordial Power Spectrum by Direct Inversion
• Post-Newtonian expansion for Gauss-Bonnet Gravity
• Oscillations in the dark energy EoS: new MCMC lessons
• Cosmological constraints combining H(z), CMB shift and SNIa observational data
• Interacting Energy Components and Observational $H(z)$ Data
• Yang-Mills condensate dark energy coupled with matter and radiation
• Buchdahl model in f(R, T) gravity: A comparative study with standard Einstein's gravity
• Constraints on a variable dark energy model with recent observations
• 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
• Avoiding the Big-Rip Jeopardy in a Quintom Dark Energy Model with Higher Derivatives
• Do observations prove that cosmological neutrinos are thermally distributed?
• Generalized Chaplygin gas model, supernovae and cosmic topology
• New coupled quintessence cosmology
• Dark Energy or Apparent Acceleration Due to a Relativistic Cosmological Model More Complex than FLRW?
• Origin of holographic dark energy models
• Observational signatures of the weak lensing magnification of supernovae
• Cosmic vector for dark energy: constraints from SN, CMB and BAO
• Estimation of Cosmological Parameters from HI Observations of Post-reionization Epoch
• Is cosmology compatible with sterile neutrinos?
• Cosmological perturbations in Palatini modified gravity
• Measuring the cosmic proper distance from fast radio bursts
• No evidence for Dark Energy Metamorphosis ?
• Scalar field instability in de Sitter space-time
• Numerical solutions of the modified Lane-Emden equation in f(R)-gravity
• Brane-bulk energy exchange : a model with the present universe as a global attractor
• A new extensive catalog of optically variable AGN in the GOODS Fields and a new statistical approach to variability selection
• Supermassive Neutron Stars in Axion $F(R)$ Gravity
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• CFHTLS weak-lensing constraints on the neutrino masses
• Low-Ionization Emission Regions in Quasars: Gas Properties Probed with Broad O I and Ca II Lines
• Finite-time future singularities models in $f(T)$ gravity and the effects of viscosity
• On the Magnitude of Dark Energy Voids and Overdensities
• Cosmological Acceleration and Gravitational Collapse
• Cosmography by orthogonalized logarithmic polynomials
• Statefinder Diagnostic for Dilaton Dark Energy
• Lukewarm dark matter: Bose condensation of ultralight particles
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope
• Observational Constraints on Silent Quartessence
• Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
• Dissipative generalized Chaplygin gas as phantom dark energy
• Inference of the cosmic rest-frame from supernovae Ia
• Crossing the phantom barrier with purely kinetic multiple k-essence
• Current Constraints on Anisotropic and Isotropic Dark Energy Models
• Phase transition of charged Black Holes in Brans-Dicke theory through geometrical thermodynamics
• Cosmologies with General Non-Canonical Scalar Field
• A Mismatch in the Ultraviolet Spectra between Low-Redshift and Intermediate-Redshift Type Ia Supernovae as a Possible Systematic Uncertainty for Supernova Cosmology
• Supernovae in Low-Redshift Galaxy Clusters: Observations by the Wise Observatory Optical Transient Search (WOOTS)
• Dark energy: investigation and modeling
• Hubble parameter reconstruction from a principal component analysis: minimizing the bias
• The cosmic jerk parameter in f(R) gravity
• Matter may matter
• Generalized dark gravity
• Reducing distance errors for standard candles and standard sirens with weak-lensing shear and flexion maps
• The cosmology in f(R,T) gravity without dark energy
• Chaplygin gas with non-adiabatic pressure perturbations
• Is the evidence for dark energy secure?
• Dark energy as a mirage
• Classification of dark energy models in the (w_0,w_a) plane
• A study of anisotropic spheres in $f(Q)$ gravity with quintessence field
• A Type Ia Supernova at Redshift 1.55 in Hubble Space Telescope Infrared Observations from CANDELS
• One-loop f(R) Gravitational Modified Models
• Cosmic perturbations with running G and Lambda
• Theoretical upper bound on the mass of the LSP in the MNSSM
• The Effect of Weak Lensing on Distance Estimates from Supernovae
• Testing Gravity with Gravitational Waves from Binary Black Hole Mergers: Contributions from Amplitude Corrections
• Scalar Field Dark Energy Perturbations and their Scale Dependence
• Attractors, Statefinders and Observational Measurement for Chameleonic Brans--Dicke Cosmology
• The growth of linear perturbations in the DGP model
• Model independent constraints on the cosmological expansion rate
• Unified Dark Energy and Dust Dark Matter Dual to Quadratic Purely Kinetic K-Essence
• Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope
• Dark energy model with variable $q$ and $\omega$ in LRS Bianchi-II space-time
• High-redshift cosmography: Application and comparison with different methods
• Global stability analysis for cosmological models with non-minimally coupled scalar fields
• The Similarity Hypothesis in General Relativity
• Quantifying the Luminosity Evolution in Gamma-ray Bursts
• Constraining interacting dark energy with CMB and BAO future surveys
• Viscous cosmology in the Weyl-type $f(Q,T)$ gravity
• Constraining f(R) gravity with PLANCK data on galaxy cluster profiles
• Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
• Observational constraints on dark energy model
• Noise in strong lensing cosmography
• Large scale structure in the HI Parkes All-Sky Survey: Filling the Voids with HI galaxies?
• Consequences of energy conservation violation: Late time solutions of $\Lambda (T)CDM$ subclass of $f(R,T)$ gravity using dynamical system approach
• Quantum Corrections to the Accretion onto a Schwarzschild Black Hole in the Background of Quintessence
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Revisiting the parametrization of Equation of State of Dark Energy via SNIa Data
• Probing decisive answers to dark energy questions from cosmic complementarity and lensing tomography
• Inhomogeneity-Induced Cosmic Acceleration in a Dust Universe
• Dark Energy from a Phantom Field Near a Local Potential Minimum
• Entropic cosmology in a dissipative universe
• Role of the Brans-Dicke scalar in the holographic description of dark energy
• Accelerating universe in scalar tensor models - confrontation of theoretical predictions with observations
• Age constraints on the cosmic equation of state
• SNR-calibrated Type Ia supernova models
• Lorentz Invariance Violation induced time delays in GRBs in different cosmological models
• Hubble Space Telescope Observations of Nine High-Redshift ESSENCE Supernovae
• Cosmology from supernova magnification maps
• How well will ton-scale dark matter direct detection experiments constrain minimal supersymmetry?
• Late Decaying Dark Matter, Bulk Viscosity and the Cosmic Acceleration
• Fresh look at the scalar-tensor theory of gravity in Jordan and Einstein frames from undiscussed standpoints
• Evolving to type Ia supernovae with long delay time
• Nonparametric reconstruction of the cosmic expansion with local regression smoothing and simulation extrapolation
• Redshift Accuracy Requirements for Future Supernova and Number Count Surveys
• Reconstruction Procedure in Nonlocal Cosmological Models
• The effect of baryons in the cosmological lensing PDFs
• An Interacting Dark Energy Model for the Expansion History of the Universe
• Bulk viscous embedded hybrid dark energy models
• Extended Chaplygin Gas in Horava-Lifshitz Gravity
• Description of our cosmological spacetime as a perturbed conformal Newtonian metric and implications for the backreaction proposal for the accelerating universe
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• Light curves for off-centre ignition models of type Ia supernovae
• Stringy Dark Energy Model with Cold Dark Matter
• Time drift of cosmological redshifts and its variance
• Model of Mass Varying Neutrinos in SUSY
• Hidden past of dark energy cosmological models
• Dynamically avoiding fine-tuning the cosmological constant: the "Relaxed Universe"
• Dark radiation and dark matter coupled to holographic Ricci dark energy
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• Using Ultra Long Period Cepheids to Extend the Cosmic Distance Ladder to 100 Mpc and Beyond
• On Wormholes supported by phantom energy
• Lensing and Supernovae: Quantifying The Bias on the Dark Energy Equation of State
• Phantom-Like Behavior in $f(R)$-Gravity
• Beyond H_0 and q_0: Cosmology is no longer just two numbers
• Invariance under complex transformations, and its relevance to the cosmological constant problem
• Type Ia Supernovae and Cosmology
• Effective equation of state for running vacuum: "mirage" quintessence and phantom dark energy
• Evolution of Oscillating Scalar Fields as Dark Energy
• Towards a Realistic Type IIA T^6/Z_4 Orientifold Model with Background Fluxes, Part 1: Moduli Stabilization
• Supernovae Ia observations in the Lemaitre--Tolman model
• Present Acceleration of Universe, Holographic Dark Energy and Brans-Dicke Theory
• Extremely Luminous Water Vapor Emission from a Type 2 Quasar at Redshift z = 0.66
• Stellar Structures in $f(\mathcal{G})$ Gravity with Tolman-Kuchowicz Spacetime
• Coupled Quintessence and Phantom Based On a Dilaton
• Modified Einstein's gravity to probe the sub- and super-Chandrasekhar limiting mass white dwarfs: a new perspective to unify under- and over-luminous type Ia supernovae
• Modified Holographic Dark Energy
• Stability of Anisotropic Stellar Filaments
• The variation of the gravitational constant inferred from the Hubble diagram of Type Ia supernovae
• Constraints on the Parameterized Deceleration Parameter in FLRW Universe
• Spectroscopic confirmation of high-redshift supernovae with the ESO VLT
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• Cosmological dynamics of fourth order gravity: A compact view
• Cosmological Solutions of a Nonlocal Model with a Perfect Fluid
• Global and Local Effects of Rotation: Observational Aspects
• A step towards testing general relativity using weak gravitational lensing and redshift surveys
• Bayesian Evidence for a Cosmological Constant using new High-Redshift Supernovae Data
• Tension in the Recent Type Ia Supernovae Datasets
• A Model to Explain Varying $\Lambda$, $G$ and ${\sigma }^2$ Simultaneously
• The thawing dark energy dynamics: Can we detect it?
• On the Stability of Jordan-Brans-Dicke Static Universe
• Testing the DGP model with ESSENCE
• Does the Big Rip survive quantization?
• Renormalization group scale-setting in astrophysical systems
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• Estimating relic magnetic fields from CMB temperature correlations
• Testing the Distance-Duality Relation with a Combination of Cosmological Distance Observations
• Scaling solutions in scalar-tensor cosmologies
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Reconstructing K-essence
• On Anisotropic Dark Energy
• Connecting LHC, ILC, and Quintessence
• Spectroscopic Observations and Analysis of the Unusual Type Ia SN 1999ac
• Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational data
• A Probabilistic Approach to Classifying Supernovae Using Photometric Information
• Bianchi Type-I Cosmological Models with Variable G and 4Λ$-Terms in General Relativity
• The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < z < 1.46
• Probing cosmic opacity at high redshifts with gamma-ray bursts
• Measuring dark energy spatial inhomogeneity with supernova data
• An Axially Symmetric Transitioning models with Observational Constraints
• Domain Walls As Probes Of Gravity
• Dark energy and dark matter from cosmological observations
• Rotating Neutron Stars in F(R) Gravity with Axions
• Narrowing Constraints with Type Ia Supernovae: Converging on a Cosmological Constant
• Constraining the Asymptotically Safe Cosmology: cosmic acceleration without dark energy
• Light Deflection, Lensing, and Time Delays from Gravitational Potentials and Fermat's Principle in the Presence of a Cosmological Constant
• Noether analysis of Scalar-Tensor Cosmology
• Transition Redshift: New constraints from parametric and nonparametric methods
• Reconstructing the interaction rate in holographic models of dark energy
• Crossing of the w=-1 Barrier in Two-Fluid Viscous Modified Gravity
• A parametrization for the growth index of linear matter perturbations
• Modified holographic Ricci dark energy coupled to interacting dark matter and a non interacting baryonic component
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Towards testing interacting cosmology by distant type Ia supernovae
• New Agegraphic Dark Energy in $f(R)$ Gravity
• When Did Cosmic Acceleration Start ?
• Higher derivative corrections of $f(R)$ gravity with varying equation of state in the case of variable $G$ and $\Lambda$
• Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land
• Some remarks about non-minimally coupled scalar field models
• The signature of dark energy perturbations in galaxy cluster surveys
• Using a phenomenological model to test the coincidence problem of dark energy
• The Redshift Sensitivities of Dark Energy Surveys
• The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models
• Transitioning Universe with hybrid scalar field in Bianchi I space-time
• Dynamics in nonlocal linear models in the Friedmann-Robertson-Walker metric
• New Constraints on Macroscopic Compact Objects as a Dark Matter Candidate from Gravitational Lensing of Type Ia Supernovae
• From Primordial Quantum Fluctuations to the Anisotropies of the Cosmic Microwave Background Radiation
• On de Sitter Vacua in Type IIA Orientifold Compactifications
• Stability analysis and Observational Measurement in Chameleonic Generalised Brans--Dicke Cosmology
• Stable Exact Solutions in Cosmological Models with Two Scalar Fields
• Anisotropic compact stars in the mimetic gravitational theory
• Interacting new agegraphic viscous dark energy with varying $G$
• Bulk Viscous LRS Biachi-I Universe with variable $G$ and decaying $\Lambda$
• The accelerating universe and a limiting curvature proposal
• Brane Cosmological Evolution With Bulk Matter
• Susskind's Challenge to the Hartle-Hawking No-Boundary Proposal and Possible Resolutions
• Statefinder Parameters for Interacting Phantom Energy with Dark Matter
• Cosmic Constraint on Ricci Dark Energy Model
• A new perspective on the relation between dark energy perturbations and the late-time ISW effect
• Observational Constraints on Accelerating Brane Cosmology with Exchange between the Bulk and Brane
• Relaxing a large cosmological constant
• General approach to the Lagrangian ambiguity in $f(R,T)$ gravity
• Exotic solutions in General Relativity: Traversable wormholes and 'warp drive' spacetimes
• Logarithmic corrected Polynomial $f(R)$ inflation mimicking a cosmological constant
• Corrections for gravitational lensing of supernovae: better than average?
• $\Lambda$-CDM Universe: A Phenomenological Approach With Many Possibilities
• The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
• Detectability of a phantom-like braneworld model with the integrated Sachs-Wolfe effect
• The REFLEX II galaxy cluster survey: power spectrum analysis
• The Laminar Flame Speedup by Neon-22 Enrichment in White Dwarf Supernovae
• Fitting Non-Minimally Coupled Scalar Models to Gold SnIa Dataset
• DGP Cosmology with a Non-Minimally Coupled Scalar Field on the Brane
• Remarks on Dynamical Dark Energy Measured by the Conformal Age of the Universe
• Calibrating Type Ia Supernovae using the Planetary Nebula Luminosity Function I. Initial Results
• Dynamical Evolution of Interacting Modified Chaplygin Gas
• Lensing magnification of supernovae in the GOODS-fields
• Composite dark energy: cosmon models with running cosmological term and gravitational coupling
• Weak lensing signal in Unified Dark Matter models
• Reconstruction of $f(Q,T)$ Lagrangian for various cosmological scenario
• Extended Born-Infeld Dynamics and Cosmology
• Constraining non-minimally coupled tachyon fields by Noether symmetry
• Confronting the relaxation mechanism for a large cosmological constant with observations
• Comparison of Recent SnIa datasets
• Continuous phase transition and microstructure of charged AdS black hole with quintessence
• Extended phase space thermodynamics and $P-V$ criticality: Brans-Dicke-Born-Infeld vs Einstein-Born-Infeld-dilaton black holes
• Generalized Second Law of Thermodynamic in Modified Teleparallel Theory
• Cosmological perturbations in SFT inspired non-local scalar field models
• Accelerating Universes from Compactification on a Warped Conifold
• Cosmological constraints with GRBs: homogeneous medium vs wind density profile
• Effects of inhomogeneities on apparent cosmological observables: "fake" evolving dark energy
• Beyond Two Dark Energy Parameters
• Reduction of Cosmological Data for the Detection of Time-varying Dark Energy Density
• Reconstructing a String-Inspired Quintom Model of Dark Energy
• Scalar field mass in generalized gravity
• New Constraints On The Dark Energy Equation of State
• Tensions with the flat $\mathbf{\Lambda }$CDM model from high-redshift cosmography
• Confronting pNGB quintessence with data
• Observational Constraints of Modified Chaplygin Gas in Loop Quantum Cosmology
• Hybrid natural inflation from non Abelian discrete symmetry
• A New $Om(z)$ Diagnostic of Dark Energy in General Relativity Theory
• Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?
• Coupled quintessence and vacuum decay
• Two-fluid atmosphere from decelerating to accelerating FRW dark energy models
• New Agegraphic Dark Energy in Brans-Dicke Theory
• Can $f(T)$ models play a bridge between early and late time Universe?
• Late-time cosmology in $f(Q,L_m)$ gravity: Analytical solutions and observational fits
• Observational constraints on generalized Chaplygin gas model
• Constraints on Dark Energy Models Including Gamma Ray Bursts
• Gravitational lensing in the Supernova Legacy Survey (SNLS)
• Baryon Acoustic Oscillations and Dynamical Dark Energy
• Dynamical instability of fluid spheres in the presence of a cosmological constant
• Optical Polarimetry of the Jets of Nearby Radio Galaxies: I. The Data
• Cosmography, Decelerating Past, and Cosmological Models: Learning the Bayesian Way
• Rotating charged black holes shadow in quintessence
• Dark viscous fluid described by a unified equation of state in cosmology
• Couplings between holographic dark energy and dark matter
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Measuring the Chaplygin gas equation of state from angular and luminosity distances
• GALEX Spectroscopy of SN 2005ay suggests a UV spectral uniformity among type II-P supernovae
• Tsallis holographic dark energy in Fractal Universe
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Power-law solution for homogeneous and isotropic universe in $f(R,T)$ gravity
• Dynamics of perfect fluid Unified Dark Energy models
• The growth factor of matter perturbations in an f(R) gravity
• Cosmic Acceleration From Matter-Curvature Coupling
• Problems with Pencils: Lensing Covariance of Supernova Distance Measurements
• Dark energy and decompactification in string gas cosmology
• Dark energy, gravitation and supernovae
• Legacy data and cosmological constraints from the angular-size/redshift relation for ultra-compact radio sources
• UV surface brightness of galaxies from the local Universe to z ~ 5
• Position and frequency shifts induced by massive modes of the gravitational wave background in alternative gravity
• Bright High z SnIa: A Challenge for LCDM?
• Effects of f(R) Dark Energy on Dissipative Anisotropic Collapsing Fluid
• How strong is the evidence for accelerated expansion?
• Constraining $f(Q,L_m)$ gravity with bulk viscosity
• Equation of state for Universe from similarity symmetries
• A Model for Dark Energy decay
• Revisiting f(R) gravity models that reproduce $\Lambda$CDM expansion
• Viscous Dark Energy In Bianchi Type V Space-Time
• LTB universes as alternatives to dark energy: does positive averaged acceleration imply positive cosmic acceleration?
• Cosmological Constant Problems and Renormalization Group
• Study Of Tachyon Dynamics For Broad Classes of Potentials
• Beyond delta: Tailoring marked statistics to reveal modified gravity
• Cosmography with cluster strong lensing
• Effects of Cosmological Constant on Clustering of Galaxies
• Direction Dependent Non-gaussianity in High-z Supernova Data
• Observational analysis of late-time acceleration in $f(Q,L_m)$ gravity
• Multiple kinetic k-essence, phantom barrier crossing and stability
• A Kinematical Approach to Conformal Cosmology
• The SNAP Strong Lens Survey
• Comparing two approaches to Hawking radiation of Schwarzschild-de Sitter black holes
• Defining Photometric Peculiar Type Ia Supernovae
• Modeling Transit Dark Energy in $f(R,L_m)$-gravity
• Localization of nonlocal cosmological models with quadratic potentials in the case of double roots
• Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data
• Duality extended Chaplygin cosmologies with a big rip
• The Twins Embedding of Type Ia Supernovae II: Improving Cosmological Distance Estimates
• FLRW cosmology with EDSFD parametrization
• Red and Reddened: Ultraviolet through Near-Infrared Observations of Type Ia Supernova 2017erp
• Crossing of $\omega =-1$ with Tachyon and Non-minimal Derivative Coupling
• New Generalizations of Cosmography Inspired by the Pade Approximant
• Optical and Near-Infrared Observations of the Peculiar Type Ia Supernova 1999ac
• The most general fourth order theory of Gravity at low energy
• Supernova light-curve fitters and Dark Energy
• Accelerated Expansion of the Universe in Gauss-Bonnet Gravity
• Solar system tests of f(R) gravity
• Phantom evolving wormholes with big rip singularities
• Post-Newtonian Approximation of Teleparallel Gravity Coupled with a Scalar Field
• Patchy He II reionization and the physical state of the IGM
• Scale Factor Dependent Equations of State for Curvature Inspired Dark Energy, Phantom Barrier and Late Cosmic Acceleration
• Cold Dark Matter in non-Standard Cosmologies, PAMELA, ATIC and Fermi LAT
• Semi-analytical approach to magnetized temperature autocorrelations
• Scalar field and time varying Cosmological constant in $f(R,T)$ gravity for Bianchi type-I Universe
• A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Soft coincidence in late acceleration
• Chameleonic Generalized Brans--Dicke model and late-time acceleration
• Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha
• Thermal fluctuations, quasi-normal modes and phase transition of the charged AdS black hole with perfect fluid dark matter
• Phenomenology of $\Lambda$-CDM model: a possibility of accelerating Universe with positive pressure
• Magnetized Bianchi Type $V{I}_0$ Barotropic Massive String Universe with Decaying Vacuum Energy Density $\Lambda$
• Anisotropic universe with anisotropic sources
• Variable Cosmological Constant model: the reconstruction equations and constraints from current observational data
• Cosmological consequences and statefinder diagnosis of a non-interacting generalized Chaplygin gas in $f(R,T)$ gravity
• The CMB spectrum in Cardassian models
• Late time Acceleration and Role of Skewness in Anisotropic models
• Corrections to the apparent value of the cosmological constant due to local inhomogeneities
• A Comparison of Cosmological Models Using Strong Gravitational Lensing Galaxies
• A Geometrical Approach to Strong Gravitational Lensing in f(R) Gravity
• Brans-Dicke Scalar Field Cosmological Model in Lyra's Geometry
• Parameter dependence of magnetized CMB observables
• Existence of black holes in Friedmann-Robertson-Walker universe dominated by dark energy
• Quantifying systematic uncertainties in supernova cosmology
• WMAP 5-year constraints on lepton asymmetry and radiation energy density: Implications for Planck
• Attractor behaviour of $f(T)$ modified gravity and the cosmic acceleration
• Quintessential Kination and Thermal Production of Gravitinos and Axinos
• Supernova Constraints on Models of Neutrino Dark Energy
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• Effective growth of matter density fluctuations in the running LCDM and LXCDM models
• Fluid observers and tilting cosmology
• Are Swift gamma-ray bursts consistent with the Ghirlanda relation?
• Complementary Constraints on Brane Cosmology
• Constraints on Energy Momentum Squared Gravity from cosmic chronometers and Supernovae Type Ia data
• Dissipative Liouville Cosmology: A Case Study
• Direct evidence of acceleration from distance modulus redshift graph
• Generalized Chaplygin gas and accelerating universe in $f(Q,T)$ gravity
• Extended quintessence, inflation, and stable de Sitter spaces
• Constraining the Schwarzschild-de Sitter Solution in Models of Modified Gravity
• Analysis of scalar perturbations in cosmological models with a non-local scalar field
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Naked Singularity Formation In f(R) Gravity
• A Closer Earth and the Faint Young Sun Paradox: Modification of the Laws of Gravitation, or Sun/Earth Mass Losses?
• Brane inflation driven by noncanonical scalar field
• Cosmological constraints for an Eddington-Born-Infeld field
• Unsuccessful cosmology with Modified Gravity Models
• Post-Planck Dark Energy Constraints
• Modified Dispersion Relations from the Renormalization Group of Gravity
• Direction Dependence in Supernova Data: Constraining Isotropy
• Accelerating Bianchi Type-V Cosmology with Perfect Fluid and Heat Flow in Saez-Ballester Theory
• Investigating the origins of the CMB-XRB cross correlation
• Two Component Model of Dark Energy
• Reconstructing the history of dark energy using maximum entropy
• Probing Neutrino Dark Energy with Extremely High-Energy Cosmic Neutrinos
• Current Acceleration from Dilaton and Stringy Cold Dark Matter
• Gravitational waves in the presence of a cosmological constant
• Why Does Gravity Ignore the Vacuum Energy?
• Hybrid Natural Low Scale Inflation
• Including Absorption in Gordon's Optical Metric
• Atypical k-essence cosmologies
• Did Boomerang hit MOND?
• Observational tests of the self-dual spacetime in loop quantum gravity
• Do the observational data favor a local void?
• Cosmology with Ricci dark energy
• Modifications by QCD transition and $e^{+}{e}^{-}$ annihilation on analytic spectrum of relic gravitational waves in accelerating universe
• Cosmological models with a Hybrid Scale Factor
• Implications from simulated strong gravitational lensing systems: constraining cosmological parameters using Gaussian Processes
• Dilatonic Equation of Hydrostatic Equilibrium and Neutron Star Structure
• Genesis of Dark Energy: Dark Energy as Consequence of Release and Two-stage Tracking Cosmological Nuclear Energy
• Dark radiation as a signature of dark energy
• On covariant long-distance modifications of Einstein theory and strong coupling problem
• Cosmological constant and late transient acceleration of the universe in the Horava-Witten Heterotic M-Theory on S^{1}/Z_{2}
• Some Impacts of Lorentz Violation on Cosmology
• Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12
• Modified Chaplygin Gas Cosmology with Bulk Viscosity
• Power Spectra to 1% Accuracy between Dynamical Dark Energy Cosmologies
• Constraining the $f(R,T)=R+2\lambda T$ cosmological model using recent observational data
• Large-scale galaxy correlations as a test for dark energy
• Observational constraint on the interacting dark energy models including the Sandage-Loeb test
• What Can Gamma Ray Bursts Teach Us About Dark Energy?
• Quantum vacuum, dark matter, dark energy and spontaneous supersymmetry breaking
• Reconstruction of interacting dark energy models from parameterizations
• Galactic rotation curves and brane world models
• Light curves of five type Ia supernovae at intermediate redshift
• Curvature Singularities from Gravitational Contraction in f(R) Gravity
• A $f(R)$-gravity model of the Sunyaev-Zeldovich profile of the Coma cluster compatible with {\it Planck} data
• Clustering of Galaxies with Dynamical Dark Energy
• Dark energy interacting with two fluids
• Luminosity distance-redshift relation for the LTB solution near the center
• Filtering out the cosmological constant in the Palatini formalism of modified gravity
• Interacting cosmic fluids in power-law Friedmann-Robertson-Walker cosmological models
• The dependency of Type Ia Supernova parameters on host galaxy morphology for the Pantheon cosmological sample
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• Data Analysis of three parameter models of deceleration parameter in FRW Universe
• The Post-Newtonian Limit of f(R)-gravity in the Harmonic Gauge
• Cosmographic analysis of a closed bouncing universe with the varying cosmological constant in $f(R,T)$ gravity
• Dark energy from bulk matter
• Generalized CMB initial conditions with pre-equality magnetic fields
• Galaxy surveys, inhomogeneous reionization, and dark energy
• Assisted dark energy
• Exact cosmological solution of a Scalar-Tensor Gravity theory compatible with the $\Lambda CDM$ model
• Model- and calibration-independent test of cosmic acceleration
• Superpotential method for chiral cosmological models connected with modified gravity
• Bouncing universe with the non-minimally coupled scaler field and its reconstructing
• Effects of early dark energy on strong cluster lensing
• Breakdown of the initial value formulation of scalar-tensor gravity and its physical meaning
• Dark-Energy Dynamics Required to Solve the Cosmic Coincidence
• Thermodynamics of the Variable Modified Chaplygin gas
• High-energetic Cosmic Antiprotons from Kaluza-Klein Dark Matter
• Dark Energy and Dark Matter unification via superfluid Chaplygin gas
• Anisotropic k-essence cosmologies
• Non-chaotic dynamics in general-relativistic and scalar-tensor cosmology
• Composition-dependent long range forces from varying m_p/m_e
• L.R.S. Bianchi type II Stiff Fluid cosmological model with Decaying Vacuum Energy Density $\Lambda$ in general relativity
• Geometrical Constraints on Dark Energy
• Investigating scalar-tensor-gravity with statistics of the cosmic large-scale structure
• Supernovae and Cosmology
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• The conformal status of $\omega =-3/2$ Brans-Dicke cosmology
• Evolution of spherical overdensities in holographic dark energy models
• Variable Chaplygin Gas: Constraints from CMBR and SNe Ia
• Constraining the dark energy statefinder hierarchy in a kinematic approach
• Holographic Dark Energy from a Modified GBIG Scenario
• Cosmic microwave background radiation temperature in a dissipative universe
• Maximal Masses of White Dwarfs for Polytropes in $R^2$ Gravity and Theoretical Constraints
• A new method to measure the virial factors in the reverberation mapping of AGNs
• Black hole and holographic dark energy
• Cosmological constant dominated transit universe from early deceleration to current acceleration phase in Bianchi-V space-time
• Anisotropic String Cosmological Models in Heckmann-Suchuking Space-Time
• A magnetized completion of the $\Lambda$CDM paradigm
• Can a dust dominated universe have accelerated expansion?
• Probing the physical and mathematical structure of $f(R)$ gravity by PSR $J0348+0432$
• An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• Some FRW Models of Accelerating Universe with Dark Energy
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• Large Scale Structure Formation of Normal Branch in DGP Brane World Model
• The flatness problem and $\Lambda$
• Stealth Acceleration and Modified Gravity
• R^n gravity and the chameleon
• Observational Constraints with Recent Data on the DGP Modified Gravity
• A Realistic Particle Physics Dark Energy Model
• Power-law Parameterized Quintessence Model
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Late-time acceleration and Phantom Divide Line Crossing with Non-minimal Coupling and Lorentz Invariance Violation
• Bayesian Statistics and Parameter Constraints on the Generalized Chaplygin Gas Model using SNe Ia Data
• Model for a Universe described by a non-minimally coupled scalar field and interacting dark matter
• Pre-Inflationary Spacetime in String Cosmology
• Null Energy Condition Violation and Classical Stability in the Bianchi I Metric
• Undulant Universe
• Dynamics of Modified Chaplygin Gas in Brane World Scenario: Phase Plane Analysis
• SNLS data are consistent with acceleration at z=3
• The Cosmological Constant Problem, an Inspiration for New Physics
• Crossing the Phantom Divide Line in a DGP-Inspired $F(R,\varphi )$-Gravity
• The dynamical viability of scalar-tensor gravity theories
• Dark energy parameterizations and their effect on dark halos
• Early and Late Transient Cosmic Acceleration due to Curvature Inspired Dark Energy
• Dark matter, and its darkness
• Current-carrying string loops in black-hole spacetimes with a repulsive cosmological constant
• Quantum backreaction in evolving FLRW spacetimes
• Cosmology and thermodynamics of FRW universe with bulk viscous stiff fluid
• Infinity in string cosmology: A review through open problems
• A Cyclic Universe With Varying Cosmological Constant in $f(R,T)$ gravity
• Analysis of galaxy kinematics based on Cepheids from the Gaia DR2 Catalogue
• Cosmological constraints on dark energy models using DESI BAO 2024
• A model independent approach to the study of $f(R)$ cosmologies with expansion histories close to $\Lambda$CDM
• Unified Dark Fluid and Cosmic Transit Models in Brans-Dicke Theory
• How Problematic is the Near-Euclidean Spatial Geometry of the Large-Scale Universe?
• Accelerated Expansion of the Universe based on Emergence of Space and Thermodynamics of the Horizon
• Bianchi type-I transit cosmological models with time dependent gravitational and cosmological constants - reexamined
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• Model-Independent Reconstruction of the Expansion History of the Universe from Type Ia Supernovae
• Observational Constraints on Interacting Dark Matter Model Without Dark Energy
• Bianchi Type-II String Cosmological Models in Normal Gauge for Lyra's Manifold with Constant Deceleration Parameter
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Cosmological Evolution of a Tachyon-Quintom Model of Dark Energy
• Revisiting the Magnification of Type Ia Supernovae with SDSS
• Photometric Classification of 2315 Pan-STARRS1 Supernovae with Superphot
• Gamma-ray Observations of Explosive Nucleosynthesis Products
• Measuring Unified Dark Matter with 3D Cosmic Shear
• Cosmological Evolution and Solar System Consistency of Massive Scalar-Tensor Gravity
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Vector field and rotational curves in dark galactic halos
• Cosmological Evolution Across Phantom Crossing and the Nature of the Horizon
• Palatini f(R) gravity as a fixed point
• Particle mixing, flavor condensate and dark energy
• Does fractal Universe describe a complete cosmic scenario?
• Multi-graviton theory from a discretized RS brane-world and the induced cosmological constant
• Cosmology of non-minimal derivative coupling to gravity in Palatini formalism and its chaotic inflation
• Neutrino masses and mixings in the baryon triality constrained minimal supersymmetric standard model
• Transit String Dark Energy Models in $f(Q)$ Gravity
• Quantum fields and "Big Rip" expansion singularities
• Holographic dark energy and late cosmic acceleration
• Geodesic Structure of the Quantum-Corrected Schwarzschild Black Hole Surrounded by Quintessence
• Traversable wormholes with logarithmic shape function in f(R, T) gravity
• Late-time phantom universe in $\mathbf{SO}(1,1)$ dark energy model with exponential potential
• Understanding the origin of CMB constraints on Dark Energy
• On astrophysical bounds of the cosmological constant
• Oxidised cosmic acceleration
• Imprint of Scalar Dark Energy on Cosmic Microwave Background Polarization
• An exponential shape function for wormholes in modified gravity
• Holographic dark energy: constraints on the interaction from diverse observational data sets
• Reconstructing a model of quintessential inflation
• Dark energy models toward observational tests and data
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Bayesian Model Averaging in Astrophysics: A Review
• Exact Cosmology in Myrzakulov Gravity
• Modified GBIG Scenario as an Alternative for Dark Energy
• Anisotropic charged dark energy star
• Single-Field Inflation After WMAP5
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Isotropic compact stars in 4D Einstein-Gauss-Bonnet gravity
• A Model-Independent Photometric Redshift Estimator for Type Ia Supernovae
• Rotation Curves of Galaxies by Fourth Order Gravity
• Tangled magnetic fields and CMBR signal from reionization epoch
• Compact stellar models in modified gravity
• Reconstructing the History of Energy Condition Violation from Observational Data
• Phenomenological Reconstruction of $f(T)$ Teleparallel Gravity
• The present universe in the Einstein frame, metric-affine R+1/R gravity
• Gauge Formulation for Higher Order Gravity
• Dynamics of Interacting Generalized Cosmic Chaplygin gas in Brane-world scenario
• Using the Topology of Large Scale Structure to constrain Dark Energy
• Mimicking the cosmological constant for more than one observable with large scale inhomogeneities
• Physical Parameters for Stable $f(R)$ Models
• The flavor vacuum in the expanding universe and dark matter
• A Braneworld Dark Energy Model with Induced Gravity and the Gauss-Bonnet Effect
• Study of eccentric binaries in Horndeski theory
• Acceleration of string loops in the Schwarzschild-de Sitter geometry
• Cosmic Dynamics in $F(R,\varphi )$ Gravity
• Cosmological Consequences of New Dark Energy Models in Einstein-Aether Gravity
• Cosmic microwave background and large-scale structure constraints on a simple quintessential inflation model
• Moving dark energy and the CMB dipole
• Asymptotically Lifshitz black hole solutions in F(R) gravity
• Accelerated expansion from cosmological holography
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Holographic kinetic k-essence model
• Viscous Generalized Chaplygin Gas as a Unified Dark Fluid: Including Perturbation of Bulk Viscosity
• The Influence of Free Quintessence on Gravitational Frequency Shift and Deflection of Light with 4D momentum
• Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
• Can we test Dark Energy with Running Fundamental Constants ?
• Dark Energy Accretion onto a Black Hole in an Expanding Universe
• Neutrino mass bounds from cosmology
• Growth of structure in interacting vacuum cosmologies
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• Accelerating Dark Energy Cosmological Model in Two Fluid with Hybrid Scale Factor
• A conventional approach to the dark-energy concept
• Can the cosmological constant be mimicked by smooth large-scale inhomogeneities for more than one observable?
• Clifton's spherical solution in f(R) vacuo harbours a naked singularity
• Analytic charged BHs in $f(\mathcal{R})$ gravity
• Quintessential power-law cosmology: dark energy equation of state
• Noether gauge symmetry for the Bianchi type I model in f(T) gravity
• Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
• Neutron stars in Einstein-$\Lambda$ gravity: the cosmological constant effects
• Observational constraints on the dark energy density evolution
• Tentative detection of the gravitational magnification of type Ia supernovae
• Dark Energy, A Cosmological Constant, and Type Ia Supernovae
• Boson mixing and flavor vacuum in the expanding Universe: a possible candidate for the dark energy
• Dynamical Relaxation of the Dark Matter to Baryon Ratio
• Complementary constraints from FR IIb radio galaxies and X-ray gas mass fractions in clusters on non-standard cosmological models
• Statistical coverage for supersymmetric parameter estimation: a case study with direct detection of dark matter
• Oscillating universe in the DGP braneworld
• Fixed points and FLRW cosmologies: Flat case
• Inhomogeneous Perfect Fluid Universe with Electromagnetic Field in Lyra Geometry
• Scalar-multi-tensorial equivalence for higher order $f\left(R,{\nabla }_{\mu }R,{\nabla }_{{\mu }_1}{\nabla }_{{\mu }_2}R,...,{\nabla }_{{\mu }_1}...{\nabla }_{{\mu }_n}R\right)$ theories of gravity
• Thermodynamics of phantom energy in the presence of a Reissner-Nordstrom black hole
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Cosmology with variable parameters and effective equation of state for Dark Energy
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• The dynamics of matter bounce cosmology in Weyl-type $f(Q,T)$ gravity
• The Effect of Type Ibc Contamination in Cosmological Supernova Samples
• Do cosmological data rule out $f(\mathcal{R})$ with $w\ne -1$?
• Interpretations of gamma-ray burst spectroscopy. II. Bright BATSE bursts
• Can the initial singularity be detected by cosmological tests?
• Cosmography and large scale structure by f(R) gravity: new results
• The Accelerating Universe
• First-order formalism for dark energy and dust
• A Lemaitre-Tolman-Bondi cosmological wormhole
• Astrophysical Signatures of Black holes in Generalized Proca Theories
• First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Effects of Chromatic Corrections to Supernova Photometry on Measurements of Cosmological Parameters
• Friedmann cosmology with decaying vacuum density in Brans-Dicke theory
• The trace of the trace of the energy-momentum tensor-dependent Einstein's field equations
• Modeling cosmic acceleration with a generalized varying deceleration parameter
• GRB neutrinos, Lorenz Invariance Violation and the influence of background cosmology
• Curvature Inspired Cosmological Scenario
• Brane Cosmology with a Non-Minimally Coupled Bulk-Scalar Field
• Sourced Friedmann equations with holographic energy density
• Cosmological Symmetry Breaking, Pseudo-scale invariance, Dark Energy and the Standard Model
• Constraints on accelerating universe using ESSENCE and Gold supernovae data combined with other cosmological probes
• Crossing of the Phantom Divided Barrier with Lorentz Invariance Violating Fields
• Inflation, Large Branes, and the Shape of Space
• High-resolution imaging of the cosmic mass distribution from gravitational lensing of pregalactic HI
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• Thermodynamics of Spinor Quintom
• Fields of accelerated sources: Born in de Sitter
• Comparison of Frames: Jordan vs Einstein Frame for a Non-minimal Dark Energy Model
• New Constraints on the Variable Equation of State Parameter from X-Ray Gas Mass Fractions and SNe Ia
• Coincidence Problem in an Oscillating Universe
• On the future of Gamma-Ray Burst Cosmology
• Universe With Time Dependent Deceleration Parameter and $\Lambda$ Term in General Relativity
• The Averaging Problem in Cosmology
• A fluid os strings as a viable candidate to the dark side of the universe
• Instability of Chaplygin gas trajectories in unified dark matter models
• Interacting modified holographic Ricci dark energy model and statefinder diagnosis in flat universe
• On the cosmological evolution of alpha and mu and the dynamics of dark energy
• Anisotropic f(Q) gravity model with bulk viscosity
• Non-singular Brans-Dicke cosmology with cosmological constant
• Scalar field cosmology in phase space
• Cosmology under Milne's shadow
• Higher neutrino mass allowed if Cold Dark Matter and Dark Energy are coupled
• Transient Crossing of Phantom divide line $w_{\Lambda }=-1$ under Gauss-Bonnet interaction
• Cosmological models in scalar tensor theories of gravity and observations: a class of general solutions
• Exponential Cardassian Universe
• Parameterizing and Measuring Dark Energy Trajectories from Late-Inflatons
• Constraining Dark Energy and Cosmological Transition Redshift with Type Ia Supernovae
• Cosmological constraints from Radial Baryon Acoustic Oscillation measurements and Observational Hubble data
• Cosmology With Non-Minimally Coupled K-Field
• Constraint on Cosmological Model with Matter Creation Using Complementary Astronomical Observations
• A solution of the dark energy and its coincidence problem based on local antigravity sources without fine-tuning or new scales
• Quantum corrected thermodynamics of nonlinearly charged BTZ black holes in massive gravity's rainbow
• Geometrical Diagnostics for Generalized Chaplygin Gas
• Testing Cosmological General Relativity against high redshift observations
• The Standard Cosmological Model
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• Geodesic Model of HF QPOs Tested for Black Holes in Spacetimes Reflecting the Effect of Surrounding Dark Matter
• Testing homogeneity with galaxy number counts : light-cone metric and general low-redshift expansion for a central observer in a matter dominated isotropic universe without cosmological constant
• Dilaton Coupled Quintessence Model in the $\omega -{\omega }^{\prime }$ Plane
• Induced Phantom and 5D Attractor Solution in Space-Time-Matter Theory
• Born-Infeld Type Phantom Model in the $\omega -{\omega }^{\prime }$ Plane
• Cosmological Consequences of a Variable Cosmological Constant Model
• Anisotropic Dark Energy Bianchi Type III Cosmological Models in Brans Dicke Theory of Gravity
• Disorder on the landscape
• Accurate Extra-Galactic Distances and Dark Energy: Anchoring the Distance Scale with Rotational Parallaxes
• Light curve studies of nearby Type Ia Supernovae with a Multi-band Stretch method
• A Redshift Dependent Color-Luminosity Relation in Type 1a Supernovae
• Interacting Dark Energy: Decay into Fermions
• Inverse problem: Reconstruction of modified gravity action in Palatini formalism by Supernova Type Ia data
• A Model of Dark Energy and Dark Matter
• Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae
• Cosmological bounds on oscillating dark energy models
• Universe opacity and Type Ia supernova dimming
• Gamma Rays Bursts: A Viable Cosmological Probe?
• Cosmic holographic bounds with UV and IR cutoffs
• Inflationary susceptibilities, duality and large-scale magnetic fields generation
• Constraints on the Cardassian Expansion from the Cosmic Lens All-Sky Survey Gravitational Lens Statistics
• Bayesian constraints on dark matter halo properties using gravitationally-lensed supernovae
• Inflation and Quintessence: Theoretical Approach of Cosmological Reconstruction
• Friedmann Equation for Brans Dicke Cosmology
• Inflessence: a phenomenological model for inflationary quintessence
• Constraints on supernovae dimming from photon-pseudo scalar coupling
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Cosmological Constant and Local Gravity
• Stability analysis of f(Q) gravity models using dynamical systems
• Self-interacting holographic dark energy
• SuperNova Acceleration Probe (SNAP): Investigating Photometric Redshift Optimization
• Logarithmic corrected $F(R)$ gravity in the light of Planck 2015
• Gödel-type solutions within the f(R,Q) gravity
• Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes
• Cosmological Constant Problem and Renormalized Vacuum Energy Density in Curved Background
• Effective equation of state in modified gravity and observational constraints
• Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
• Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey
• Tension between SN and BAO: current status and future forecasts
• Consistency Test of Dark Energy Models
• Geometrical Origin of the Cosmological Constant
• A short review of "DGP Specteroscopy"
• Spatial Ricci scalar dark energy model
• Embedding the Texture of the Neutrino Mass Matrix into the MaVaNs Scenario
• Testing Lambda and the Limits of Cosmography with the Union2.1 Supernova Compilation
• New rotating AdS/dS black holes in $\mathrm{f}(\mathrm{R})$ gravity
• A New Type of Dark Energy Model
• Interaction of divergence-free deceleration parameter in Weyl-type $f(Q,T)$ gravity
• A model-independent method with phantom divide line crossing in Weyl-type $f(Q,T)$ gravity
• The Structure and Interpretation of Cosmology: Part I - General Relativistic Cosmology
• Weakly-Gravitating Objects in dynamical Chern-Simons gravity and Constraints with Gravity Probe B
• Observation of Discrete Oscillations in a Model-independent Plot of Cosmological Scale Factor vs. Lookback Time and a Scalar Field Model
• Viability of Variable Generalised Chaplygin gas - a thermodynamical approach
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• Presence of Dark Energy and Dark Matter : Does Cosmic Acceleration signifies a Weak Gravitational collapse?
• Observational Constraints on a Variable Dark Energy Model
• Testing the mutual consistency of different supernovae surveys
• The luminosity-redshift relation in brane-worlds: II. Confrontation with experimental data
• Brane Cosmology with the Chameleon Scalar Field in Bulk
• The simplest parametrization of equation of state parameter in the scalar field Universe
• Crossing the phantom divide with Ricci-like holographic dark energy
• The Abnormally Weighting Energy Hypothesis: the Missing Link between Dark Matter and Dark Energy
• GCG Parametrization for Growth Function and Current Constraints
• Constraints on the DGP Universe Using Observational Hubble parameter
• Phantom Instability of Viscous Dark Energy in Anisotropic Space-Time
• The Spatio-Temporal Evolution of Solar Flares Observed with AIA/SDO: Fractal Diffusion, Sub-Diffusion, or Logistic Growth ?
• Constraints on Quintessence From Using Cosmological Data
• Holographic interacting dark energy in the braneworld cosmology
• Testing $f(R)$ Gravity With Scale Dependent Cosmic Void Velocity Profiles
• Ghosts in asymmetric brane gravity and the decoupled stealth limit
• Linear perturbations in K-mouflage cosmologies with massive neutrinos
• Dark energy and inflation invoked in CCGG by locally contorted space-time
• Perturbations for transient acceleration
• Dark energy, curvature, and cosmic coincidence
• Prospects for Dark Energy Evolution: a Frequentist Multi-Probe Approach
• Observational constraints on modified gravity models and the Poincaré dodecahedral topology
• The Hubble Constant from Type Ia Supernova Calibrated with the Linear and Non-Linear Cepheid Period-Luminosity Relation
• New constraint on the cosmological background of relativistic particles
• Study of parametrized dark energy models with a general non-canonical scalar field
• Cosmological implications of Rastall-$f(R)$ theory
• Gravitational collapse due to dark matter and dark energy in the brane world scenario
• Distance-redshift from an optical metric that includes absorption
• Extragalactic Point Source Search in WMAP 61 and 94 GHz Data
• Constraints on dark energy models from radial baryon acoustic scale measurements
• Perturbations in the relaxation mechanism for a large cosmological constant
• Cosmological constraints on polytropic gas model
• Noether Symmetry Analysis of Anisotropic Universe in Modified Gravity
• Conservative Estimates of the Mass of the Neutrino from Cosmology
• On the Emergence of Accelerating Cosmic Expansion in f(R) Theories of Gravity
• Relic abundance of mass-varying cold dark matter particles
• Periodic cosmic evolution in $f(Q)$ gravity formalism
• QSSC re-examined for the newly discovered SNe Ia
• Raytracing simulations of coupled dark energy models
• The Influence of Evolving Dark Energy on Cosmology
• Observational evidence favors a static universe
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Dark Energy: The Observational Challenge
• Dark matter and dark energy induced by condensates
• Holographic Dark Energy Model and Scalar-Tensor Theories
• Transverse Wave Propagation in Relativistic Two-fluid Plasmas around Schwarzschild-de Sitter Black Hole
• Horndeski gravity without screening in binary pulsars
• Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy
• Cosmological Implications of 5-dimensional Brans-Dicke Theory
• Anisotropic bulk viscous string cosmological models of the Universe under a time-dependent deceleration parameter
• Reconstructing the properties of dark energy from recent observations
• Cosmology from Moduli Dynamics
• Interstellar Silicate Dust in the z=0.89 Absorber Towards PKS 1830-211: Crystalline Silicates at High Redshift?
• What do the cosmological supernova data really tell us?
• A new parametrization of dark energy equation of state leading to double exponential potential
• Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
• Conformal Cosmological Model Parameters with Distant SNe Ia Data: "gold" and "silver"
• Quantum Aspects of Massive Gravity
• Monster Redshift Surveys through Dispersive Slitless Imaging: The Baryon Oscillation Probe
• Exploiting scale dependence in cosmological averaging
• Revisiting the matter power spectra in $f(R)$ gravity
• Self accelerating solutions in a DGP brane with a scalar field trapped on it: the dynamical systems perspective
• An Inverse $f(R)$ Gravitation for Cosmic Speed up, and Dark Energy Equivalent
• Probing Dark Energy Inhomogeneities with Supernovae
• Prospects and pitfalls of gravitational lensing in large supernova surveys
• Weak Gravitational Lensing in Fourth Order Gravity
• Gradient expansion(s) and dark energy
• Constraining Thawing Quintessence
• Deviation from $\Lambda$CDM: Pressure Parametrization
• Modified holographic Ricci dark energy model and statefinder diagnosis in flat universe
• Charge Conjugation Invariance of the Vacuum and the Cosmological Constant Problem
• Answering a Basic Objection to Bang/Crunch Holography
• Marked correlation functions in perturbation theory
• Growth of perturbations in dark energy parametrization scenarios
• Large-scale peculiar motions and cosmic acceleration
• A Two-field Dilaton Model of Dark Energy
• Cosmic Acceleration in Brans-Dicke Cosmology
• QCD modified ghost scalar field dark energy models
• Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
• Probing Dark Energy with Supernovae : a concordant or a convergent model?
• A new class of holographic dark energy models in LRS Bianchi Type-I
• Future state of the Universe
• Inflationary Perturbations in Anisotropic, Shear-Free Universes
• Uncertainty on determining the dark energy equation of state due to the spatial curvature
• Effective Dark Matter Halo catalog in $f(R)$ gravity
• The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries
• The D-material universe
• Structure formation in dark energy cosmologies described by PADE parameterization
• Dark Matter from the Inflaton Field
• The physical foundations for the geometric structure of relativistic theories of gravitation. From General Relativity to Extended Theories of Gravity through Ehlers-Pirani-Schild approach
• Constraints on Dark Energy from the Observed Expansion of our Cosmic Horizon
• Cosmological neutrino mass limit and the dynamics of dark energy
• Possible dark energy imprints in gravitational wave spectrum of mixed neutron-dark-energy stars
• Cosmological Dynamics of Modified Gravity With a Non-minimal Curvature-matter Coupling
• The distance modulus determined from Carmeli's cosmology fits the accelerating universe data of the high-redshift type Ia supernovae without dark matter
• Limitations of Bayesian Evidence Applied to Cosmology
• Dark Matter, Modified Gravity and the Mass of the Neutrino
• $\Lambda$CDM-type cosmological model and observational constraints
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• A cosmological dust model with extended f(chi) gravity
• Optimized supernova constraints on dark energy evolution
• Thermodynamical Behaviour of Inhomogeneous Universe with Varying $\Lambda$ in Presence of Electromagnetic Field
• Constraints on the generalized tachyon field models from latest observational data
• Thawing Versus. Tracker Behaviour: Observational Evidence
• $f(T)$ non-linear massive gravity and the cosmic acceleration
• Equilibrium of large astrophysical structures in the Newton-Hooke spacetime
• Cosmological constrains from X-ray AGN clustering and SNIa data
• Pre-explosive accretion and simmering phases of Type Ia Supernovae
• Lyman alpha absorbers in motion: consequences of gravitational lensing for the cosmological redshift drift experiment
• Properties of white dwarfs in Einstein-$\Lambda$ gravity
• Cosmological aspects of a unified dark energy and dust dark matter model
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Revisiting the screening mechanism in $f(R)$ gravity
• Introduction to neutrino cosmology
• Observational constraints to a phenomenological $f\left(R,\nabla R\right)$-model
• Dependence on supernovae light-curve processing in void models
• Thermodynamical properties of dark energy with the equation of state
• Testing and selection of cosmological models with $(1+z{)}^6$ corrections
• Rest-Frame R-band Lightcurve of a z~1.3 Supernova Obtained with Keck Laser Adaptive Optics
• Is Dark Energy Dynamical? Prospects for an Answer
• Interacting dark energy: generic cosmological evolution for two scalar fields
• Complete cosmic scenario in the Randall-Sundrum braneworld from the dynamical systems perspective
• Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld
• Testing the cosmic conservation of photon number with type Ia supernovae and ages of old objects
• Dynamical-Screening and the Phantom-Like Effects in a DGP-Inspired $F(R,\varphi )$ Model
• Small Cosmological Constant from Running Gravitational Coupling
• Chameleon Field Dynamics During Inflation
• Holographic Dark Energy Like in $f(R)$ Gravity
• New parameterization for unified dark matter and dark energy
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• Axially magnetized Dark Energy cosmological model
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• FLRW accelerating universe with interactive dark energy
• Interacting entropy-corrected holographic Chaplygin gas model
• Fluid-gravity correspondence in the scalar-tensor theory of gravity: (in)equivalence of Einstein and Jordan frames
• Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample
• Precision measurements of large scale structure with future type Ia supernova surveys
• Is Thick Brane Model Consistent with the Recent Observations?
• Empirical evidences in favor of a varying-speed-of-light
• The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey
• Observational tests of a two parameter power-law class modified gravity in Palatini formalism
• Inhomogeneous Bulk Viscous Fluid Universe with Electromagnetic Field and Variable $\Lambda$-Term
• Constraints on Power Law and Exponential models in $f(Q)$ Gravity
• Unconventional cosmology on the (thick) brane
• Cosmological Solutions with Torsion in a Model of de Sitter Gauge Theory of Gravity
• Role Of Generalized Cosmic Chaplygin Gas In Accelerating Universe : A Field Theoretical Prescription
• Scalar perturbations and the possible self-destruction of the phantom menace
• Chebyshev cosmography in the framework of extended symmetric teleparallel theory
• Spectroscopy of twelve Type Ia supernovae at intermediate redshift
• Cosmology with viscous generalized Chaplygin gas in $f(Q)$ gravity
• Holographic dark energy interacting with dark matter in a Closed Universe
• Investigating dark energy by electromagnetic frequency shifts
• Growth of structures and redshift-space distortion data in scale-dependent gravity
• Structure formation in $f(R)$ gravity: A distinguishing probe between the dark energy and modified gravity
• A simplified approach for Chaplygin-type cosmologies
• Singularity-free nonexotic compact star in $f(R,T)$ gravity
• Constraining a double component dark energy model using type Ia supernovae data
• Consequences of f(R)-theories of gravity on gravitational leptogenesis
• SNe Ia as a cosmological probe
• Weighing dark matter haloes with gravitationally lensed supernovae
• Exact Solutions and Accelerating Universe in Modified Brans-Dicke Theories
• Evidence for new physics from clusters ?
• Using machine learning to compress the matter transfer function $T(k)$
• Why do we Still Believe in Newton's Law ? Facts, Myths and Methods in Gravitational Physics
• Noether Symmetries of a Modified Model in Teleparallel Gravity and a New Approach for Exact Solutions
• Dark Energy Nature in Logarithmic $f(R,T)$ Cosmology
• Barrow entropic Quintessence and Dilation dark energy Models with Generalized HDE cut-off
• Cosmological test using strong gravitational lensing systems
• Expanding Universe: slowdown or speedup?
• Tomographic Representation of Minisuperspace Quantum Cosmology and Noether Symmetries
• An FLRW interacting dark energy model of the Universe
• Constraints on Dark Energy Models Using Late Universe Probes
• Topological phantom AdS black holes in $F(R)$ gravity
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• An indirect limit on the amplitude of primordial Gravitational Wave Background from CMB-Galaxy Cross Correlation
• Surveying the dark side
• Measuring the speed of light with updated Hubble diagram of high-redshift standard candles
• Tracing cosmic evolution through Weyl-Type f(Q,T) gravity model: theoretical analysis and observational validation
• A minimal set of invariants as a systematic approach to higher order gravity models
• Dark Energy From Vacuum Fluctuations
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• New Horizons in Gravity: Dark Energy and Condensate Stars
• Neutralino dark matter stars can not exist
• A Direct Upper Limit on the Density of Cosmological Dust from the Absence of an X-ray Scattering Halo around the z=4.3 QSO 1508+5714
• Dust in the Host Galaxies of Supernovae
• Smooth deformations and cosmic statefinders
• Observational Constraints on Undulant Cosmologies
• Quintessential Inflation with Dynamical Higgs Generation as an Affine Gravity
• Dark energy, integrated Sachs-Wolfe effect and large-scale magnetic fields
• Cosmological constraints on unifying Dark Fluid models
• A New Class of Bianchi Type-I Cosmological Models in Scalar-Tensor Theory of Gravitation and Late Time Acceleration
• Acceleration of the Universe driven by the Casimir force
• Observational Evidence for Negative-Energy Dust in Late-Times Cosmology
• Twister quintessence scenario
• Particle Production in f(R) Gravity during Structure Formation
• Quantum driven Bounce of the future Universe
• Galileons, phantom fields, and the fate of the Universe
• Weighing neutrinos in the presence of a running primordial spectral index
• Constraining the CDM spectrum normalization in flat dark energy cosmologies
• Is there a standard measuring rod in the Universe?
• Gravitational time delay of light for various models of modified gravity
• Can Strong Gravitational Lensing Constrain Dark Energy?
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Validity of Generalized Second Law of Thermodynamics in the Logamediate and Intermediate scenarios of the Universe
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Phase transitions and entropy force of charged de Sitter black holes with cloud of string and quintessence
• Power-law solutions and accelerated expansion in scalar-tensor theories
• Constraints on Cubic and $f(P)$ Gravity from the Cosmic Chronometers, BAO & CMB datasets : Use of Machine Learning Algorithms
• Cosmic Acceleration and Anisotropic models with Magnetic field
• The Angular-Diameter-Distance-Maximum and Its Redshift as Constraints on $\Lambda \ne 0$ FLRW Models
• Extending the redshift-distance relation in Cosmological General Relativity to higher redshifts
• The Hubble constant and dark energy from cosmological distance measures
• The Unified Equation of State for Dark Matter and Dark Energy
• Transient acceleration in $f(T)$ gravity
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• Dynamical Dark Energy model parameters with or without massive neutrinos
• Gravitational lens optical scalars in terms of energy-momentum distributions in the cosmological framework
• Holographic dark energy and validity of the generalized second law of thermodynamics in the dgp brane world
• A Study of Black Holes in $F(R)-$ModMax Gravity: Gravitational Lensing and Constraints from EHT Observations
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• Scaling Dark Energy
• FRW dark energy cosmological model with hybrid expansion law
• Cosmologies from higher-order string corrections
• Observational Constraints on the Normal Branch of a Warped DGP Cosmology
• Cosmology With A Dark Refraction Index
• Influence of the cosmic repulsion on the MOND model of the Magellanic Cloud motion in the field of Milky Way
• Tracking Quintessence and Cold Dark Matter Candidates
• Forecast and analysis of the cosmological redshift drift
• Non-commutative Power-law Inflation: Mode Equation and Spectra Index
• On the viability of Planck scale cosmology with quartessence
• Quintom dark energy in DGP braneworld cosmology
• Cosmic Dust Induced Flux Fluctuations: Bad and Good Aspects
• Modified General Relativity and dark matter
• Redshift-distance relations from type Ia supernova observations. New constraints on grey dust models
• Yang-Mills Gravity in Flat Space-time, II. Gravitational Radiations and Lee-Yang Force for Accelerated Cosmic Expansion
• Can brane dark energy model be probed observationally by distant supernovae?
• Symmetric-Bounce Quantum State of the Universe
• $Om$ Diagnostic for Dilaton Dark Energy
• Exploring the Cosmological Model in $f(R,T^{\varphi })$ Gravity with Observational Constraints
• Interacting holographic dark energy models: A general approach
• Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
• Geometrical aspects on the dark matter problem
• A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity in Bianchi-I spacetime
• Probing for variation of neutrino mass with current observations
• Localization of the SFT inspired Nonlocal Linear Models and Exact Solutions
• Non-flat universe and interacting dark energy model
• Falsifying Field-based Dark Energy Models
• Effects of structure formation on the expansion rate of the Universe: An estimate from numerical simulations
• Observational Constraints on the Generalized Chaplygin Gas
• Cosmological Scaling Solutions with Tachyon:Modified Gravity Model
• Constraints on the Phase Plane of the Dark Energy Equation of State
• Braneworld Black Holes
• Like vs. Like: Strategy and Improvements in Supernova Cosmology Systematics
• Asymptotic behavior of Cardassian cosmologies with exponential potentials
• Simplified Quartessence Cosmology
• Universe Bounded By Event Horizon: A Non equilibrium Thermodynamic Prescription
• Spectral Energy Distribution of z>1 Type Ia Supernova Hosts in GOODS: Constraints on Evolutionary Delay and the Initial Mass Function
• Observation constraints on scalar field cosmological model in Anisotropic universe
• Bianchi type-VI anisotropic dark energy model with varying EoS parameter
• The $k$-essence scalar field in the context of Supernova Ia Observations
• Inclusive Constraints on Unified Dark Matter Models from Future Large-Scale Surveys
• Scalar field power-law cosmology with spatial curvature and dark energy-dark matter interaction
• Accelerating model of flat universe in $f(R,T)$ gravity
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Mimicking general relativity in the solar system
• Holographic dark energy in Barrow cosmology with Granda-Oliveros IR cutoff
• Complete density perturbations in the Jordan-Fierz-Brans-Dicke theory
• Entropy and statefinder diagnosis in chameleon cosmology
• First-order perturbations of Gödel-type metrics in non-dynamical Chern-Simons modified gravity
• Observational tests of backreaction with recent data
• Reconstructing the interaction between the dark matter and holographic dark energy
• Cosmological implications of massive gravitons
• Interacting new agegraphic Phantom model of dark energy in non-flat universe
• Fundamental physics from black holes, neutron stars and gamma-ray bursts
• Ellipsoidal configurations in the de Sitter spacetime
• Dynamical quintessence fields Press-Schechter mass function: detectability and effect on dark haloes
• Probing the cosmic acceleration history and the properties of dark energy from the ESSENCE supernova data with a model independent method
• Finite Temperature Casimir Effect for a Massless Fractional Klein-Gordon field with Fractional Neumann Conditions
• Towards observational constraints on negative (1+z)^4 type contribution in the Friedmann equation
• Cosmic Variation of Proton to Electron Mass Ratio with an interacting Higgs Scalar Field
• Weyl Anomaly and Initial Singularity Crossing
• Thermodynamical behaviour of the Variable Chaplygin gas
• Deviation From ΛCDM With Cosmic Strings Networks
• Complementary constraints on non-standard cosmological models from CMB and BBN
• Evolution of Spherical Overdensity in Thawing Dark energy Models
• A Modified Generalized Chaplygin Gas as the Unified Dark Matter-Dark Energy Revisited
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Distinguishing f(R) theories from general relativity by gravitational lensing effect
• Holographic dilatonic model of dark energy
• Cosmological models of generalized ghost pilgrim dark energy (GGPDE) in the gravitation theory of Saez-Ballester
• The CMBR ISW and HI 21-cm Cross-correlation Angular Power Spectrum
• Decaying dark energy in light of the latest cosmological dataset
• Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
• Noether Symmetry Approach in "Cosmic Triad" Vector Field Scenario
• Halting eternal acceleration with an effective negative cosmological constant
• Crossing the Phantom Divide in Extended Dvali-Gabadadze-Porrati Gravity
• Gamma ray burst distances and the timescape cosmology
• Inflection Point Quintessence
• Spatial Periodicity of Galaxy Number Counts, CMB Anisotropy, and SNIa Hubble Diagram Based on the Universe Accompanied by a Non-Minimally Coupled Scalar Field
• Bianchi Type V Viscous Fluid Cosmological Models in Presence of Decaying Vacuum Energy
• Einstein-de Sitter model re-examined for the newly discovered SNe Ia
• Effective dark matter power spectra in $f(R)$ gravity
• On the luminosity distance and the epoch of acceleration
• Dark energy constraint on equation of state parameter in the Weyl type $f(Q,T)$ gravity
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Constraints on the Transition Redshift using Hubble Phase Space Portrait
• Gravitational Origin of Phantom Dark Energy and Late Cosmic Acceleration
• Long Gamma-Ray Burst prompt emission properties as a cosmological tool
• Direct Measurement of the Positive Acceleration of the Universe and Testing Inhomogeneous Models under Gravitational Wave Cosmology
• Smooth crossing of $w_{\Lambda }=-1$ line in a single scalar field model
• Interacting Scalar and Electromagnetic Fields in $f(R,T)$ Theory of Gravity
• Cosmological dynamics of a non-minimally coupled bulk scalar field in DGP setup
• The Universe Dynamics from Topological Considerations
• A model of dark matter dark energy interaction with some cosmic consequences
• Tilt and phantom cosmology
• Observational constraints on the time-dependence of dark energy
• Cosmologies with variable parameters and dynamical cosmon: implications on the cosmic coincidence problem
• On thermodynamic and quantum fluctuations of cosmological constant
• Relaxing a large cosmological constant in the astrophysical domain
• FRW type of cosmology with a Chaplygin gas
• Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
• Resolving Hubble tension with the Milne model
• Renyi Holographic Dark Energy models in Teleparallel gravity
• Combining Optical and X-ray Observations of Galaxy Clusters to Constrain Cosmological Parameters
• Surface Tension of Cosmic Voids as a Possible Source for Dark Energy
• Dynamics of Domain Walls for Split and Runaway Potentials
• Thin accretion disk signatures in hybrid metric-Palatini gravity
• Scaling Dark Energy in a Five-Dimensional Bouncing Cosmological Model
• The current status of observational cosmology
• The $R_{\mathrm{h}}=ct$ universe and quintessence
• First cosmological constraints on the Superfluid Chaplygin gas model
• Alternative High-z Cosmic Tracers and the Dark Energy Equation of State
• Towards Ghost-Free Gravity and Standard Model
• Is it possible to estimate the Higgs Mass from the CMB Power Spectrum?
• Accelerated Expansion of the Universe in the Model with Non-Uniform Pressure
• A solution to the cosmological constant problem
• Constraining Perturbative Early Dark Energy with Current Observations
• N-body simulations, halo mass functions, and halo density profile in $f(T)$ gravity
• Dark Sector from Interacting Canonical and Non-Canonical Scalar Fields
• Quantum Statistical Entropy and Minimal Length of 5D Ricci-flat Black String with Generalized Uncertainty Principle
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Naked Singularity in a Modified Gravity Theory
• The Slow-Roll and Rapid-Roll Conditions in the Space-like Vector Field Scenario
• Testing backreaction effects with observational Hubble parameter data
• Averaging inhomogeneities in scalar-tensor cosmology
• Construction of Multiple Spherical Branes Cosmological Scenario
• Phantom energy accretion and primordial black holes evolution in Brans-Dicke theory
• Modeling Repulsive Gravity with Creation
• Inflaton field governed universe from NKK theory of gravity: stochastic approach
• Angular distribution of cosmological parameters as a probe of inhomogeneities: a kinematic parametrisation
• Phantom fields: bounce solutions in the early Universe and S-branes
• An Inhomogeneous Model Universe Behaving Homogeneously
• Strong lensing, cosmology and lensing halos
• Evidence for Evolution or Bias in Host Extinctions of Type 1a Supernovae at High Redshift
• No "big trips" for the universe
• Conformal symmetry of gravity and the cosmological constant problem
• Why CMB physics?
• Confronting quintessence models with recent high-redshift supernovae data
• Cosmological constraints on dark energy
• Bulk viscous cosmological model with interacting dark fluids
• On the holographic dark energy in chameleon scalar-tensor cosmology
• Stability analysis in Modified Non-Local Gravity
• Fitting cosmological data to the function $q(z)$ from GR Theory: Modified Chaplygin Gas
• Interacting Generalised Cosmic Chaplygin gas in Loop quantum cosmology: A singularity free universe
• Weak gravitational lensing by compact objects in fourth order gravity
• The cosmological constant in the brane world of string theory on $S^1/Z_2$
• Hamiltonian General Relativity in Finite Space and Cosmological Potential Perturbations
• Interacting holographic tachyon model of dark energy
• Principles of Quantum Universe
• Fractal FRW Model within Domain Wall
• A back-reaction approach to dark energy
• Anisotropic massive strings in scalar-tensor theory of gravitation
• Towards a possible solution for the coincidence problem: f(G) gravity as background
• Constraints on Cardassian universe from Gamma ray bursts
• Information geometry in cosmological inference problems
• Stability, dark energy parameterization and swampland aspect of Bianchi Type-$V{I}_h$ cosmological models with f(R, T)-gravity
• Hubble Diagram of Gamma-Rays Bursts calibrated with Gurzadyan-Xue Cosmology
• Selection effects on X-ray and strong-lensing clusters in various cosmologies
• The Fate of the Universe: Dark Energy Dilution?
• Szekeres models: a covariant approach
• Generalized Model for $\Lambda$-Dark Energy
• Scalar Field as Dark Energy Accelerating Expansion of the Universe
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• A primer on problems and prospects of dark energy
• Galaxy-galaxy lensing data: $f(T)$ gravity challenges General Relativity
• Phase transition in Schwarzschild-de Sitter spacetime
• Classification of the FRW universe with a cosmological constant and a perfect fluid of the equation of state $p=w\rho$
• The structure of hybrid neutron star in Einstein-$\Lambda$ gravity
• Non-Minimal Quintessence With Nearly Flat Potential
• Effect of low anisotropy on cosmological models by using supernova data
• Cosmic transparency and acceleration
• Tachyonic (phantom) power-law cosmology
• Weakly trapped surfaces in asymptotically de Sitter spacetimes
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• Scale-Free model for governing universe dynamics
• Phantom-Like Behavior in Modified Teleparallel Gravity
• Machine learning unveils the linear matter power spectrum of modified gravity
• Neutrino Mass Limit from Galaxy Cluster Number Density Evolution
• "The Waters I am Entering No One yet Has Crossed": Alexander Friedman and the Origins of Modern Cosmology
• Interacting warm dark matter
• DGP Cosmological model with generalized Ricci dark energy
• Gravitational Collapse With Dark Energy And Dark Matter In Hořava-Lifshitz Gravity
• Dynamics of Brans-Dicke cosmology with varying mass fermions
• Spherically symmetric and static solutions in $f(R)$ gravity coupled with EM fields
• Search for Global Metric Anisotropy in Type Ia Supernova Data
• Model-Independent Plotting of the Cosmological Scale Factor as a Function of Lookback Time
• Mixed fluid cosmological model in $f(R,T)$ gravity
• Improved parametrization of the growth index for dark energy and DGP models
• Scalar field exact solutions for non-flat FLRW cosmology: A technique from non-linear Schrödinger-type formulation
• Phantom-Like Behavior of a DGP-Inspired Scalar-Gauss-Bonnet Gravity
• Discriminating Electroweak-ino Parameter Ordering at the LHC and Its Impact on LFV Studies
• Challenges in Constraining Gravity with Cosmic Voids
• Study of Some Parameters of Modified Chaplygin Gas in Galileon Gravity Theory from Observational Perspective
• Dark Energy from Wet Dark Fluid
• Accelerated cosmic expansion in a scalar-field universe
• Cancellation of the central singularity of the Schwarzschild solution with natural mass inversion process
• Barrow holographic dark energy models in $f\left(Q\right)$ symmetric teleparallel gravity with Lambert function distribution
• Utilizing the Updated Gamma-Ray Bursts and Type Ia Supernovae to Constrain the Cardassian Expansion Model and Dark Energy
• Observational data fitting to constrain Variable Modified Chaplygin Gas in the background of Horava-Lifshitz Gravity
• Gödel-type solutions within the $f(R,Q,P)$ gravity
• The tension of cosmological magnetic fields as a contribution to dark energy
• The variation of the fine structure constant: testing the dipole model with thermonuclear supernovae
• Fischler-Susskind holographic cosmology revisited
• Phantom-like effects in asymmetric brane embedding with induced gravity and the Gauss-Bonnet term in the Bulk
• Generalised second law of thermodynamics for interacting dark energy in the DGP brane world
• Qualitative analysis and characterization of two cosmologies including scalar fields
• Braneworld Isotropization and Magnetic Fields
• `Pure' Supernovae and Accelerated Expansion of the Universe
• $\Lambda$-CDM type Heckmann - Suchuking model and union 2.1 compilation
• Bootstrapping from inflationary magnetogenesis to CMB initial conditions
• The Gravitational Deflection of Light in F(R)-gravity
• A holographic bound on the total number of computations in the visible Universe
• A new method to determine large scale structure from the luminosity distance
• Observational Constraints of Homogeneous Higher Dimensional Cosmology with Modified Chaplygin Gas
• High-z Supernova Type Ia Data: non-Gaussianity and Direction Dependence
• Interacting parametrized post-Friedmann method
• Cosmological bounds on TeV-scale physics and beyond
• Stability analysis of agegraphic dark energy in Brans-Dicke cosmology
• Scalar - Tensor gravity with scalar -matter direct coupling and its cosmological probe
• Non-adiabatic perturbations in Ricci dark energy model
• Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
• Holographic dark energy in the DGP model
• A new estimator of the deceleration parameter from galaxy rotation curves
• Ricci curvature non-minimal derivative coupling cosmology with field re-scaling
• A Viable Dark Fluid Model
• Modelling Time-varying Dark Energy with Constraints from Latest Observations
• Noncommutative Universe and Chameleon Field Dynamics
• String Cosmology in Anisotropic Bianchi-II Space-time
• Modified general relativity
• A conjecture on the origin of dark energy
• Specific Effect of Peculiar Velocities on Dark-Energy Constraints from Type Ia Supernovae
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• Latest Observational Constraints on Cardassian Models
• Coupled Quintessence scalar field model in light of observational datasets
• Multi-frequency investigation of the parsec- and kilo-parsec-scale radio structures in high-redshift quasar PKS 1402+044
• Reconstructing FHDE with Scalar and Gauge Fields
• Quantifying parameter errors due to the peculiar velocities of type Ia supernovae
• Energy conditions in $f(Q,L_m)$ gravity
• Vacuum properties of nonsymmetric gravity in de Sitter space
• Slow-rotating charged black hole solution in dynamical Chern-Simons modified gravity
• Stability analysis of an interacting holographic dark energy model
• Neutron Stars in f(R)-Gravity and Its Extension with a Scalar Axion Field
• Pupil Masks for Spectrophotometry of Transiting Exoplanets
• Flat Cosmology with Coupled Matter and Dark Energies
• Elliptical Solutions to the Standard Cosmology Model with Realistic Values of Matter Density
• Acceleration of a Spherical Brane-Universe
• A Parameterized Variable Dark Energy Model: Structure Formation and Observational Constraints
• Lyra's Cosmology of Massive String in Anisotropic Bianchi-II Space-time
• Inhomogeneous Cosmology, Inflation and Late-Time Accelerating Universe
• A possible interrelation between the estimated luminosity distances and internal extinctions of type Ia supernovae
• Local dark energy: HST evidence from the expansion flow around Cen A/M83 galaxy group
• Light Propagation in Inhomogeneous Universes. V. Gravitational Lensing of Distant Supernovae
• Cosmology as a search for overall equilibrium
• Two Component Baryonic-Dark Matter Structure Formation in Top-Hat Model
• Constraining Dark Energy From Splitting Angle Statistic of Strong Gravitational Lenses
• Late transient acceleration of the universe in string theory on $S^1/Z_2$
• No-Bang Quantum State of the Cosmos
• Kinematical Conformal Cosmology: fundamental parameters from astrophysical observations
• Constraining Parameters of Generalized Cosmic Chaplygin Gas in Loop Quantum Cosmology
• Dark Energy and Dark Matter From Hidden Symmetry of Gravity Model with a Non-Riemannian Volume Form
• Determination of Cosmological Parameters from Gamma Ray Burst Characteristics and Afterglow Correlations
• Charged black holes in expanding Einstein-de Sitter universes
• Observational constraints on the growth index parameters in $f(Q)$ gravity
• Unveiling the Universe with Emerging Cosmological Probes
• Coincidence Problem in f(T) Gravity Models
• Cosmological observations in non-local $F(R)$ cosmology
• Abundance stratification in type Ia supernovae -- VI: the peculiar slow decliner SN\,1999aa
• There is no vacuum zero-point energy in our universe for massive particles within the scope of relativistic quantum mechanics
• Constraining Parameters for the Accelerating Universe in $f(R,{\mathcal{L}}_m)$ Gravity
• The Transparency of the Universe Limited by Ly-alpha Clouds
• The Cosmology of Asymmetric Brane Modified Gravity
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• Observational Constraints of Modified Chaplygin Gas in RS II Brane
• Higher Curvature Brane Corrections to the DGP Model
• Dark Energy, Dark Matter and Gravity
• Cosmological constrains on fast transition Unified Dark Energy/Matter models
• A numerical approach to model independently reconstruct $f(R)$ functions through cosmographic data
• The Next Generation of Cosmological Measurements with Type Ia Supernovae
• Measuring the cosmological density perturbation
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Cosmological applications of a geometrical interpretation of "c"
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• A Calibration of NICMOS Camera 2 for Low Count-Rates
• Low red-shift formula for the luminosity distance in a LTB model with cosmological constant
• Observational Consequences of Quantum Cosmology
• Do recent supernovae Ia observations tend to rule out all the cosmologies?
• Towards an Observational Appraisal of String Cosmology
• Dark Gravitational Field on Riemannian and Sasaki Spacetime
• Reconstruction of Five-dimensional Bounce cosmological Models From Deceleration Factor
• "Expansion" around the vacuum: how far can we go from Lambda?
• Paczynski-Wiita-like potential for any static spherical black hole in metric theories of gravity
• Hydrogen 2p--2s transition: signals from the epochs of recombination and reionization
• Statefinder analysis of the superfluid Chaplygin gas model
• Indirect Detection of Kaluza-Klein Dark Matter from Latticized Universal Dimensions
• How effective is new variable modified Chaplygin gas to play the role of dark energy- A dynamical system analysis in RS II Brane model
• Interacting Kasner-type cosmologies
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Anisotropic Cosmological Model with Variable G and Lambda
• Local measurement of Λ using pulsar timing arrays
• Can Quantum Gravitational Effects Influence the Entire History of the Universe?
• Crossing of the Cosmological Constant Boundary - an Equation of State Description
• Constraining some $r^{-n}$ extra-potentials in modified gravity models with LAGEOS-type laser-ranged geodetic satellites
• Curvature Singularity in f(R) Theories of Gravity
• UV caps, IR modification of gravity, and recovery of 4D gravity in regularized braneworlds
• Parameterized Deceleration in $f(Q,C)$ Gravity: A Logarithmic Approach
• Large-scale structure and the Cardassian fluid
• Dynamical and gravitational lensing properties of a new phenomenological model of elliptical galaxies
• The Shared Causal Pasts and Futures of Cosmological Events
• Cosmic Acceleration in an Extended Brans-Dicke-Higgs Theory
• Dark energy induced by neutrino mixing
• Cosmological expansion and local systems: a Lemaître-Tolman-Bondi model
• Fitting the luminosity data from type Ia supernovae in the frame of the Cosmic Defect theory
• Impact of the matter density uncertainty on the dark energy reconstruction
• A Possible Late Time $\Lambda$CDM-like Background Cosmology in Relativistic MOND Theory
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Revisiting kink-like parametrization and constraints using OHD/Pantheon+/BAO samples
• A Nearly Model-Independent Characterization of Dark Energy Properties as a Function of Redshift
• Cosmological applications in Kaluza-Klein theory
• Type Ia SNe along redshift: the R(Si II) ratio and the expansion velocities in intermediate z supernovae
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• Type Ia supernovae tests of fractal bubble universe with no cosmic acceleration
• Cosmic Acceleration and Geodesic Deviation in Chameleon Scalar Field Model
• Interacting Three Fluid System and Thermodynamics of the Universe Bounded by the Event Horizon
• Bouncing Universe with a Nonminimally Coupled Scalar Field on a Moving Domain Wall
• Dynamics of entropy perturbations in assisted dark energy with mixed kinetic terms
• Addressing the $r_d$ Tension using Late-Time Observational Measurements in a Novel deceleration Parametrization
• Cosmological implications of non-minimally coupled f(Q) gravity
• Validity of Thermodynamical Laws in Dark Energy Filled Universe
• A study of different horizons in inhomogeneous LTB cosmological model
• Observational constraints on the unified dark matter and dark energy model based on the quark bag model
• Phantom Divide Crossing with General Non-minimal Kinetic Coupling
• Apparent versus true value of the cosmological constant
• Laser interferometer response to scalar massive gravitational waves
• Cosmology from Planck
• Quintessential Inflation, Unified Dark Energy and Dark Matter, and Higgs Mechanism
• Complementary cosmological tests of RSII brane models
• Multipole analysis on gyroscopic precession in $f(R)$ gravity with irreducible Cartesian tensors
• Energy conditions and a bounce in FLRW cosmologies
• Cosmological Parameters and Cosmic Topology
• A Conceptual Tour About the Standard Cosmological Model
• Trapping of Nonlinear Gravitational Waves by Two-Fluid Systems
• Cosmological extrapolation of MOND
• Gödel-type Solutions in Cubic Galileon Gravity
• Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
• The hierarchy problem, radion mass, localization of gravity and 4D effective Newtonian potential in string theory on $S^1/Z_2$
• Genetic algorithms and the analysis of SnIa data
• Luminosity distance for Born-Infeld electromagnetic waves propagating in a cosmological magnetic background
• Quantum fluctuations in the DGP model and the size of the cross-over scale
• Quasar spectral energy distribution in EUV restored from associated absorbers: indications to the HeII opacity of the quasar accretion disk wind
• Bulk scalar field in brane-worlds with induced gravity inspired by the $\mathcal{L}(R)$ term
• Quantum fields near phantom-energy `sudden' singularities
• Constraints on the unified dark energy-dark matter model from latest observational data
• Expressing the equation of state parameter in terms of the three dimensional cosmic shear
• Numerical Solutions of Inflating Higher Dimensional Global Defects
• Cosmic Evolution with Early and Late Acceleration Inspired by Dual Nature of the Ricci Scalar Curvature
• Observational constraints on viscous cosmology in $f(T,L_m)$ gravity
• Cosmic Acceleration in a Model of Fourth Order Gravity
• Considering Late-Time Acceleration in some Cosmological Models
• The coincidence problem in $f(R)$ gravity models
• Viability of Arctan Model of f(R) Gravity for Late-time Cosmology
• Different faces of the phantom
• Running Cosmological Constant and Running Newton Constant in Modified Gravity Theories
• Evolving extrinsic curvature and the cosmological constant problem
• Evolution of proto-galaxy-clusters to their present form: theory and observations
• Cosmological models with interacting components and mass-varying neutrinos
• Constraining hybrid potential scalar field cosmological model in Lyra's geometry with recent observational data
• How Much NEC Breaking Can the Universe Endure?
• Brane cosmology in the Horava-Witten heterotic M-Theory on $S^1/Z_2$
• An introduction to the dark energy problem
• Modification to the Luminosity Distance Redshift Relation in Modified Gravity Theories
• D/antiD Dark Energy in String Warped Compactification
• A comprehensive analysis of the compact phase space for Hu-Sawicki $f(R)$ dark energy models including spatial curvature
• Cosmological consequences of Modified Gravity (MOG)
• Equation of State for Neutralino Star as a Form of Cold Dark Matter
• Towards a covariant model for cosmic self-acceleration
• de Sitter field equations from quadratic curvature gravity: A group theoretical approach
• Stability analysis and observational constraints in scalar tensor theory
• Interacting Viscous Dark Energy in Bianchi Type-III Universe
• Statefinders and observational measurement of superenergy
• Generalized Ghost Pilgrim Dark Energy Fractal Cosmology with Observational Constraint
• Constraining the runaway dilaton and quintessential dark energy
• Scaling attractors for quintessence in flat universe with cosmological term
• Ghost condensate model of flat rotation curves
• The cosmological constant and the coincidence problem in a new cosmological interpretation of the universal constant c
• Constraints on Holographic cosmologies from strong lensing systems
• Hybrid Inflation, Dark Energy And Dark Matter
• Quantum effects and superquintessence in the new age of precision cosmology
• LRS Bianchi I model with perfect fluid equation of state
• A Century of Cosmology
• Dark Energy in an Astrophysical Context
• On the Number of Cosmic Strings
• Observational Study of Higher Dimensional Magnetic Universe in Non-linear Electrodynamics
• Dynamical stability in scalar-tensor cosmology
• The Energy Density of "Wound" Fields in a Toroidal Universe
• Supernovae constraints on dark energy and modified gravity models
• Observational constraints on a Yang-Mills condensate dark energy model
• The Dark Side of the Universe
• Observational Constraints on Phantom Crossing DGP Gravity
• Finite bounded expanding white hole universe without dark matter
• Constructing a Robust Universe with Attraction-Repulsion Coupling and Energy Conservation
• The Friedmann equations in deformed Hořava-Lifshitz gravity and Debye model
• Gödel-type universes in energy-momentum-squared gravity
• Probing Composite Gravity in Colliders
• Cosmological Solutions of Chameleon Scalar Field Model
• Comparison of Supernovae datasets Constraints on Dark Energy
• Constraints on a new alternative model to dark energy
• Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane
• The Quadratic Approximation for Quintessence with Arbitrary Initial Conditions
• Flat Galactic Rotation Curves from Geometry in Weyl Gravity
• Small cosmological constant in seesaw mechanism with breaking down SUSY
• Cosmic Acceleration from Causal Backreaction in a Smoothly Inhomogeneous Universe
• Ether and Relativity
• Nonparametric determination of redshift evolution index of Dark Energy
• Sky surveys and deep fields of ground-based and space telescopes
• The Cosmic Lens All-Sky Survey parent population - I. Sample selection and number counts
• Supernovae observations and cosmic topology
• Reconstruction of a Deceleration Parameter from the Latest Type Ia Supernovae Gold Dataset
• A comprehensive analysis of Barrow holographic Chaplygin gas model reconstruction and its cosmological consequences
• Braneworld Quintessential Inflation and Sum of Exponentials Potentials
• Cosmology: a bird's eye view
• Inflation is the generic feature of phantom field-not the big-rip
• Primordial black hole detection through diffractive microlensing
• On the propagation of gravitational waves in a $\Lambda$CDM universe
• Slow-roll, acceleration, the Big Rip and WKB approximation in NLS-type formulation of scalar field cosmology
• Extragalactic Gamma--Rays: Gamma Ray Bursts and Blazars
• Thick DGP braneworlds
• Holographic entanglement entropy and complexity for the cosmological braneworld model
• Analytical model of compact star in low-mass X-ray binary with de Sitter spacetime
• Supernova observations fit Einstein-deSitter expansion in 4-sphere
• $f(R)$ Gravity and Crossing the Phantom Divide Barrier
• Horizons and singularity in Clifton's spherical solution of f(R) vacuum
• Reaffirmation of Cosmological Oscillations in the Scale Factor from the Pantheon Compilation of 1048 Type Ia Supernovae
• Gamma Ray Bursts: Cosmic Rulers for the High-Redshift Universe?
• Ghost-Free Higher Derivative Quantum Gravity, the Hierarchy and the Cosmological Constant Problems
• Turbulence and turbulent mixing in natural fluids
• Possible black universes in a brane world
• Accelerated expansion of the Universe in the Presence of Dark Matter Pressure
• Diagnostic Approaches for Interacting generalized holographic Ricci Dark Energy Models
• Compactifications of conformal gravity
• Dark Energy and Matter in 4 Dimensions From an Empty Kaluza-Klein Spacetime
• The reconstruction of dark energy with Ridge Regression Approach
• An Exploration of Heterogeneity in Supernova Type Ia Samples
• Extended models of gravity in SNIa cosmological data using genetic algorithms
• Cosmic Microwave Background Polarization
• Geometric Description of Schrödinger Equation in Finsler and Funk Geometry
• Extending cosmology: the metric approach
• The expansion of the universe observed with supernovae
• ACCESS: Enabling an Improved Flux Scale for Astrophysics
• Cosmological nanolensing by dense gas clouds
• Cosmic microwave background limits on spatially homogeneous cosmological models with dark energy
• A theoretically-explained new-variant of Modified-Newtonian-Dynamics (MOND)
• Cosmological constant from gauge fields on extra dimensions
• Quantum Effects on Cosmic Scales as an Alternative to Dark Matter and Dark Energy
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• Is it possible to observationally distinguish adiabatic Quartessence from LambdaCDM?
• Anisotropic cosmology using observational datasets: exploring via machine learning approaches
• Nonlinear evolution of anisotropic matter configurations under higher-order curvature corrections
• The ${\Omega }_{DE}-{\Omega }_M$ Plane in Dark Energy Cosmology
• APSIS - an Artificial Planetary System in Space to probe extra-dimensional gravity and MOND
• The shadow of black holes in $F(R)$-ModMax theory with cosmic strings
• Cosmological scalar fields that mimic the $\Lambda CDM$ cosmological model
• Gravitational Waves Emission in Quadratic Gravity: longitudinal modes, angular momentum emission, and positivity of the radiated power
• Dark matter, dark energy and modern cosmology: the case for a Kuhnian paradigm shift
• Accelerated expansion of a universe containing a self-interacting Bose-Einstein gas
• Scalar-tensor representation to $f(R,T)-$brane with Gauss-Bonnet gravity
• The gravitational field outside a spatially compact stationary source in a generic fourth-order theory of gravity
• Potentials of Coupled Quintessence Based on a Dilaton
• Method of determining cosmological parameter ranges with samples of candles with an intrinsic distribution
• The age of the universe, the Hubble constant, the accelerated expansion and the Hubble effect
• Constraints on the Sum of Neutrino Masses from Cosmology and their impact on world neutrino data
• Rigorous derivation of dark energy and inflation as geometry effects in Covariant Canonical Gauge Gravity
• Loop Quantum Corrections to Statefinder Parameters of Dark Energy
• The Djorgovski-Gurzadyan dark energy integral equation and the Hubble diagram
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• Twinlike models for parametrized dark energy
• Measuring $H_0$ with pulsar timing arrays
• Time dependent dark energy and the thermodynamics of many-body systems
• The Fourth Gravity Test and Quintessence Matter Field
• Non linear equation of state and effective phantom divide in brane models
• Scattering of scalar perturbations with cosmological constant in low-energy and high-energy regimes
• Hubble Expansion as an Einstein Curvature
• Multipole analysis in the radiation field for linearized $f(R)$ gravity with irreducible Cartesian tensors
• Mass Varying Neutrinos in Supernovae
• Can MONDian vector theories explain the cosmic speed up ?
• What is there in the black box of dark energy: variable cosmological parameters or multiple (interacting) components?
• On the cosmological viability of the Hu-Sawicki type modified induced gravity
• Cosmology with type-Ia supernovae
• Cosmic Acceleration and a New Concordance from Causal Backreaction
• Observational constraints in scalar tensor theory with tachyonic potential
• Study of Some Cosmological Parameters for Interacting New Holographic Dark Energy Model in f(T) Gravity
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• Spectrums of Black Hole in de Sitter Spacetime with Highly Damped Quasinormal Modes: High Overtone Case
• The first turbulent combustion
• A Holographic Energy Model
• Cosmologies of Multiple Spherical Brane-universe Model
• Evolution of proto-galaxy-clusters to their present form: theory and observations
• Complex supergravity quintessence models confronted with Sn Ia data
• Investigating the compatibility of exact solutions in Weyl-type $f(Q,T)$ gravity with observational data
• Linear and nonlinear clusterings of Horndeski-inspired dark energy models with fast transition
• Quintessence, Unified Dark Energy and Dark Matter, and Confinement/Deconfinement Mechanism
• Hubble Diagrams in the Jordan and Einstein Frames
• Supersymmetric Cosmological FRW Model and Dark Energy
• Eternally inflating cosmologies from intersecting spacelike branes
• A bound system in the expanding universe with modified holographic Ricci dark energy and dark matter
• Some remarks on the observational constraints on the self-interacting scalar field model for dark energy
• Dark matter: A phenomenological existence proof
• How does Inflation Depend Upon the Nature of Fluids Filling Up the Universe in Brane World Scenario
• Natures of Statefinder Parameters and Om Diagnostic for Cardassian Universe in Horava-Lifshitz Gravity
• From Hubble diagrams to scale factors
• Constraints on the cosmological density parameters and cosmic topology
• Instruments on large optical telescopes -- A case study
• Cosmological Constraints on Radion Evolution in the Universal Extra Dimension Model
• Conjecture on the Avoidance of the Big Crunch
• Approximate $w_{\varphi }\sim {\Omega }_{\varphi }$ Relations in Quintessence Models
• Dark Energy Density in Brane World
• Light propagation around a Kerr-like black hole immersed in an inhomogeneous anisotropic plasma in Rastall gravity: Analytical solutions to the equations of motion
• Cosmology with dark energy decaying through its chemical-potential contribution
• Numerical analysis of cosmological models for accelerating Universe in Poincare gauge theory of gravity
• Dynamics of the universe as a "test 3-brane" in a 5D bulk
• Dynamical Shortcomings in the Generalized SU(2) Proca Theory: Challenges for Cosmic Acceleration
• Cuscuton-like contribution to dark energy evolution
• Cosmological volume acceleration in dust epoch: using scaling solutions and variable cosmological term $\Lambda (t)$ within an anisotropic cosmological model
• Colliders and Cosmology
• Phase transition of black holes in Brans--Dicke Born--Infeld gravity through geometrical thermodynamics
• Reconstructing the weak lensing magnification distribution of Type Ia supernovae
• Causal cosmology with braneworld gravity including Gauss Bonnet coupling
• Red-shift parametrizations of dark energy and observational constraint on their parameters: Galileon gravity as background
• A Cosmological Holographic Reconstruction of f(Q) Theory
• Constraints on scalar-tensor theories from observations
• Construction of f(R) Gravity Models
• Barboza-Alcaniz Equation of State Parametrization : Constraining the Parameters in Different Gravity Theories
• Acceleration and Deceleration in Curvature Induced Phantom Model of the Late and Future Universe, Cosmic Collapse as Well as its Quantum Escape
• Interacting Models of Generalised Chaplygin Gas and Modified Chaplygin Gas with Barotropic Fluid
• Back to the basis - observations support spherically closed dynamic space
• Hypergeometric viable models in $f(R)$ gravity
• An inhomogeneous universe with thick shells and without cosmological constant
• On the total energy conservation of the Alcubierre spacetime
• Cosmological constraints on a dark energy model with a non-linear scalar field
• Cosmic acceleration via space-time-matter theory
• New Constraints on Dark Energy
• Cosmic Acceleration Data and Bulk-Brane Energy Exchange
• Boundary terms and Brown-York quasi-local parameters for scalar-tensor theory: a study on both timelike and null hypersurfaces
• Dark Energy and Life's Ultimate Future
• Do data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Supernovae Light Curves: An Argument for a New Distance Modulus
• Singularities in and Stability of Ooguri-Vafa-Verlinde Cosmologies
• Kinematical models of latetime cosmology and the statefinder diagnostic
• Ice emission and the redshifts of submillimeter sources
• Semi-holographic model revisited
• Dynamics of General Barotropic Stellar Fluid in the Framework of $R+2\alpha T$ Gravity
• Constraining bouncing cosmology caused by Casimir effect
• An Alternative Approach to the Exact Solution of FRW-Type Spacetime with a Generalized Chaplygin Gas
• Eternally oscillating zero energy Universe
• Mixed gauge-gravity term and proper time
• Enhancement of Dark Matter Abundance in Scalar-Tensor Dark Energy
• Perturbations of Einstein--Maxwell--phantom spacetime: Instabilities of charged Ellis--Bronnikov wormholes and quasinormal modes of black holes
• String Cosmology in LRS Bianchi Type-II Dusty Universe with Time Decaying Vacuum Energy Density $\Lambda$
• A new inflationary Universe scenario with inhomogeneous quantum vacuum
• Particle mixing as possible explanation of the dark energy conundrum
• Inflation and Cosmological Constant
• Can hyperbolic phase of Brans-Dicke field account for Dark Matter?
• From Quantum Information to Gravitation (in German)
• A novel mechanism for the distance-redshift relation
• Features of deSitter Vacua in M-Theory
• Microlensing in phase space II: Correlations analysis
• Evolution of the horizons for dark energy universe
• MAUVE: An Ultraviolet Astrophysics Probe Mission Concept
• Gravitational waves driven by Holographic dark energy
• Electromagnetic Waves in Cosmological Space-Time II. Luminosity Distance
• Thermal Gravitational Radiation and Condensed Universe
• Long-wavelength gravitational waves and cosmic acceleration
• Optimal Extraction of Cosmological Information from Supernova Data in the Presence of Calibration Uncertainties
• Cosmology via Metric-Independent Volume-Form Dynamics
• Geometric and thermodynamic properties in Gauss-Bonnet gravity
• Angular Power Spectrum in Modular Invariant Inflation Model
• Cosmological bootstrap
• Fomin's conception of quantum cosmogenesis
• Expanding Universe: Thermodynamical Aspects From Different Models
• Cosmological General Relativity With Scale Factor and Dark Energy
• When can we compute analytically lookback time, age of the universe, and luminosity distance?
• Precision cosmological measurements: independent evidence for dark energy
• K-Inflation with a Dark Energy Coupling
• A new approach to modified-gravity models
• Perspectives for studying the dark energy at z>2 with galaxy surveys
• Unified Model for Inflation and Dark Matter
• Post-Newtonian Gravitational Waves with cosmological constant $\Lambda$ from the Einstein-Hilbert theory
• Testing modified (Horndeski) gravity by combining intrinsic galaxyalignments with cosmic shear
• Topological Expansion, Study and Applications
• Cosmological constraints from supernova data set with corrected redshift
• Electrovac Universes with a Cosmological Constant
• Addressing type Ia supernova color variability with a linear spectral template
• Observational Evidences of the Cosmological Deceleration of Time
• Dust content of core-collapse supernova hosts
• Some cylindrically symmetric vacuum solutions of Brans-Dicke scalar fields in Robertson-Walker universe
• Determining the expansion history of the universe with the three dimensional cosmic shear
• Supermassive black holes surrounded by dark matter modeled as anisotropic fluid: epicyclic oscillations and their fitting to observed QPOs
• Quintessence in Multi-Measure Generalized Gravity Stabilized by Gauss-Bonnet/Inflaton Coupling
• PISCOLA: a data-driven transient light-curve fitter
• The Compactification Problems of Additional Dimensions in Multidimensional Cosmological Theories
• Windowing Artifacts Likely Account for Recent Claimed Detection of Oscillating Cosmic Scale Factor
• Energy conditions and entropy density of the universe
• The Fate of the Accelerating Universe
• Investigating the Period-Luminosity Relations of delta Scuti Stars: A Pathway to Distance and 3-D Dust Map Inference
• An Inertial Reaction to Cosmological Accelerations
• ELT Observations of Supernovae at the Edge of the Universe
• Propagation of gravitational waves in a universe with slowly-changing equation of state
• Quantum Quintom Cosmology
• A self-consistent solution in affine space with scalar field
• Seeable universe and its accelerated expansion: an observational test
• Electromagnetic Origin for Planck Mass and Dark Energy
• Notes on the compatibility of type Ia supernovae data and varying--$G$ cosmology
• On curvature coupling and quintessence fine-tuning
• Studies of the Inhomogeneous Cosmology in Higher Dimensional space-time with a Cosmological Constant
• The Limits of Quintessence
• Cosmological solutions of Tensor-Vector theories of gravity with varying the space-time-matter coupling constant
• Some Consequences of Dark Energy Density varying Exponentially with Scale Factor
• Unstable Axion Quintessence Revisited
• Effect of the cosmological parameters on gravitational waves: general analysis
• A Study on Ricci Dark Energy in Bulk-Brane Interaction
• Quintessence reconstruction of interacting HDE in a non-flat universe
• Cosmic coincidences and relic neutrinos
• Testing the effects from dark radiation
• Non Thermal Features in the Cosmic Neutrino Background
• Supersymmetric Barotropic FRW Model and Dark Energy
• Bayesian evidence and model selection approach for time-dependent dark energy
• Accelerating electrically charged ModMax black hole solutions in $F(R)$ gravity
• Thermodynamics and optical aspects of ModMax black holes in higher order curvature gravity with quintessence dark energy
• Temperature Fluctuation and an Expected Limit of Hubble Parameter in the Self-Consistent Model
• Space-Time Entropy, Space of Singularities and Gravity Origin: A Case Study
• Using the large scale quasar clustering to constrain flat quintessential universes
• Dark Energy: relating the evolution of the universe from the past to the future
• The Schwarzschild Static Cosmological Model
• Cosmic Expansion via Axion-Induced Quintessence
• $\Lambda$CDM, $\Lambda$DGP and extended phantom-like cosmologies
• Primordial gravitational waves: Model effects on time evolution and spectrum
• Dark Energy Induced Anisotropy in Cosmic Expansion
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• Gauss-Bonnet Gravity and Spacetime Singularities
• The evolution of relative frequencies of ONe and CO SNe Ia
• The European Southern Observatory and VLT Telescopes on Paranal
• Pathology of the Unified Dark Sectors in Modified General Relativity
• Holographic dark energy in modified Kaniadakis cosmology
• Reconstructing the Equation of State for Dark Energy In the Double Complex Symmetric Gravitational Theory
• Dark energy and the future fate of the Universe
• On Gauge Choice of Spherically Symmetric 3-Branes
• GUP-corrected $\Lambda$CDM cosmology
• On Generalized Theories of Varying Fine Structure Constant