Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

Abstract

We present the large-scale correlation function measured from a spectroscopic sample of 46,748 luminous red galaxies from the Sloan Digital Sky Survey. The survey region covers 0.72 h^{-3} Gpc^3 over 3816 square degrees and 0.16<z<0.47, making it the best sample yet for the study of large-scale structure. We find a well-detected peak in the correlation function at 100h^{-1} Mpc separation that is an excellent match to the predicted shape and location of the imprint of the recombination-epoch acoustic oscillations on the low-redshift clustering of matter. This detection demonstrates the linear growth of structure by gravitational instability between z=1000 and the present and confirms a firm prediction of the standard cosmological theory. The acoustic peak provides a standard ruler by which we can measure the ratio of the distances to z=0.35 and z=1089 to 4% fractional accuracy and the absolute distance to z=0.35 to 5% accuracy. From the overall shape of the correlation function, we measure the matter density Omega_mh^2 to 8% and find agreement with the value from cosmic microwave background (CMB) anisotropies. Independent of the constraints provided by the CMB acoustic scale, we find Omega_m = 0.273 +- 0.025 + 0.123 (1+w_0) + 0.137 Omega_K. Including the CMB acoustic scale, we find that the spatial curvature is Omega_K=-0.010+-0.009 if the dark energy is a cosmological constant. More generally, our results provide a measurement of cosmological distance, and hence an argument for dark energy, based on a geometric method with the same simple physics as the microwave background anisotropies. The standard cosmological model convincingly passes these new and robust tests of its fundamental properties.

Submitted to the ApJ. Additional pedagogical material and numerical data at http://cmb.as.arizona.edu/~eisenste/acousticpeak

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• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges
• Reconstruction of the deceleration parameter and the equation of state of dark energy
• Hubble expansion & Structure Formation in Time Varying Vacuum Models
• Corrfunc --- A Suite of Blazing Fast Correlation Functions on the CPU
• Cosmological constraints on f(R) gravity theories within the Palatini approach
• A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey
• Dark Matter: A Primer
• Quantum Tests of the Einstein Equivalence Principle with the STE-QUEST Space Mission
• Flowing with Time: a New Approach to Nonlinear Cosmological Perturbations
• Baryonic acoustic oscillations in simulated galaxy redshift surveys
• Be it therefore resolved: Cosmological Simulations of Dwarf Galaxies with Extreme Resolution
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Optical and Near-Infrared Observations of the Highly Reddened, Rapidly Expanding Type Ia Supernova 2006X in M100
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function
• Cosmological models with linearly varying deceleration parameter
• Testing Gravity Against Early Time Integrated Sachs-Wolfe Effect
• The role of energy conditions in $f(R)$ cosmology
• Galaxy Interactions Trigger Rapid Black Hole Growth: an unprecedented view from the Hyper Suprime-Cam Survey
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space
• Reconstructing holographic quintessence
• Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
• Large-Scale Anisotropic Correlation Function of SDSS Luminous Red Galaxies
• General Relativity and Cosmology: Unsolved Questions and Future Directions
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogs for Cosmological Analysis
• The Clustering of DESI-like Luminous Red Galaxies Using Photometric Redshifts
• Revisiting a negative cosmological constant from low-redshift data
• Cosmological Constraints on New Agegraphic Dark Energy
• On the LCDM Universe in f(R) gravity
• Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1
• Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects
• The BOSS Emission-Line Lens Survey (BELLS). I. A large spectroscopically selected sample of Lens Galaxies at redshift ~ 0.5
• Revisiting Bimaximal Neutrino Mixing in a Model with S4 Discrete Symmetry
• Rastall Cosmology and the ΛCDM Model
• Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
• Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
• LRS Bianchi Type I Models with Anisotropic Dark Energy and Constant Deceleration Parameter
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
• A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements and the strong power of normalized growth rate on constraining dark energy
• Resumming Cosmic Perturbations
• Cosmic Flows on 100 Mpc/h Scales: Standardized Minimum Variance Bulk Flow, Shear and Octupole Moments
• The detectability of baryonic acoustic oscillations in future galaxy surveys
• Possibility of Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization
• Conformal symmetry and accelerating cosmology in teleparallel gravity
• Simulation of the Cosmic Evolution of Atomic and Molecular Hydrogen in Galaxies
• Cosmology in generalized Proca theories
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• First Measurement of the Clustering Evolution of Photometrically-Classified Quasars
• Observational constraints on an interacting dark energy model
• Lemaitre-Tolman-Bondi model and accelerating expansion
• Time drift of cosmological redshifts as a test of the Copernican principle
• Observables sensitive to absolute neutrino masses. II
• On the Growth of Perturbations as a Test of Dark Energy
• Target Selection and Validation of DESI Emission Line Galaxies
• Cosmological Parameters from the 2003 flight of BOOMERANG
• From Cosmology to Cold Atoms: Observation of Sakharov Oscillations in Quenched Atomic Superfluids
• Intrinsic Ellipticity Correlation of SDSS Luminous Red Galaxies and Misalignment with their Host Dark Matter Halos
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12
• Running Hubble Tension and a H0 Diagnostic
• Thermodynamics of cosmological horizons in $f(T)$ gravity
• Generalized Galileon cosmology
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples
• Cosmological solutions from Induced Matter Model applied to 5D f(R,T) gravity and the shrinking of the extra coordinate
• Accelerated expansion from structure formation
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Combining cluster observables and stacked weak lensing to probe dark energy: Self-calibration of systematic uncertainties
• f(R) gravity theories in Palatini formalism: cosmological dynamics and observational constraints
• Dynamical Dark Energy or Simply Cosmic Curvature?
• Update on Coupled Dark Energy and the $H_0$ tension
• The acceleration of the universe and the physics behind it
• A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
• Constraining Interactions in Cosmology's Dark Sector
• The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts
• The effect of inhomogeneous expansion on the supernova observations
• Observational constraints on self-accelerating cosmology
• New constraints on dark energy from the observed growth of the most X-ray luminous galaxy clusters
• Cosmological baryonic and matter densities from 600,000 SDSS Luminous Red Galaxies with photometric redshifts
• Measuring Baryon Acoustic Oscillations along the line of sight with photometric redshifs: the PAU survey
• Inflation and WMAP three year data: Features have a Future!
• Cosmology with hybrid expansion law: scalar field reconstruction of cosmic history and observational constraints
• Very Small-Scale Clustering and Merger Rate of Luminous Red Galaxies
• Pointer states for primordial fluctuations in inflationary cosmology
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
• The EAGLE simulations: atomic hydrogen associated with galaxies
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations at redshift of 0.72 with the DR14 Luminous Red Galaxy Sample
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• Observational Constraints on Teleparallel Dark Energy
• Gravitational collapse in f(R) theories
• Gamma Ray Bursts as standard candles to constrain the cosmological parameters
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Probing interaction and spatial curvature in the holographic dark energy model
• Baryonic Acoustic Oscillations in 21cm Emission: A Probe of Dark Energy out to High Redshifts
• `Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function
• High Performance P3M N-body code: CUBEP3M
• Structure formation in the presence of dark energy perturbations
• Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications
• Using Quantitative Spectroscopic Analysis to Determine the Properties and Distances of Type II-Plateau Supernovae: SNe 2005cs and 2006bp
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering
• Acoustic oscillations in the SDSS DR4 Luminous Red Galaxy sample power spectrum
• Measuring the matter density using baryon oscillations in the SDSS
• Non-linear structure formation and the acoustic scale
• Energy Conditions Constraints and Stability of Power Law Solutions in f(R,T) Gravity
• Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range $0.8<z<2.2$
• Challenges to the DGP Model from Horizon-Scale Growth and Geometry
• Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
• Radiative Transfer Modeling of Lyman Alpha Emitters. I. Statistics of Spectra and Luminosity
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample
• Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-Gaussianity
• Concerns regarding the use of black hole shadows as standard rulers
• The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints
• Observational Constraints on Cosmological Models with the Updated Long Gamma-Ray Bursts
• New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?
• Modified Gravity N-body Code Comparison Project
• CLASH-VLT: A Highly Precise Strong Lensing Model of the Galaxy Cluster RXC J2248.7-4431 (Abell S1063) and Prospects for Cosmography
• Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
• Self-Consistent Cosmological Simulations of DGP Braneworld Gravity
• Exploring Cosmic Origins with CORE: Inflation
• On measuring the covariance matrix of the nonlinear power spectrum from simulations
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogues and Measurement of the isotropic BAO between redshift 0.6 and 1.1 for the Emission Line Galaxy Sample
• The BOSS Emission-Line Lens Survey. II. Investigating Mass-Density Profile Evolution in the SLACS+BELLS Strong Gravitational Lens Sample
• Infrared Resummation for Biased Tracers in Redshift Space
• Mapping the Cosmological Expansion
• One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
• Observational constraints on Galileon cosmology
• Galaxy Merger Statistics and Inferred Bulge-to-Disk Ratios in Cosmological SPH Simulations
• On the evolution of density perturbations in f(R) theories of gravity
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Verifying the Cosmological Utility of Type Ia Supernovae: Implications of a Dispersion in the Ultraviolet Spectra
• An Electron Fixed Target Experiment to Search for a New Vector Boson A' Decaying to e+e-
• No further gravitational wave modes in $F(T)$ gravity
• Accelerated cosmos in a non-extensive setup
• Modeling scale-dependent bias on the baryonic acoustic scale with the statistics of peaks of Gaussian random fields
• Science with a lunar low-frequency array: from the dark ages of the Universe to nearby exoplanets
• Cosmographic analysis with Chebyshev polynomials
• Two Windows on Acceleration and Gravitation: Dark Energy or New Gravity?
• Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
• The effect of peculiar velocities on supernova cosmology
• Cosmological parameters from large scale structure - geometric versus shape information
• The COpernicus COmplexio: Statistical Properties of Warm Dark Matter Haloes
• Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces
• A Search for Warm/Hot Gas Filaments Between Pairs of SDSS Luminous Red Galaxies
• SHARDS: an optical spectro-photometric survey of distant galaxies
• A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - II: Fitting Techniques
• Modelling clusters of galaxies by f(R)-gravity
• Beyond generalized Proca theories
• Constraints on cosmological models from strong gravitational lensing systems
• Large-Scale Tests of the DGP Model
• Using the Noether symmetry approach to probe the nature of dark energy
• Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
• Statefinder diagnosis in a non-flat universe and the holographic model of dark energy
• A first application of the Alcock-Paczynski test to stacked cosmic voids
• Energy conditions bounds on f(T) gravity
• The dark degeneracy: On the number and nature of dark components
• Lunar laser ranging: the millimeter challenge
• A cosmic vector for dark energy
• Cosmic acceleration with bulk viscosity in modified $f(Q)$ gravity
• Combining perturbation theories with halo models
• Cosmological bounds on dark matter-neutrino interactions
• The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture
• An improved model-independent assessment of the late-time cosmic expansion
• The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789
• Clustering of luminous red galaxies I: large scale redshift space distortions
• Charged Black Holes in Phantom Cosmology
• High-precision predictions for the acoustic scale in the non-linear regime
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Testing the interaction between dark energy and dark matter via latest observations
• Detection of Baryon Acoustic Oscillation Features in the Large-Scale 3-Point Correlation Function of SDSS BOSS DR12 CMASS Galaxies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample
• Measurements of H(z) and D_A(z) from the Two-Dimensional Two-Point Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Constraints on modified Chaplygin gas from recent observations and a comparison of its status with other models
• How to suppress the shot noise in galaxy surveys
• New Constraints on Oscillations in the Primordial Spectrum of Inflationary Perturbations
• Cuscuton Cosmology: Dark Energy meets Modified Gravity
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• Power of Observational Hubble Parameter Data: a Figure of Merit Exploration
• The neutrino mass bound from WMAP-3, the baryon acoustic peak, the SNLS supernovae and the Lyman-alpha forest
• Light propagation in statistically homogeneous and isotropic dust universes
• First-year Sloan Digital Sky Survey-II (SDSS-II) supernova results: consistency and constraints with other intermediate-redshift datasets
• The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators
• Null test of the cosmic curvature using $H(z)$ and supernovae data
• Bouncing Loop Quantum Cosmology from $F(T)$ gravity
• Average observational quantities in the timescape cosmology
• Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of N-body Simulations and Analytic Models
• Cosmological information in the redshift-space bispectrum
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation
• Observational constraints on the dark energy and dark matter mutual coupling
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: galaxy clustering measurements in the low redshift sample of Data Release 11
• Density perturbations in general modified gravitational theories
• New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
• Connection between Newtonian simulations and general relativity
• Density perturbations in f(R) gravity theories in metric and Palatini formalisms
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Cosmological Constraints on $f(G)$ Dark Energy Models
• The Carnegie Supernova Project: First Near-Infrared Hubble Diagram to z~0.7
• Simulations of Baryon Acoustic Oscillations II: Covariance matrix of the matter power spectrum
• Gamma-ray Burst Cosmology
• Clustering Fossils from the Early Universe
• A New Method to Correct for Fiber Collisions in Galaxy Two-Point Statistics
• Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles
• Observational constraint on interacting Tsallis holographic dark energy in logarithmic Brans-Dicke theory
• Observational Constraints on Quintessence: Thawing, Tracker, and Scaling models
• Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
• Cosmic Calibration: Constraints from the Matter Power Spectrum and the Cosmic Microwave Background
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Constraining Anisotropic Baryon Oscillations
• Acoustic scale from the angular power spectra of SDSS-III DR8 photometric luminous galaxies
• Quintessential interpretation of the evolving dark energy in light of DESI
• Weak-Field Spherically Symmetric Solutions in $f(T)$ gravity
• Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
• Cosmic Rulers
• Clustering of obscured and unobscured quasars in the Bootes field: Placing rapidly growing black holes in the cosmic web
• Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies
• Dark goo: Bulk viscosity as an alternative to dark energy
• Cosmology with Void-Galaxy Correlations
• Differentiating dark energy and modified gravity with galaxy redshift surveys
• Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results
• An updated Gamma Ray Bursts Hubble diagram
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• Constraining Isocurvature Initial Conditions with WMAP 3-year data
• Ghost conditions for Gauss-Bonnet cosmologies
• The SDSS-IV extended Baryonic Oscillation Spectroscopic Survey: Luminous Red Galaxy Target Selection
• A ground-based 21cm Baryon acoustic oscillation survey
• Supernova cosmology: legacy and future
• Probing for dynamics of dark energy and curvature of universe with latest cosmological observations
• Model Independent Reconstruction of the Expansion History of the Universe and the Properties of Dark Energy
• Observational constraints on the linear fluctuation growth rate
• $f(T)$ cosmology via Noether symmetry
• Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Luminosity and stellar mass dependence of galaxy clustering at 0.5<z<1.1
• Phenomenological Consequences of See-Saw in S4 Based Models
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• Generalizing the running vacuum energy model and comparing with the entropic-force models
• Anisotropic strange star with Tolman-Kuchowicz metric under $f(R,T)$ gravity
• The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
• Modelling the number density of Halpha emitters for future spectroscopic near-IR space missions
• Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835
• Observational constraints on holographic dark energy with varying gravitational constant
• Likelihood-Free Cosmological Inference with Type Ia Supernovae: Approximate Bayesian Computation for a Complete Treatment of Uncertainty
• Subaru Weak Lensing Measurements of Four Strong Lensing Clusters: Are Lensing Clusters Over-Concentrated?
• Hubble expansion and structure formation in the "running FLRW model" of the cosmic evolution
• Constraint on Coupled Dark Energy Models from Observations
• Reheating via a generalized non-minimal coupling of curvature to matter
• Constraints on Dark Energy from Supernovae, Gamma Ray Bursts, Acoustic Oscillations, Nucleosynthesis and Large Scale Structure and the Hubble constant
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: the low redshift sample
• Constraining f(R) gravity in the Palatini formalism
• Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation
• Precision cosmology defeats void models for acceleration
• An analytic model for interacting dark energy and its observational constraints
• The Extended Baryon Oscillation Spectroscopic Survey: Variability Selection and Quasar Luminosity Function
• SDSS Galaxy Clustering: Luminosity & Colour Dependence and Stochasticity
• Constraints on Gauss-Bonnet Gravity in Dark Energy Cosmologies
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological constraints from the full shape of the clustering wedges
• Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
• Testing modified gravity with Planck: the case of coupled dark energy
• Nonlinear Structure Formation and "Apparent" Acceleration: an Investigation
• Calibrating the cosmic distance scale ladder: the role of the sound horizon scale and the local expansion rate as distance anchors
• Confronting Braneworld Cosmology with Supernova data and Baryon Oscillations
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Using the CMB angular power spectrum to study Dark Matter-photon interactions
• The dark degeneracy and interacting cosmic components
• Growth factor parametrization and modified gravity
• A new interacting two fluid model and its consequences
• The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
• Viscous dark fluid universe
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• The significance of the integrated Sachs-Wolfe effect revisited
• Signature of the interaction between dark energy and dark matter in observations
• Cosmology in $f(R,L_m)$ gravity
• Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of ${\sigma }_8$
• Cosmic Chronometers in the R_h=ct Universe
• The Sloan Lens ACS Survey. XII. Extending Strong Lensing to Lower Masses
• Luminosity Function from dedicated SDSS-III and MMT data of quasars in 0.7<z<4.0 selected with a new approach
• Predicted and observed evolution in the mean properties of Type Ia supernovae with redshift
• Features of holographic dark energy under the combined cosmological constraints
• Cosmological simulation with dust formation and destruction
• Cosmic Emulation: Fast Predictions for the Galaxy Power Spectrum
• 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
• Cosmography and flat $\Lambda$CDM tensions at high redshift
• On holographic dark-energy models
• The Hubble Constant
• On the large-scale instability in interacting dark energy and dark matter fluids
• Archipelagian Cosmology: Dynamics and Observables in a Universe with Discretized Matter Content
• Primordial Neutrinos
• Observational constraints on phantom-like braneworld cosmologies
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• Assessment of the Information Content of the Power Spectrum and Bispectrum
• Relic gravitational waves and their detection
• Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test
• The Beginning and Evolution of the Universe
• Present and future evidence for evolving dark energy
• Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
• Baryon acoustic signature in the clustering of density maxima
• Some Anisotropic Dark Energy Models in Bianchi Type-V Space-time
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• Revealing the galaxy-halo connection in IllustrisTNG
• Dark matter and dark energy as a effects of Modified Gravity
• SN 2006bt: A Perplexing, Troublesome, and Possibly Misleading Type Ia Supernova
• Tachyon dark energy models: dynamics and constraints
• Dark energy models from a parametrization of $H$: A comprehensive analysis and observational constraints
• Cosmological parameter analyses using transversal BAO data
• The Physics and Early History of the Intergalactic Medium
• Constraining f(T) teleparallel gravity by Big Bang Nucleosynthesis
• Some Bianchi Type-V Models of Accelerating Universe with Dark Energy
• Some remarks on the dynamical systems approach to fourth order gravity
• Effects of dark sectors' mutual interaction on the growth of structures
• An optimal FFT-based anisotropic power spectrum estimator
• Friedmann Robertson-Walker model in generalised metric space-time with weak anisotropy
• Introducing the Dirac-Milne universe
• Exploring the Properties of Dark Energy Using Type Ia Supernovae and Other Datasets
• Relativistic Krori-Barua Compact Stars in $f(R,T)$ Gravity
• Solar System tests in $f(T)$ gravity
• Accelerating f(T) gravity models constrained by recent cosmological data
• Observational signatures of Jordan-Brans-Dicke theories of gravity
• Observational bounds on the cosmic radiation density
• The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with 3-point correlation functions
• The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey
• Cosmology from quantum potential
• Examining the cosmic acceleration with the latest Union2 supernova data
• Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields
• $e^{\pm }$ Excesses in the Cosmic Ray Spectrum and Possible Interpretations
• Improved constraints on cosmological parameters from SNIa data
• A Field Theory Model for Dark Matter and Dark Energy in Interaction
• Measuring neutrino masses and dark energy with weak lensing tomography
• Quantifying the $S_8$ tension with the Redshift Space Distortion data set
• Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
• Future singularities and Teleparallelism in Loop Quantum Cosmology
• Observational constraints on the acceleration of the Universe
• Improving measurements of H(z) and Da(z) by analyzing clustering anisotropies
• Radio galaxies in the 2SLAQ Luminous Red Galaxy Survey: I. The evolution of low-power radio galaxies to z~0.7
• Measuring dark energy with the $E_{\mathrm{iso}}-E_{\mathrm{p}}$ correlation of gamma-ray bursts using model-independent methods
• Variability selected high-redshift quasars on SDSS Stripe 82
• Interacting Ghost Dark Energy in Non-Flat Universe
• Dynamics of interacting dark energy model in Einstein and Loop Quantum Cosmology
• Cosmological consequences of an adiabatic matter creation process
• Signals From the Epoch of Cosmological Recombination
• General analytic formulae for attractor solutions of scalar-field dark energy models and their multi-field generalizations
• Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
• Comparison of dark energy models: A perspective from the latest observational data
• The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from the Third Data Release Quasar Lens Catalog
• Thermodynamical properties of the Universe with dark energy
• Multiple inflation and the WMAP 'glitches' II. Data analysis and cosmological parameter extraction
• First test of Verlinde's theory of Emergent Gravity using Weak Gravitational Lensing measurements
• Measuring cosmological parameters with Gamma-Ray Bursts
• Cosmological Constraints on the Sign-Changeable Interactions
• Current constraints on interacting holographic dark energy
• Cosmic history of viable exponential gravity: Equation of state oscillations and growth index from inflation to dark energy era
• Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
• A Cross-Correlation Analysis of Mg II Absorption Line Systems and Luminous Red Galaxies from the SDSS DR5
• Halo-model signatures from 380,000 SDSS Luminous Red Galaxies with photometric redshifts
• Cosmological dynamics of tachyonic teleparallel dark energy
• Modeling the angular correlation function and its full covariance in Photometric Galaxy Surveys
• The New Horizon Run Cosmological N-Body Simulations
• Constraints on dark energy with the LOSS SN Ia sample
• Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae
• Constraining the LRG Halo Occupation Distribution using Counts-in-Cylinders
• Can f(R) Modified Gravity Theories Mimic a LCDM Cosmology?
• Cosmological Applications of Pade Approximant
• Strange stars in Krori-Barua space-time under f(R; T) gravity
• Anisotropic Universe Models with Perfect Fluid and Scalar Field in f(R,T) Gravity
• On the co-existence of matter dominated and accelerating solutions in f(G)-gravity
• If Gauss-Bonnet interaction plays the role of dark energy
• Thermal history of the plasma and high-frequency gravitons
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: I. Real Space
• The stability of the Einstein static state in $f(T)$ gravity
• Friedmann cosmology with bulk viscosity: a concrete model for dark energy
• Fitting Methods for Baryon Acoustic Oscillations in the Lyman-α Forest Fluctuations in BOSS Data Release 9
• The Three-Point Correlation Function of Luminous Red Galaxies in the Sloan Digital Sky Survey
• Investigating dark energy experiments with principal components
• Photon-axion mixing and ultra-high-energy cosmic rays from BL Lac type objects -- Shining light through the Universe
• Tracing The Sound Horizon Scale With Photometric Redshift Surveys
• The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: final Emission Line Galaxy Target Selection
• Cosmology and Convention
• The Art of Lattice and Gravity Waves from Preheating
• $Om$ diagnostic applied to scalar field models and slowing down of cosmic acceleration
• Hubble parameter measurement constraints on dark energy
• Testing Models of Intrinsic Brightness Variations in Type Ia Supernovae, and their Impact on Measuring Cosmological Parameters
• Effective $F(T)$ gravity from the higher-dimensional Kaluza-Klein and Randall-Sundrum theories
• Angular Baryon Acoustic Oscillation measure at z=2.225 from the SDSS quasar survey
• The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
• Coarse-Grained Cosmological Perturbation Theory
• Is exponential gravity a viable description for the whole cosmological history?
• Baryon Acoustic Oscillations from the SDSS DR10 galaxies angular correlation function
• A designer approach to $f(Q)$ gravity and cosmological implications
• Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study
• The growth of matter perturbations in some scalar-tensor DE models
• Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD
• Radiative Transfer Modeling of Lyman Alpha Emitters. II. New Effects in Galaxy Clustering
• X-Ray Study of the Outer Region of Abell 2142 with Suzaku
• Dynamical behavior of generic quintessence potentials: constraints on key dark energy observables
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• Is there evidence for dark energy evolution?
• Testing the dark energy with gravitational lensing statistics
• Color Dispersion and Milky Way Reddening Among Type Ia Supernovae
• Predicting Future Space Near-IR Grism Surveys using the WFC3 Infrared Spectroscopic Parallels Survey
• Cross-Correlation Lensing: Determining Galaxy and Cluster Mass Profiles from Statistical Weak Lensing Measurements
• The Abell Cluster A586 and the Detection of the Equivalence Principle
• Modified equation of state, scalar field, and bulk viscosity in Friedmann universe
• Cosmic Acceleration, Dark Energy and Fundamental Physics
• Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements
• Model-independent test of the FLRW metric, the flatness of the Universe, and non-local measurement of $H_0{r}_{\mathrm{d}}$
• A model with interaction of dark components and recent observational data
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• Comparing approximate methods for mock catalogues and covariance matrices I: correlation function
• Wide Angle Effects in Future Galaxy Surveys
• Consistency among distance measurements: transparency, BAO scale and accelerated expansion
• Precision cosmology with voids in the final BOSS data
• Testing General Relativity at Cosmological Scales: Implementation and Parameter Correlations
• Reconstruction of the Scalar-Tensor Lagrangian from a LCDM Background and Noether Symmetry
• A clear and measurable signature of modified gravity in the galaxy velocity field
• The updated luminosity correlations of gamma-ray bursts and cosmological implications
• Dynamics of f(R)-cosmologies containing Einstein static models
• Evaluating backreaction with the peak model of structure formation
• The Sloan Great Wall. Morphology and galaxy content
• Constraints on gravity and dark energy from the pairwise kinematic Sunyaev-Zeldovich effect
• Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
• The age problem in $\Lambda$CDM model
• Can dark energy be dynamical?
• Observational constraints on generalized Proca theories
• On using the CMB shift parameter in tests of models of dark energy
• A generalized equation of state for dark energy
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
• How flat can you get? A model comparison perspective on the curvature of the Universe
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Phases of New Physics in the BAO Spectrum
• Realistic cosmological scenario with non-minimal kinetic coupling
• Testing coupled dark energy models with their cosmological background evolution
• Chasing the phantom: A closer look at Type Ia supernovae and the dark energy equation of state
• An analytic model for the bispectrum of galaxies in redshift space
• On the Validity of Cosmological Fisher Matrix Forecasts
• Cosmological Models and Gamma-Ray Bursts Calibrated by Using Pade Method
• Information content of the non-linear power spectrum: the effect of beat-coupling to large scales
• Relativistic Stars in dRGT Massive Gravity
• Fast and accurate mock catalogue generation for low-mass galaxies
• Phantom Dark Energy Models with a Nearly Flat Potential
• Super Luminous Supernovae as standardizable candles and high redshift distance probes
• The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
• Do cosmological observations allow a negative $\Lambda$?
• Geometrical Constraint on Curvature with BAO experiments
• Probing the cosmographic parameters to distinguish between dark energy and modified gravity models
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• Shedding Light on the Galaxy Luminosity Function
• Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
• A new null diagnostic customized for reconstructing the properties of dark energy from BAO data
• Metric Tests for Curvature from Weak Lensing and Baryon Acoustic Oscillations
• The Fate of the Initial State Fluctuations in Heavy Ion Collisions. III The Second Act of Hydrodynamics
• Applications and Techniques for Fast Machine Learning in Science
• On the impact of $f(Q)$ gravity on the Large Scale Structure
• Gaussian Process Estimation of Transition Redshift
• Improving time-delay cosmography with spatially resolved kinematics
• Constraining cosmic deceleration-acceleration transition with type Ia supernova, BAO/CMB and H(z) data
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample
• Fermion Masses and Flavor Mixings in a Model with $S_4$ Flavor Symmetry
• Strong evidence for an accelerating universe
• The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
• Cosmic Voids in the SDSS DR12 BOSS Galaxy Sample: The Alcock-Paczynski Test
• Cosmological dynamics with non-linear interactions
• A new framework for studying spherically symmetric static solutions in f(R) gravity
• Comparison of dark energy models after Planck 2015
• Estimation of Primordial Spectrum with post-WMAP 3 year data
• Simulation of Astronomical Images from Optical Survey Telescopes using a Comprehensive Photon Monte Carlo Approach
• Cosmic voids in modified gravity models with massive neutrinos
• Constraining cosmological parameters by Gamma Ray Burst X - ray afterglow lightcurves
• Direction Dependence of the Deceleration Parameter
• Cosmological Parameter Uncertainties from SALT-II Type Ia Supernova Light Curve Models
• Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data
• The DEEP2 Galaxy Redshift Survey: Clustering Dependence on Galaxy Stellar Mass and Star Formation Rate at z~1
• 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
• Beyond the perfect fluid hypothesis for dark energy equation of state
• The Clustering of MgII Absorption Systems at z=0.5 and Detection of Cold Gas in Massive Halos
• Tracking quintessence by cosmic shear - Constraints from VIRMOS-Descart and CFHTLS and future prospects
• Improved WIMP-search reach of the CDMS II germanium data
• $\Lambda \alpha$DM: Observational constraints on unified dark matter with constant speed of sound
• Falsifying Paradigms for Cosmic Acceleration
• A new measurement of the expansion history of the Universe at z=1.26 with cosmic chronometers in VANDELS
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• SPACE: the SPectroscopic All-sky Cosmic Explorer
• The clustering of ALFALFA galaxies: dependence on HI mass, relationship to optical samples & clues on host halo properties
• Magnetized CMB observables: a dedicated numerical approach
• An exact quantification of backreaction in relativistic cosmology
• Revisiting the Baryon Fractions of Galaxy Clusters: A Comparison with WMAP 3-year Results
• Exact solutions of three dimensional black holes: Einstein gravity vs F(R) gravity
• Clustering properties of a sterile neutrino dark matter candidate
• Nonlinear growth in modified gravity theories of dark energy
• Pilgrim Dark Energy
• A new parametrization of Hubble parameter in $f(Q)$ gravity
• Cosmological Constraints from a Combination of Galaxy Clustering & Lensing -- II. Fisher Matrix Analysis
• Luminous Red Galaxies in Clusters: Central Occupation, Spatial Distributions, and Mis-centering
• Scientific Synergy Between LSST and Euclid
• Near-ultraviolet Spectroscopy of Star-forming Galaxies from eBOSS: Signatures of Ubiquitous Galactic-scale Outflows
• De Sitter Universe in Nonlocal Gravity
• DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
• The Onset of Gravothermal Core Collapse in Velocity Dependent Self-Interacting Dark Matter Subhaloes
• An improved cosmological bound on the thermal axion mass
• Photon-axion conversion in intergalactic magnetic fields and cosmological consequences
• Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5
• Lookback time as a test for brane cosmology
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• An Intensive HST Survey for z>1 Supernovae by Targeting Galaxy Clusters
• Interacting dark matter and modified holographic Ricci dark energy plus a noninteracting cosmic component
• The Mildly Non-Linear Regime of Structure Formation
• Cosmology of Holographic and New Agegraphic $f(R,T)$ Models
• Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Constraints on Neutrino Masses from Weak Lensing
• Constraints on the Dark Side of the Universe and Observational Hubble Parameter Data
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Spherical collapse model with shear and angular momentum in dark energy cosmologies
• Slow-roll k-essence
• Cosmological Evolution in f(R,T) theory with Collisional Matter
• More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
• Comparison of Standard Ruler and Standard Candle constraints on Dark Energy Models
• Energy conditions and current acceleration of the universe
• Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
• Constraining the Dark Energy Equation of State with HII Galaxies
• Gravitational lenses as cosmic rulers: density of dark matter and dark energy from time delays and velocity dispersions
• Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the ${\sigma }_8$ and $H_0$ tensions
• Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
• The Santiago-Harvard-Edinburgh-Durham void comparison II: unveiling the Vainshtein screening using weak lensing
• Simulating Redshift-Space Distortions for Galaxy Pairs with Wide Angular Separation
• Comparison of an X-ray selected sample of massive lensing clusters with the MareNostrum Universe LCDM simulation
• Evolution and Dynamics of a Matter creation model
• Present bounds on the relativistic energy density in the Universe from cosmological observables
• Empirical H-alpha emitter count predictions for dark energy surveys
• Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case
• The evidence of cosmic acceleration and observational constraints
• Constraints on coupling constant between dark energy and dark matter
• Constraints on reconstructed dark energy model from SN Ia and BAO/CMB observations
• Observational constraints on late-time Lambda(t) cosmology
• The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
• The growth of luminous red galaxies by merging
• Updated Constraints and Forecasts on Primordial Tensor Modes
• Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
• Determining the WIMP mass using direct detection experiments
• Dark matter and dark energy from Bose-Einstein condensate
• Cosmic transparency: A test with the baryon acoustic feature and type Ia supernovae
• New measurements of ${\Omega }_m$ from gamma-ray bursts
• The Limits of Extended Quintessence
• Can dark energy be expressed as a power series of the Hubble parameter?
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• A 2% Distance to z = 0.35 by Reconstructing Baryon Acoustic Oscillations - III : Cosmological Measurements and Interpretation
• Towards an Optimal Reconstruction of Baryon Oscillations
• Implications of a Stochastic Microscopic Finsler Cosmology
• Test of the cosmic evolution using Gaussian processes
• A comprehensive comparison of cosmological models from latest observational data
• Reconstructing the dark energy equation of state with varying couplings
• Neutrino masses and cosmic radiation density: Combined analysis
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• Kaluza-Klein cosmological model in $f(R,T)$ gravity with $\Lambda (T)$
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• The Observed Growth of Massive Galaxy Clusters III: Testing General Relativity on Cosmological Scales
• Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• Testing Low-Redshift Cosmic Acceleration with Large-Scale Structure
• Dark Energy in Practice
• Modelling non-linear redshift-space distortions in the galaxy clustering pattern: systematic errors on the growth rate parameter
• Constraining Primordial Non-Gaussianity with High-Redshift Probes
• Cosmography: Supernovae Union2, Baryon Acoustic Oscillation, Observational Hubble Data and Gamma Ray Bursts
• WMAP5 constraints on the unified model of dark energy and dark matter
• MCMC analysis of WMAP3 and SDSS data points to broken symmetry inflaton potentials and provides a lower bound on the tensor to scalar ratio
• Dark Energy: Recent Developments
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• Cosmology of neutrinos and extra light particles after WMAP3
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• Einstein's Universe: Cosmological structure formation in numerical relativity
• Accelerated Cosmological Models in Modified Gravity tested by distant Supernovae SNIa data
• Quintessence reconstructed: new constraints and tracker viability
• Dependence of the non-linear mass power spectrum on the equation of state of dark energy
• STRIDES: Automated uniform models for 30 quadruply imaged quasars
• A needlet ILC analysis of WMAP 9-year polarisation data: CMB polarisation power spectra
• Cosmological hydrogen recombination: The effect of extremely high-n states
• Power spectrum of the maxBCG sample: detection of acoustic oscillations using galaxy clusters
• Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
• Correlation properties of the kinematic Sunyaev-Zel'dovich effect and implications for Dark Energy
• Observational Constraints on Oscillating Dark-Energy Parametrizations
• Large-Scale Bulk Motions Complicate the Hubble Diagram
• Observational constraints on a logarithmic scalar field dark energy model and black hole mass evolution in the Universe
• Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\Lambda$CDM
• Distance, Growth Factor, and Dark Energy Constraints from Photometric Baryon Acoustic Oscillation and Weak Lensing Measurements
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
• The galaxy power spectrum: precision cosmology from large scale structure?
• Non-minimal quintessence and phantom with nearly flat potentials
• Probing Cosmological Isotropy With Type IA Supernovae
• Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
• Testing the phenomenological interacting dark energy with observational $H(z)$ data
• Dark Energy Constraints after Planck
• Are cosmological neutrinos free-streaming?
• Constraining effective equation of state in $f(Q,T)$ gravity
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Cosmography beyond standard candles and rulers
• Cosmic Equation of state from Strong Gravitational Lensing Systems
• Reconstruction and constraining of the jerk parameter from OHD and SNe Ia observations
• How predictions of cosmological models depend on Hubble parameter data sets
• Inhomogeneities in the universe
• The matter distribution in the local Universe as derived from galaxy groups in SDSS DR12 and 2MRS
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• A sub-horizon framework for probing the relationship between the cosmological matter distribution and metric perturbations
• First Cosmological Constraints on Dark Energy from the Radial Baryon Acoustic Scale
• Can Dark Matter Decay in Dark Energy?
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• First Detection of Cosmic Structure in the 21-cm Intensity Field
• Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations
• Independent Cosmological Constraints from high-z HII Galaxies
• 6+1 lessons from f(R) gravity
• Enriched haloes at redshift $z=2$ with no star-formation: Implications for accretion and wind scenarios
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Gravastars in $f(\mathbb{T},\mathcal{T})$ gravity
• Anisotropic dark energy model with a hybrid scale factor
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• A third alternative to explain recent observations: Future deceleration
• Anisotropic Strange Quintessence Stars in $f(R)$ Gravity
• Accretion Processes for General Spherically Symmetric Compact Objects
• Observational constraint on generalized Chaplygin gas model
• Complete dark energy scenario in $f(Q)$ gravity
• Statistical methods in cosmology
• The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements
• Isocurvature, non-gaussianity and the curvaton model
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering -- towards an accurate model
• Energy conditions in generalized teleparallel gravity models
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• The 21cm Power Spectrum After Reionization
• The clustering of galaxies as a function of their photometrically-estimated atomic gas content
• Large Scale Structure Constraints for a Class of f(R) Theories of Gravity
• Reconciling the local void with the CMB
• Overcoming the Circular Problem for γ-ray Bursts in Cosmological Global Fitting Analysis
• Modified Gravity Explains Dark Matter?
• A New Equation of State for Dark Energy Model
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• The Peculiar Velocities of Local Type Ia Supernovae and their Impact on Cosmology
• Constraining dark energy with gamma-ray bursts
• Reliability of the detection of the Baryon Acoustic Peak
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• SN and BAO constraints on (new) polynomial dark energy parametrizations: current results and forecasts
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• A model of interacting holographic dark energy at the Ricci's scale
• Forecasting the Cosmological Constraints with Anisotropic Baryon Acoustic Oscillations from Multipole Expansion
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space
• Accelerating dark energy models in bianchi Type-V space-time
• Latest supernovae constraints on f(R) cosmologies
• Gravitational energy as dark energy: Concordance of cosmological tests
• Cosmological Constraints on the Modified Entropic Force Model
• Constraining the dark energy equation of state with double source plane strong lenses
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample
• B-modes and the Nature of Inflation
• An evaluation of cosmological models from expansion and growth of structure measurements
• On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
• Constraints on Cold Dark Matter Accelerating Cosmologies and Cluster Formation
• Banana Split: Testing the Dark Energy Consistency with Geometry and Growth
• Annual Modulation in Direct Dark Matter Searches
• Barrow Entropy Cosmology: an observational approach with a hint of stability analysis
• Thermodynamic Behavior of particular $f(R,T)$ Gravity Models
• ISW measurements with photometric redshift surveys: 2MASS results and future prospects
• Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
• LCDM Model in f(T) Gravity: Reconstruction, Thermodynamics and Stability
• Large-Scale Structure of the Universe as a Cosmic Standard Ruler
• Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
• Measuring the transverse baryonic acoustic scale from the SDSS DR11 galaxies
• A Critique of Holographic Dark Energy
• Robust and model-independent cosmological constraints from distance measurements
• Cosmological consequences of a possible $\Lambda$-dark matter interaction
• Stability analysis for cosmological models in $f(R)$ gravity using dynamical system analysis
• How clustering dark energy affects matter perturbations
• Galaxy redshift surveys selected by neutral hydrogen using FAST
• Dark degeneracy I: Dynamical or interacting dark energy?
• Constraints on a generalized deceleration parameter from cosmic chronometers
• Observational constraints on the interacting Ricci dark energy model
• Bandpass Dependence of X-ray Temperatures in Galaxy Clusters
• On Precision Measurement of the Mean Curvature
• Testing the Copernican Principle via Cosmological Observations
• Neutrino mass constraint with the Sloan Digital Sky Survey power spectrum of luminous red galaxies and perturbation theory
• Euclid: Cosmological forecasts from the void size function
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Robust model comparison disfavors power law cosmology
• AIC and BIC for cosmological interacting scenarios
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering
• Dynamical analysis on $f(R,\mathcal{G})$ cosmology
• Constrained $f(Q,T)$ gravity accelerating cosmological model and its dynamical system analysis
• Cosmic tomographies: baryon acoustic oscillations and weak lensing
• The spherical collapse model and cluster formation beyond the $\Lambda$ cosmology: Indications for a clustered dark energy?
• An iterative reconstruction of cosmological initial density fields
• Cosmography with cluster strong lenses: the influence of substructure and line-of-sight halos
• Stability analysis of the Tsallis holographic dark energy model
• Cosmic acceleration without dark energy: Background tests and thermodynamic analysis
• Cosmological constraints on neutrino plus axion hot dark matter
• Can a galaxy redshift survey measure dark energy clustering?
• How closely do baryons follow dark matter on large scales?
• Extended Spherical Collapse and the Accelerating Universe
• Cosmic voids in modified gravity scenarios
• Non-minimally coupled f(R) Cosmology
• The High Redshift Integrated Sachs-Wolfe Effect
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• Holographic hessence models
• Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
• Generalized Holographic and Ricci Dark Energy Models
• Model-independent estimations for the curvature from standard candles and clocks
• Cosmological model with interactions in the dark sector
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Probing elastic interactions in the dark sector and the role of $S_8$
• Dirac Neutrinos with $S_4$ Flavor Symmetry in Warped Extra Dimensions
• Structure formation in cosmologies with oscillating dark energy
• Dark energy, matter creation and curvature
• Holographic Dark Energy Model with Hubble Horizon as an IR Cut-off
• Dark energy scenario consistent with GW170817 in theories beyond Horndeski gravity
• Clustering of Photometric Luminous Red Galaxies II: Cosmological Implications from the Baryon Acoustic Scale
• Matter bispectrum in cubic Galileon cosmologies
• Remarks on the formulation of the cosmological constant/dark energy problems
• Dark Energy Evolution and the Curvature of the Universe from Recent Observations
• Holographic f(T)-gravity model with power-law entropy correction
• Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
• Cosmological data favor Galileon ghost condensate over $\Lambda$CDM
• Constraints on Cosmological Models and Reconstructing the Acceleration History of the Universe with Gamma-Ray Burst Distance Indicators
• Statefinder diagnostic for the modified polytropic Cardassian universe
• Matter Power Spectrum Covariance Matrix from the DEUS-PUR ΛCDM simulations: Mass Resolution and non-Gaussian Errors
• Accelerating cosmologies tested by distance measures
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Constraints on Exotic Matter for An Emergent Universe
• AIC, BIC, Bayesian evidence against the interacting dark energy model
• The foreground wedge and 21 cm BAO surveys
• Gaussian processes reconstruction of dark energy from observational data
• The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 LRG sample: structure growth rate measurement from the anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0
• Measuring deviations from a cosmological constant: a field-space parameterization
• Constraining the expansion rate of the Universe using low-redshift ellipticals as cosmic chronometers
• Observational constraints on a holographic, interacting dark energy model
• Clustering of Luminous Red Galaxies III: Detection of the Baryon Acoustic Peak in the 3-point Correlation Function
• Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach
• Dynamical system analysis for nonminimal torsion-matter coupled gravity
• Streaming velocities and the baryon-acoustic oscillation scale
• Systematic biases on galaxy haloes parameters from Yukawa-like gravitational potentials
• High redshift cosmography: new results and implication for dark energy
• Conservative Constraints on Dark Matter from the Fermi-LAT Isotropic Diffuse Gamma-Ray Background Spectrum
• Effective field description of the Anton-Schmidt cosmic fluid
• Implication of Dark Energy Parametrizations on the Determination of the Curvature of the Universe
• From a Bounce to the Dark Energy Era with $F(R)$ Gravity
• Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
• Multiscale Inference of Matter Fields and Baryon Acoustic Oscillations from the Ly-alpha Forest
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Measuring Dark Energy with Gamma-Ray Bursts and Other Cosmological Probes
• Galaxy Formation as a Cosmological Tool. I: The Galaxy Merger History as a Measure of Cosmological Parameters
• Tachyonic Teleparallel Dark Energy
• New holographic reconstruction of scalar field dark energy models in the framework of chameleon Brans-Dicke cosmology
• Constant sound speed and its thermodynamical interpretation in $f(Q)$ gravity
• Consistency of $f(R)=\sqrt{R^2-R_0^2}$ Gravity with the Cosmological Observations in Palatini Formalism
• Constraints on cosmological models from lens redshift data
• A Unified Approach to Variational Derivatives of Modified Gravitational Actions
• Exact scaling solutions and fixed points for general scalar field
• Fitting the Constitution SNIa Data with Redshift Binned Parameterization Method
• Simulations of Wide-Field Weak Lensing Surveys II: Covariance Matrix of Real Space Correlation Functions
• Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey
• Imprint of DES super-structures on the Cosmic Microwave Background
• Revisit of cosmic age problem
• Cosmological Constraints from Hubble Parameter on f(R) Cosmologies
• Cosmological constraints from the BOSS DR12 void size function
• Can all cosmological observations be accurately interpreted with a unique geometry?
• The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
• Late universe dynamics with scale-independent linear couplings in the dark sector
• Towards equation of state of dark energy from quasar monitoring: Reverberation strategy
• The Universal Einstein Radius Distribution from 10,000 SDSS Clusters
• Constraints on the generalized Chaplygin gas model including gamma-ray bursts via a Markov Chain Monte Carlo approach
• Testing the equation of state for viscous dark energy
• Are There Rotation Measure Gradients Across AGN Jets?
• Lagrangian or Eulerian; Real or Fourier? Not All Approaches to Large-Scale Structure Are Created Equal
• Constraining cosmological parameters in FLRW metric with lensed GW+EM signals
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring H(z) and D_A(z) at z = 0.57 with Clustering Wedges
• Unified dark fluid in Brans-Dicke theory
• The Hubble diagram extended to z>>1: the gamma-ray properties of GRBs confirm the Lambda-CDM model
• Transient cosmic acceleration from interacting fluids
• Self-similarity and universality of void density profiles in simulation and SDSS data
• Is there a concordance value for $H_0$?
• The Sunyaev-Zel'dovich effects from a cosmological hydrodynamical simulation: large-scale properties and correlation with the soft X-ray signal
• Analytic models of Anisotropic Strange Stars in $f(T)$ Gravity with Off-diagonal tetrad
• Cosmology with nonminimal kinetic coupling and a power-law potential
• SPT-GMOS: A Gemini/GMOS-South Spectroscopic Survey of Galaxy Clusters in the SPT-SZ Survey
• Cosmological evolution and statefinder diagnostic for new holographic dark energy model in non flat universe
• How close can an Inhomogeneous Universe mimic the Concordance Model?
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Swiss Cheese and a Cheesy CMB
• Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments
• Cosmological constraints combining H(z), CMB shift and SNIa observational data
• Systematic effects in the sound horizon scale measurements
• Oscillations in the dark energy EoS: new MCMC lessons
• Can structure formation distinguish ΛCDM from non-minimal f(R) Gravity?
• A test of the CPL parameterization for rapid dark energy equation of state transitions
• Response function of the large-scale structure of the universe to the small scale inhomogeneities
• A New Test of the Statistical Nature of the Brightest Cluster Galaxies
• Magnetogenesis, spectator fields and CMB signatures
• Constraints on a variable dark energy model with recent observations
• Nonlinear Power Spectrum from Resummed Perturbation Theory: a Leap Beyond the BAO Scale
• New coupled quintessence cosmology
• Does Chaplygin gas have salvation?
• Accelerating expansion of the universe in modified symmetric teleparallel gravity
• Phantom cosmological model with observational constraints in $f(Q)$ gravity
• Cosmic acceleration in non-flat $f(T)$ cosmology
• An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at $z\sim 0.3$
• Cosmological constraints of phantom dark energy models
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• Cosmological perturbations in Palatini modified gravity
• Baryon Oscillations and Consistency Tests for Photometrically-Determined Redshifts of Very Faint Galaxies
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multi-tracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate
• Anisotropic Magnification Distortion of the 3D Galaxy Correlation: II. Fourier and Redshift Space
• Measuring the cosmic proper distance from fast radio bursts
• F(R) gravity's rainbow and its Einstein counterpart
• Large-Scale Structure Observables in General Relativity
• Is cosmology compatible with sterile neutrinos?
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Latest astronomical constraints on some nonlinear parametric dark energy models
• UV stable, Lorentz-violating dark energy with transient phantom era
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Large-scale tidal effect on redshift-space power spectrum in a finite-volume survey
• Generic feature of future crossing of phantom divide in viable $f(R)$ gravity models
• Absence of anti-correlations and of baryon acoustic oscillations in the galaxy correlation function from the Sloan Digital Sky Survey DR7
• Interacting model of new agegraphic dark energy: observational constraints and age problem
• Quasi-dilaton non-linear massive gravity: Investigations of background cosmological dynamics
• Observational Constraints on Exponential Gravity
• The Imperial IRAS-FSC Redshift Catalogue (IIFSCz)
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• Experimental constraints on the uncoupled Galileon model from SNLS3 data and other cosmological probes
• Modelling and testing the equation of state for (Early) dark energy
• Particle mesh simulations of the Lyman-alpha forest and the signature of Baryon Acoustic Oscillations in the intergalactic medium
• Stability of de Sitter spacetime under isotropic perturbations in semiclassical gravity
• The Acoustic Peak in the Lyman Alpha Forest
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Complete Treatment of Galaxy Two-Point Statistics: Gravitational Lensing Effects and Redshift-Space Distortions
• Time Delay Lens Modelling Challenge
• Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
• Observational evidence of galaxy assembly bias
• Precision cosmology with redshift-space bispectrum: a perturbation theory based model at one-loop order
• Current Constraints on Anisotropic and Isotropic Dark Energy Models
• Primordial non-Gaussianity from the Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey I: Catalogue Preparation and Systematic Mitigation
• 3D Genus Topology of Luminous Red Galaxies
• Accelerating Universe scenario in anisotropic $f\left(Q\right)$ cosmology
• QSO-LRG 2-Point Cross-Correlation Function and Redshift-Space Distorions
• The Sloan Digital Sky Survey Quasar Lens Search. IV. Statistical Lens Sample from the Fifth Data Release
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Dark energy: investigation and modeling
• $\Lambda (t)$ cosmology induced by a slowly varying Elko field
• Dark energy records in lensed cosmic microwave background
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• COSMIC BIRTH: Efficient Bayesian Inference of the Evolving Cosmic Web from Galaxy Surveys
• Analytical models of supermassive black holes in galaxies surrounded by dark matter halos
• Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces
• Generalization of Regular Black Holes in General Relativity to $f(R)$ Gravity
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Angular correlation function of 1.5 million LRGs: clustering evolution and a search for BAO
• Cosmological reconstruction of $f(T,\mathcal{T})$ Gravity
• Cosmology with dropout selection: Straw-man surveys and CMB lensing
• Looking Beyond Lambda with the Union Supernova Compilation
• Modified gravity for surveys
• Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope
• The LambdaCDM model on the lead -- a Bayesian cosmological models comparison
• The Scale of Cosmic Isotropy
• Magnetized strange quark matter in $f(R,T)$ gravity with bilinear and special form of time varying deceleration parameter
• Dark energy as a mirage
• Constraints on modified gravity from the BOSS galaxy survey
• Exploring stable models in $f(R;T;R_{\mu \nu }{T}^{\mu \nu })$ gravity
• Hierarchical clustering in chameleon $f(R)$ gravity
• Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
• Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $\Lambda$CDM simulation
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• The nonlinear matter power spectrum
• Investigating the dark energy phenomenon in $f(R,L_m)$ cosmological models with observational constraints
• Background history and cosmic perturbations for a general system of self-conserved dynamical dark energy and matter
• Testing deviations from $\Lambda$CDM with growth rate measurements from 6 Large Scale Structure Surveys at $\mathbf{z}=0.06$ to 1
• Massive Photon and Dark Energy
• Is the evidence for dark energy secure?
• Cosmic perturbations with running G and Lambda
• Testable dark energy predictions from current data
• Non-vacuum Solutions of Bianchi Type VI_0 Universe in f(R) Gravity
• Power spectrum of halo intrinsic alignments in simulations
• What is the best way to measure baryonic acoustic oscillations?
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology
• Model independent constraints on the cosmological expansion rate
• Dark energy model with variable $q$ and $\omega$ in LRS Bianchi-II space-time
• Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey
• Tension in the Void: Cosmic Rulers Strain Inhomogeneous Cosmologies
• Observational Constraints on Modified Chaplygin Gas from Cosmic Growth
• Viscous cosmology in the Weyl-type $f(Q,T)$ gravity
• Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
• How robust are inflation model and dark matter constraints from cosmological data?
• The growth of linear perturbations in the DGP model
• On the determination of curvature and dynamical Dark Energy
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
• Redshift Measurement and Spectral Classification for eBOSS Galaxies with the Redmonster Software
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
• How runaway stars boost galactic outflows
• Modified Dust and the Small Scale Crisis in CDM
• Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters
• Gravitationally induced adiabatic particle production: From Big Bang to de Sitter
• Scalar field cosmology modified by the Generalized Uncertainty Principle
• Regularized cosmological power spectrum and correlation function in modified gravity models
• Galaxy and Mass Assembly (GAMA): The evolution of bias in the radio source population to z ~ 1.5
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• Dark Energy Parametrizations and the Curvature of the Universe
• The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis
• Shedding Light on Dark Matter: A Faraday Rotation Experiment to Limit a Dark Magnetic Moment
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Cosmological Constraints on Decaying Dark Matter
• $f(R,T)=f(R)+\lambda T$ gravity models as alternatives to cosmic acceleration
• Interacting Cosmological Fluids and the Coincidence Problem
• What is parameterized $Om(z)$ diagnostics telling us in light of recent observations?
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• Scale-dependent bias and the halo model
• Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
• Constraints on Kinematic Model from Recent Cosmic Observations: SN Ia, BAO and Observational Hubble Data
• Cosmic acceleration from modified gravity with Palatini formalism
• Dark matter-dark energy interaction for a time-dependent equation of state
• FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
• Cosmological investigations of (extended) nonlinear massive gravity schemes with non-minimal coupling
• Age constraints on the cosmic equation of state
• Hubble Space Telescope Observations of Nine High-Redshift ESSENCE Supernovae
• Toward More Realistic Forecasting of Dark Energy Constraints from Galaxy Redshift Surveys
• Revisiting the parametrization of Equation of State of Dark Energy via SNIa Data
• Constraints on growth index parameters from current and future observations
• Early Dark Energy at High Redshifts: Status and Perspectives
• Time drift of cosmological redshifts and its variance
• Coupling constant constraints in a nonminimally coupled phantom cosmology
• An Interacting Dark Energy Model for the Expansion History of the Universe
• Reconstruction Procedure in Nonlocal Cosmological Models
• Structure Formation in Modified Gravity Scenarios
• Testing the isotropy of the Universe with type Ia supernovae in a model-independent way
• Predicting Hα emission line galaxy counts for future galaxy redshift surveys
• A Hybrid Deep Learning Approach to Cosmological Constraints From Galaxy Redshift Surveys
• Quintessential inflation: A tale of emergent and broken symmetries
• Exploring the evidence for a large local void with supernovae Ia data
• Bulk viscous embedded hybrid dark energy models
• Model-independent cosmological constraints from growth and expansion
• Safely smoothing spacetime: backreaction in relativistic cosmological simulations
• Analytic rotating black hole solutions in $N$-dimensional $f(T)$ gravity
• The part and the whole: voids, supervoids, and their ISW imprint
• Method for Direct Measurement of Cosmic Acceleration by 21-cm Absorption Systems
• Screening of cosmological constant for De Sitter Universe in non-local gravity, phantom-divide crossing and finite-time future singularities
• Constraints on the anisotropy of dark energy
• Space-based research in fundamental physics and quantum technologies
• Cosmology in beyond-generalized Proca theories
• Cosmology Inference from Biased Tracers using the EFT-based Likelihood
• Future Oscillations around Phantom Divide in f(R) Gravity
• Cosmological Perturbations of Extreme Axion in the Radiation Era
• Singularity Problem in Teleparallel Dark Energy Models
• Model independent constraints on transition redshift
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Matter power spectrum from a Lagrangian-space regularization of perturbation theory
• Model-Independent Constraints on Lorentz Invariance Violation via the Cosmographic Approach
• Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\mathrm{eff}}$=0.85 from the final dataset
• Unbiased methods for removing systematics from galaxy clustering measurements
• Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?
• Thermodynamics and Phase Transition of Spherically Symmetric Black Hole in de Sitter Space from Rényi Statistics
• Strong energy condition and the repulsive character of f(R) gravity
• Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
• Probing deviations from General Relativity with the Euclid spectroscopic survey
• Clustering of photometric luminous red galaxies I : Growth of Structure and Baryon Acoustic Feature
• Detectability of Torsion Gravity via Galaxy Clustering and Cosmic Shear Measurements
• Cosmological dynamics of fourth order gravity: A compact view
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• Linearisation with Cosmological Perturbation Theory
• Estimating relic magnetic fields from CMB temperature correlations
• Global and Local Effects of Rotation: Observational Aspects
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• Bayesian Evidence for a Cosmological Constant using new High-Redshift Supernovae Data
• Cosmological Solutions of a Nonlocal Model with a Perfect Fluid
• Unbiased pseudo-Cl power spectrum estimation with mode projection
• A step towards testing general relativity using weak gravitational lensing and redshift surveys
• Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
• The minimally extended Varying Speed of Light (meVSL)
• X-ray Plateaus in Gamma-Ray Burst Afterglows and Their Application in Cosmology
• Regarding the Line-of-Sight Baryonic Acoustic Feature in the Sloan Digital Sky Survey and Baryon Oscillation Spectroscopic Survey Luminous Red Galaxy Samples
• Possible antigravity regions in $F(R)$ theory?
• Cosmological distance indicators
• Testing the DGP model with ESSENCE
• Impact of shell crossing and scope of perturbative approaches in real and redshift space
• Reconstruction of the neutrino mass as a function of redshift
• Tension in the Recent Type Ia Supernovae Datasets
• Modified Holographic Dark Energy
• $f(R)$ gravity theories in the Palatini Formalism constrained from strong lensing
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Pairwise-Inverse-Probability and Angular Correction for Fibre Collisions in Clustering Measurements
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Teleparallel Dark Energy with Purely Non-minimal Coupling to Gravity
• The Jubilee ISW Project I: simulated ISW and weak lensing maps and initial power spectra results
• Cosmological implications and structure formation from a time varying vacuum
• Large-Scale Structure in Brane-Induced Gravity I. Perturbation Theory
• A new method for the Alcock-Paczynski test
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• Lensing Corrections to Features in the Angular Two-Point Correlation Function and Power Spectrum
• The thawing dark energy dynamics: Can we detect it?
• Gauge-Invariance and Infrared Divergences in the Luminosity Distance
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Large Scale Structure of the Universe
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Forecasts for Dark Energy Measurements with Future HI Surveys
• HI intensity mapping with MeerKAT: 1/f noise analysis
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• Low redshift observational constraints on tachyon models of dark energy
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• The Coincidence Problem and Interacting Holographic Dark Energy
• Scale-dependent Galaxy Bias
• First Detection of the BAO Signal from Early DESI Data
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• Measuring the 2D Baryon Acoustic Oscillation signal of galaxies in WiggleZ: Cosmological constraints
• Chaos in the motion of a test scalar particle coupling to Einstein tensor in Schwarzschild-Melvin black hole spacetime
• The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < z < 1.46
• The Cosmic Microwave Background for Pedestrians: A Review for Particle and Nuclear Physicists
• Thermodynamical aspects of Bianchi type-I Universe in quadratic form of $f\left(Q\right)$ gravity and observational constraints
• Connecting LHC, ILC, and Quintessence
• A novel teleparallel dark energy model
• Kaluza-Klein Cosmology With Modified Holographic Dark Energy
• Revisiting the WMAP - NVSS angular cross correlation. A skeptic's view
• Observational constraints on cosmological models with Chaplygin gas and quadratic equation of state
• Baryon effects on void statistics in the EAGLE simulation
• New Exact Spherically Symmetric Solutions in $f(R,\varphi ,X)$ gravity by Noether's symmetry approach
• Non-linear evolution of the BAO scale in alternative theories of gravity
• Excursion Sets and Non-Gaussian Void Statistics
• Testing dark energy models with a new sample of strong-lensing systems
• Backreaction from non-conformal quantum fields in de Sitter spacetime
• Narrowing Constraints with Type Ia Supernovae: Converging on a Cosmological Constant
• Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land
• The signature of dark energy perturbations in galaxy cluster surveys
• Using a phenomenological model to test the coincidence problem of dark energy
• Reconstructing the interaction rate in holographic models of dark energy
• Transition Redshift: New constraints from parametric and nonparametric methods
• The Redshift Sensitivities of Dark Energy Surveys
• Quintessence with Yukawa Interaction
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• Gamma ray burst constraints on cosmological models from the improved Amati correlation
• Cosmic distance inference from purely geometric BAO methods: Linear Point standard ruler and Correlation Function Model Fitting
• Emergent Universe from A Composition of Matter, Exotic Matter and Dark Energy
• Observational constraints on non-minimally coupled Galileon model
• Quintessence Universe and cosmic acceleration in $f(Q,T)$ gravity
• A parametrization for the growth index of linear matter perturbations
• Modeling the Very Small-Scale Clustering of Luminous Red Galaxies
• New Parametrization for the Scale Dependent Growth Function in General Relativity
• Adjoint SUSY $SU(5)$ Grand Unified Model with $S_4$ Flavor Symmetry
• Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak
• Running vacuum in QFT in FLRW spacetime: The dynamics of ${\rho }_{\mathrm{vac}}(H)$ from the quantized matter fields
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Shedding Light on Dark Matter at Colliders
• Luminous Red Galaxies in hierarchical cosmologies
• Cosmological Parameters from the SDSS DR5 Velocity Dispersion Function of Early-Type Galaxies through Radio-Selected Lens Statistics
• 3D Spherical Analysis of Baryon Acoustic Oscillations
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• Interacting viscous dark fluids
• Relativistic Modified Newtonian Dynamics from String Theory?
• Separating out the Alcock-Paczynski Effect on 21cm Fluctuations
• Anisotropies of galaxy ellipticity correlations in real and redshift space: angular dependence in linear tidal alignment model
• The Hubble Space Telescope Cluster Supernova Survey: VI. The Volumetric Type Ia Supernova Rate
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• High Redshift Standard Candles: Predicted Cosmological Constraints
• Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS
• The spatial distribution of cold gas in hierarchical galaxy formation models
• Testing the distance duality relation with present and future data
• Internal Robustness: systematic search for systematic bias in SN Ia data
• The transient and the late time attractor tachyon dark energy: Can we distinguish it from quintessence ?
• Evolution of The Velocity-Dispersion Function of Luminous Red Galaxies: A Hierarchical Bayesian Measurement
• Testing phenomenological and theoretical models of dark matter density profiles with galaxy clusters
• A Study of Finite-time Singularities of Loop Quantum Cosmology Interacting Multifluids
• Dwarf galaxies imply dark matter is heavier than $2.2\times 10^{-21}\mathbf{eV}$
• Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
• Bouncing Universe and Reconstructing Vector Field
• Testing logarithmic corrections on $R^2$-exponential gravity by observational data
• Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
• Cosmic Constraint on Ricci Dark Energy Model
• Logarithmic corrected Polynomial $f(R)$ inflation mimicking a cosmological constant
• Constraining the evolution of dark energy with type Ia supernovae and gamma-ray bursts
• The REFLEX II galaxy cluster survey: power spectrum analysis
• Latest Observational Constraints to the Ghost Dark Energy Model by Using Markov Chain Monte Carlo Approach
• Combining perturbation theories with halo models for the matter bispectrum
• Statistical Test of Distance--Duality Relation with Type Ia Supernovae and Baryon Acoustic Oscillations
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
• Dynamical Evolution of Interacting Modified Chaplygin Gas
• New Limits on Coupled Dark Energy from Planck
• $E_{\mathrm{iso}}$-$E_{\mathrm{p}}$ correlation of gamma ray bursts: calibration and cosmological applications
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
• The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase
• Using the Zeldovich dynamics to test expansion schemes
• Supernovae as seen by off-center observers in a local void
• Cosmic propagators at two-loop order
• An optimized correlation function estimator for galaxy surveys
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
• Small-scale clumping at recombination and the Hubble tension
• A See-Saw $S_4$ model for fermion masses and mixings
• The evolution of the [OII], Hβ and [OIII] emission-line luminosity functions over the last nine billions years
• QCD ghost f(T)-gravity model
• Roles of dark energy perturbations in the dynamical dark energy models: Can we ignore them?
• Dynamical Collapse of Charged Scalar Field in Phantom Gravity
• Reconstructing a String-Inspired Quintom Model of Dark Energy
• Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement
• Reduction of Cosmological Data for the Detection of Time-varying Dark Energy Density
• The High-Mass End of the Red Sequence at z~0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function
• Modified gravity without dark matter
• Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology
• Observational constraints on cosmic neutrinos and dark energy revisited
• Estimating the galaxy two-point correlation function using a split random catalog
• Observational signatures of the theories beyond Horndeski
• Cosmological constraints on dark energy in $f(Q)$ gravity: A parametrized perspective
• Tensions with the flat $\mathbf{\Lambda }$CDM model from high-redshift cosmography
• Constraints on the cosmic expansion rate at redshift 2.3 from the Lyman-$\alpha$ forest
• Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• Characterizing the linear growth rate of cosmological density perturbations in an f(R) model
• Isobaric Reconstruction of the Baryonic Acoustic Oscillation
• Confronting the relaxation mechanism for a large cosmological constant with observations
• Comparison of Recent SnIa datasets
• Cosmological Constraints from Hubble parameter $H(z)$ and SN Ia observations
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Figures of merit for present and future dark energy probes
• Supernova tests of the timescape cosmology
• Beyond Two Dark Energy Parameters
• Dynamics of holographic vacuum energy in the DGP model
• Two-fluid atmosphere from decelerating to accelerating FRW dark energy models
• Observational Constraints of Modified Chaplygin Gas in Loop Quantum Cosmology
• Cosmological parameter extraction and biases from type Ia supernova magnitude evolution
• Bulk viscous matter and the cosmic acceleration of the universe in $f(Q,T)$ gravity
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?
• 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
• Coupled quintessence and vacuum decay
• Baryon Acoustic Oscillations and Dynamical Dark Energy
• Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power Spectrum
• Dark viscous fluid described by a unified equation of state in cosmology
• Couplings between holographic dark energy and dark matter
• A New $Om(z)$ Diagnostic of Dark Energy in General Relativity Theory
• Confronting dark energy models mimicking $\Lambda$CDM epoch with observational constraints: future cosmological perturbations decay or future Rip?
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• Smoothing the $H_0$ tension with a dynamical dark energy model
• Power-law solution for homogeneous and isotropic universe in $f(R,T)$ gravity
• Power law correlations in galaxy distribution and finite volume effects from the Sloan Digital Sky Survey Data Release Four
• Bright High z SnIa: A Challenge for LCDM?
• Bayesian Comparison of Interacting Scenarios
• Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant
• Big Bang Nucleosynthesis constraints on $f(T,\mathcal{T})$ gravity
• Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect
• Cosmic opacity: cosmological-model-independent tests from gravitational waves and Type Ia Supernova
• Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
• Can Old Galaxies at High Redshifts and Baryon Acoustic Oscillations Constrain H_0?
• Constrained evolution of effective equation of state parameter in non-linear $f(R,L_m)$ dark energy model: Insights from Bayesian analysis of cosmic chronometers and Pantheon samples
• Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey
• Holographic Dark Energy with Cosmological Constant
• The growth factor of matter perturbations in an f(R) gravity
• Constraints on Lorentz Invariance Violation with gamma-ray bursts via a Markov Chain Monte Carlo approach
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Constraining An Exact Brans-Dicke gravity theory with Recent Observations
• A New Statistic for Analyzing Baryon Acoustic Oscillations
• Luminosity distance and anisotropic sky-sampling at low redshifts: a numerical relativity study
• Dark energy, gravitation and supernovae
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Identification of filamentary structures in the environment of superclusters of galaxies in the Local Universe
• Exploring the Latest Union2 SNIa Dataset by Using Model-Independent Parametrization Methods
• Calibration of GRB Luminosity Relations with Cosmography
• BAO from angular clustering: optimization and mitigation of theoretical systematics
• The effect of FIR emission from SDSS galaxies on the SFD Galactic extinction map
• Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in $f(R)$ gravity
• Cosmological model-independent test of $\Lambda$CDM with two-point diagnostic by the observational Hubble parameter data
• Agegraphic dark energy: growth index and cosmological implications
• Observational tests for Λ(t)CDM cosmology
• Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
• The effect of photometric redshift uncertainties on galaxy clustering and baryonic acoustic oscillations
• Dynamics and cosmological constraints on Brans-Dicke cosmology
• Limits on statistical anisotropy from BOSS DR12 galaxies using bipolar spherical harmonics
• Photometric Redshifts from SDSS Images with an Interpretable Deep Capsule Network
• Holographic Dark Energy from Fluid/Gravity Duality Constraint by Cosmological Observations
• Study Of Tachyon Dynamics For Broad Classes of Potentials
• Supernova light-curve fitters and Dark Energy
• FLRW cosmology with EDSFD parametrization
• 2MTF - VII. 2MASS Tully-Fisher survey final data release: distances for 2,062 nearby spiral galaxies
• Constraining DGP Gravity from Observational Data
• Multiple kinetic k-essence, phantom barrier crossing and stability
• Renormalized Newtonian Cosmic Evolution with Primordial Non-Gaussianity
• Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
• Evidence for an environment-dependent shift in the baryon acoustic oscillation peak
• Modeling Transit Dark Energy in $f(R,L_m)$-gravity
• Reionisation in sterile neutrino cosmologies
• Thermodynamic properties of modified gravity theories
• Cosmological tests of sudden future singularities
• Observational analysis of late-time acceleration in $f(Q,L_m)$ gravity
• CLARA's view on the escape fraction of Lyman-Alpha photons in high redshift galaxies
• Modified holographic dark energy in DGP brane world
• Induced cosmological constant and other features of asymmetric brane embedding
• Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
• Exploring accelerated expansion in the universe: A study of $f(Q,T)$ gravity with parameterized EoS and cosmological constraints
• Comparing two approaches to Hawking radiation of Schwarzschild-de Sitter black holes
• Correction to Lagrangian for Bouncing Cosmologies in $f(Q)$ Gravity
• Estimating Covariance Matrices for Two- and Three-Point Correlation Function Moments in Arbitrary Survey Geometries
• Beyond delta: Tailoring marked statistics to reveal modified gravity
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• Confronting the Hubble Diagram of Gamma-Ray Bursts with Cardassian Cosmology
• The correlation function of galaxy clusters and detection of baryon acoustic oscillations
• Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data
• Sunyaev-Zel'dovich clusters reconstruction in multiband bolometer camera surveys
• Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Cosmography with next-generation gravitational wave detectors
• Geodesic Deviation Equation in $f(R,T)$ Gravity
• Small-scale galaxy clustering in the EAGLE simulation
• Spectral Evolution in High Redshift Quasars from the Final BOSS Sample
• Semi-analytical approach to magnetized temperature autocorrelations
• Cluster Ellipticities as a Cosmological Probe
• Quantifying systematic uncertainties in supernova cosmology
• Magnetized Bianchi Type $V{I}_0$ Barotropic Massive String Universe with Decaying Vacuum Energy Density $\Lambda$
• Variable Cosmological Constant model: the reconstruction equations and constraints from current observational data
• Constraining $H_0$ from Sunyaev-Zel'dovich effect, Galaxy Clusters X-ray data, and Baryon Oscillations
• Implications of a Scalar Dark Force for Terrestrial Experiments
• Parameter dependence of magnetized CMB observables
• An exploration of an early gravity transition in light of cosmological tensions
• Expansion schemes for gravitational clustering: computing two-point and three-point functions
• The BINGO Project II: Instrument Description
• Dynamical stability of K-essence field interacting non-minimally with a perfect fluid
• A Geometrical Approach to Strong Gravitational Lensing in f(R) Gravity
• Effect of Intergalactic Medium on the Observability of Lyman Alpha Emitters during Cosmic Reionization
• Polytropic dark matter flows illuminate dark energy and accelerated expansion
• Parameters of cosmological models and recent astronomical observations
• Observational constraint on the varying speed of light theory
• Intrinsic alignment statistics of density and velocity fields at large scales: Formulation, modeling, and baryon acoustic oscillation features
• The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at $z=0.59$
• Testing for dynamical dark energy models with redshift-space distortions
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Sources of $H_0$-tensions in dark energy scenarios
• One-point remapping of Lagrangian perturbation theory in the mildly non-linear regime of cosmic structure formation
• Prediction of Supernova Rates in Known Galaxy-galaxy Strong-lens Systems
• Observational constraints on the equation of state of viscous fluid in $f(R,T)$ gravity
• Exploring the Dark Universe: constraints on dynamical Dark Energy models from CMB, BAO and growth rate measurements
• Is there evidence for anomalous dipole anisotropy in the large-scale structure?
• Breaking parameter degeneracy in interacting dark energy models from observations
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• Constraining the Expansion History and Early Dark Energy with Line Intensity Mapping
• Constraints on Tsallis Cosmology from Big Bang Nucleosynthesis and the Relic Abundance of Cold Dark Matter Particles
• Post-Planck Dark Energy Constraints
• Linear Point and Sound Horizon as Purely Geometric standard rulers
• Constraints on f(R) cosmologies from strong gravitational lensing systems
• Measuring large-scale structure with quasars in narrow-band filter surveys
• Direct evidence of acceleration from distance modulus redshift graph
• The effect of redshift-space distortions on projected 2-pt clustering measurements
• Dissipative Liouville Cosmology: A Case Study
• Redshift-space streaming velocity effects on the Lyman-$\alpha$ forest baryon acoustic oscillation scale
• Constraining the Schwarzschild-de Sitter Solution in Models of Modified Gravity
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Collision Avoidance in Next-generation Fiber Positioner Robotic System for Large Survey Spectrograph
• Thermodynamics and dark energy
• Weighing the Universe with Photometric Redshift Surveys and the Impact on Dark Energy Forecasts
• $H_0$ Tension in Torsion-based Modified Gravity
• A fast semi-discrete optimal transport algorithm for a unique reconstruction of the early Universe
• Constraints on Energy Momentum Squared Gravity from cosmic chronometers and Supernovae Type Ia data
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• The improved Amati correlations from Gaussian copula
• Cosmological constraints to dark matter with two- and many-body decays
• Computing the Small-Scale Galaxy Power Spectrum and Bispectrum in Configuration-Space
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): ${\Omega }_{{\mathrm{m}}_0}$ from the galaxy clustering ratio measured at $z\sim 1$
• Exploring late-time cosmic acceleration: A study of a linear $f(T)$ cosmological model using observational data
• Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect
• Non-Gravitational Contributions to the Clustering of Ly-alpha Selected Galaxies: Implications for Cosmological Surveys
• Bayesian evidence for $\alpha$-attractor dark energy models
• A comprehensive investigation on the slowing down of cosmic acceleration
• Test of the FLRW metric and curvature with strong lens time delays
• Large-scale galaxy correlations as a test for dark energy
• Accretion onto Some Well-Known Regular Black Holes
• Background cosmological dynamics in $f(R)$ gravity and observational constraints
• Observational constrained $F(R,\mathcal{G})$ gravity cosmological model and the dynamical system analysis
• Zeta Function Methods and Quantum Fluctuations
• Reconstructing the history of dark energy using maximum entropy
• Reconstruction and Stability Analysis of Some Cosmological Bouncing Solutions in $F(\mathcal{R},T)$ Theory
• Cosmological models with a Hybrid Scale Factor
• Cosmology with interaction in the dark sector
• Gravitational waves in the presence of a cosmological constant
• Cosmological constant and late transient acceleration of the universe in the Horava-Witten Heterotic M-Theory on S^{1}/Z_{2}
• Have Baryonic Acoustic Oscillations in the galaxy distribution really been measured?
• Constraining the $\Lambda$CDM and Galileon models with recent cosmological data
• Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
• Cosmology with Ricci dark energy
• Is thermodynamics of the universe bounded by the event horizon a Bekenstein system?
• How does non-linear dynamics affect the baryon acoustic oscillation?
• Domain wall solution in $F(R)$ gravity and variation of the fine structure constant
• Forecasting neutrino masses from combining KATRIN and the CMB: Frequentist and Bayesian analyses
• Constraining the Anisotropy of the Universe from Supernovae and Gamma-ray Bursts
• Gravitational quantum effects on power spectra and spectral indices with higher-order corrections
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• The effects of massive neutrinos on the linear point of the correlation function
• Slow-roll freezing quintessence
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• BAO reconstruction: a swift numerical action method for massive spectroscopic surveys
• Non-adiabatic Chaplygin gas
• Detecting quantum gravitational effects of loop quantum cosmology in the early universe?
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Simulations of BAO reconstruction with a quasar Lyman-alpha survey
• Redshift-Space Enhancement of Line-of-Sight Baryon Acoustic Oscillations in the SDSS Main-Galaxy Sample
• Testing tidal alignment models for anisotropic correlations of halo ellipticities with N-body simulations
• Observing Cosmological Processes in Real Time with Repeating Fast Radio Bursts
• Analysing dissipative effects in the $\Lambda$CDM model
• The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering
• CMB Temperature and Matter Power Spectrum in a Decay Vacuum Dark Energy Model
• Generalised nonminimally gravity-matter coupled theory
• Oscillating universe in massive gravity
• The 2QDES Pilot : The luminosity and redshift dependence of quasar clustering
• Luminous Red Galaxy Clustering at z~0.7 - First Results using AAOmega
• Modelling the Accelerating Universe with $f(Q)$ Gravity: Observational Consistency
• The spatial distribution of Milky Way satellites, gaps in streams and the nature of dark matter
• First Constraints on Growth Rate from Redshift-Space Ellipticity Correlations of SDSS Galaxies at $0.16<z<0.70$
• Galaxy-Galaxy Lensing in HSC: Validation Tests and the Impact of Heterogeneous Spectroscopic Training Sets
• Noether symmetries and boundary terms in extended Teleparallel gravity cosmology
• Weyl type $f(Q,T)$ gravity observational constrained cosmological model
• The distinctions between $\Lambda$CDM and $f(T)$ gravity according Noether symmetry
• Beating non-linearities: improving the Baryon Acoustic Oscillations with the linear point
• Graph Database Solution for Higher Order Spatial Statistics in the Era of Big Data
• Cosmological Constraints on Variable Warm Dark Matter
• Distance Measurements from Supernovae and Dark Energy Constraints
• Curvature from strong gravitational lensing: a spatially closed Universe or systematics?
• Measuring Distance Ratios with CMB-Galaxy Lensing Cross-correlations
• Rotating and non-rotating AdS black holes in $f(\mathcal{T})$ gravity non-linear electrodynamics
• Expansion history and f(R) modified gravity
• Solving the main cosmological puzzles with a generalized time varying vacuum energy
• Constraining massive gravity with recent cosmological data
• Prospects for detecting the 326.5 MHz redshifted 21 cm HI signal with the Ooty Radio Telescope (ORT)
• Optimal Reconstruction of Baryon Acoustic Oscillations for DESI 2024
• Using the cluster mass function from weak lensing to constrain neutrino masses
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Generalized CMB initial conditions with pre-equality magnetic fields
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: selecting emission line galaxies using the Fisher discriminant
• Reconstructing a String-Inspired Non-minimally Coupled Quintom Model
• Statistical Classification Techniques for Photometric Supernova Typing
• Probing the cosmic opacity from Future Gravitational Wave Standard Sirens
• Gravitational energy and cosmic acceleration
• Dark energy and cosmic curvature: Monte-Carlo Markov Chain approach
• Evolution of spherical overdensities in holographic dark energy models
• Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
• DEMNUni: disentangling dark energy from massive neutrinos with the void size function
• BAO cosmography
• Dark-Energy Dynamics Required to Solve the Cosmic Coincidence
• Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach
• Constraining viscous dark energy equation of state in $f(R,L_m)$ gravity
• Galaxy surveys, inhomogeneous reionization, and dark energy
• Assisted dark energy
• How well do we know the polar hydrogen distribution on the Moon?
• Supernovae and Cosmology
• Testing modified gravity models with recent cosmological observations
• Estimating CDM Particle Trajectories in the Mildly Non-Linear Regime of Structure Formation. Implications for the Density Field in Real and Redshift Space
• Cosmological constraints on dark matter annihilation and decay: Cross-correlation analysis of the extragalactic $\gamma$-ray background and cosmic shear
• Probing the dynamical behavior of dark energy
• Understanding the nature of luminous red galaxies (LRGs): Connecting LRGs to central and satellite subhalos
• Bouncing universe with the non-minimally coupled scaler field and its reconstructing
• Exploring Large-scale Structure with Billions of Galaxies
• Higher-order coupled quintessence
• Growth of matter perturbations in the extended viscous dark energy models
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Cosmological model with decaying vacuum energy law from principles of quantum mechanics
• Galaxy clustering dependence on the $\left[\mathrm{O}\mathrm{II}\right]$ emission line luminosity in the local Universe
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• How the Big Bang Ends up Inside a Black Hole
• Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
• Formulation and constraints on decaying dark matter with finite mass daughter particles
• The Linear Point: A cleaner cosmological standard ruler
• Some FRW Models of Accelerating Universe with Dark Energy
• Cosmological model of the interaction between dark matter and dark energy
• Connecting inflation with late cosmic acceleration by particle production
• Pre-Inflationary Spacetime in String Cosmology
• Isotropic vs. Anisotropic components of BAO data: a tool for model selection
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Cosmological data analysis of f(R) gravity models
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Deviation from the Cosmological Constant or Systematic Errors?
• Dark matter from dark energy-baryonic matter couplings
• The absolute age of the globular cluster M15 using near-infrared adaptive optics images from PISCES/LBT
• Power-law Parameterized Quintessence Model
• Reheating in 3-form inflation
• Forecasting the Dark Energy Measurement with Baryon Acoustic Oscillations: Prospects for the LAMOST surveys
• Observational constraints on new generalized Chaplygin gas model
• CMB anisotropy science: a review
• Tracing the cosmic history by Gauss-Bonnet gravity
• Detecting the cosmic acceleration with current data
• A magnetized completion of the $\Lambda$CDM paradigm
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Static Cylindrically Symmetric Interior Solutions in f(R) Gravity
• The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements
• Hunting down systematics in baryon acoustic oscillations after cosmic high noon
• Constraining the cosmological model of modified $f(Q)$ gravity: Phantom dark energy and observational insights
• Kantowski-Sachs Universe Models in $f(T)$ Theory of Gravity
• Multiplicative errors in the galaxy power spectrum: self-calibration of unknown photometric systematics for precision cosmology
• Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
• Definitive Test of the R_h=ct Universe Using Redshift Drift
• Observational Constraints with Recent Data on the DGP Modified Gravity
• Cosmological constraints on dark energy models using DESI BAO 2024
• Non-Gaussian errors of baryonic acoustic oscillations
• Interacting Two-Fluid Viscous Dark Energy Models In Non-Flat Universe
• Cosmological Models and Latest Observational Data
• Decoherence out of fire: Purity loss in expanding and contracting universes
• Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
• A Cyclic Universe With Varying Cosmological Constant in $f(R,T)$ gravity
• The Influence of Galaxy Formation Physics on Weak Lensing Tests of General Relativity
• Generalized Chaplygin gas model: Cosmological consequences and statefinder diagnosis
• Can the quantum vacuum fluctuations really solve the cosmological constant problem?
• Effects of voids on the reconstruction of the equation of state of Dark Energy
• Equations of State in the Brans-Dicke cosmology
• A model independent approach to the study of $f(R)$ cosmologies with expansion histories close to $\Lambda$CDM
• The Evolution of Our Local Cosmic Domain: Effective Causal Limits
• Generalized Holographic Dark Energy and its Observational Constraints
• Observational constraints on decaying vacuum dark energy model
• The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1
• On the impact of intergalactic dust on cosmology with type Ia supernovae
• Dark matter searches at LHC
• The dynamical viability of scalar-tensor gravity theories
• Unified Dark Fluid and Cosmic Transit Models in Brans-Dicke Theory
• Crossing the phantom divide in brane cosmology with curvature corrections and brane-bulk energy transfer
• Broadband distortion modeling in Lyman-$\alpha$ forest BAO fitting
• Analytic study on backreacting holographic superconductors with dark matter sector
• Model-independent determination of the cosmic expansion rate. I. Application to type-Ia supernovae
• Covariance matrices for halo number counts and correlation functions
• Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism
• Galaxy cluster angular size data constraints on dark energy
• Accuracy of cosmological parameters using the baryon acoustic scale
• Re-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores
• 3D galaxy clustering with future wide-field surveys: Advantages of a spherical Fourier-Bessel analysis
• Cosmology with Hu-Sawicki gravity in Palatini Formalism
• Does $\Lambda$CDM really be in tension with the Hubble diagram data?
• Measuring Coherent Motions in the Universe
• Testing generalized logotropic models with cosmic growth
• Reconstruction of interaction rate in Holographic dark energy model with Hubble horizon as the infrared cut-off
• Constraining Cosmology with Big Data Statistics of Cosmological Graphs
• The Equation of State of Tracker Fields
• Testing flatness of the universe with probes of cosmic distances and growth
• Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
• Does fractal Universe describe a complete cosmic scenario?
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Physical constraints on interacting dark energy models
• Detecting the power spectrum turnover with HI intensity mapping
• Extensive search for bias in SNIa data
• Statefinder Analysis of Symmetric Teleparallel Cosmology
• Dark energy models toward observational tests and data
• Cyclic cosmology in modified gravity
• Uphill inflation
• CUBE: An Information-optimized parallel Cosmological $N$-body Algorithm
• Cosmology with nonminimal kinetic coupling and a Higgs-like potential
• Strong gravitational lensing constraints on holographic dark energy
• Study on the mapping of dark matter clustering from real space to redshift space
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• First Results from the La Silla-QUEST Supernova Survey and the Carnegie Supernova Project
• Cosmological Constant, Fine Structure Constant and Beyond
• Bouncing cosmological models in $f(R,L_m)$ gravity
• Observational test for $f(Q)$ gravity with weak gravitational lensing
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• Constraints on field flows of quintessence dark energy
• Peculiar Velocities into the Next Generation: Cosmological Parameters From Large Surveys without Bias from Nonlinear Structure
• Constraints on oscillating dark energy models
• Probing a Steep EoS for Dark Energy with latest observations
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Model-independent Estimations for the Cosmic Curvature from the Latest Strong Gravitational Lensing Systems
• Impact of the mean pressure profile of galaxy clusters on the cosmological constraints from the $Planck$ tSZ power spectrum
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Anisotropic stellar models admitting conformal motion
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Galaxy peculiar velocities and evolution-bias
• Cosmic slowing down of acceleration using $f_{gas}$
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Constraining the relative velocity effect using the Baryon Oscillation Spectroscopic Survey
• Optimizing baryon acoustic oscillation surveys II: curvature, redshifts, and external datasets
• Bayesian model comparison in cosmology with Population Monte Carlo
• Turning noise into signal: learning from the scatter in the Hubble diagram
• Bulk Flow and Shear Moments of the SFI++ Survey
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Cosmology with a successful Vainshtein screening in theories beyond Horndeski
• Cosmological dependence of the measurements of luminosity function, projected clustering and galaxy-galaxy lensing signal
• Modified Gravity: the CMB, Weak Lensing and General Parameterisations
• Quantum harmonic oscillator spectrum analyzers
• Accelerating Dark Energy Cosmological Model in Two Fluid with Hybrid Scale Factor
• Compact stellar models in modified gravity
• Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
• CMB and matter power spectra with non-linear dark-sector interactions
• Spherical collapse model and cluster number counts in power law $f(T)$ gravity
• A Specific Case of Generalized Einstein-aether Theories
• Cluster counts: calibration issue or new physics?
• Probing Dark Energy with Baryonic Acoustic Oscillations at High Redshifts
• Exact Cosmology in Myrzakulov Gravity
• Gravitationally Bound Bose Condensates with Rotation
• Probing modified gravity theories with the Sandage-Loeb test
• Isotropic compact stars in 4D Einstein-Gauss-Bonnet gravity
• Measuring the Density Fields around Bright Quasars at $z\sim 6$ with XQR-30 Spectra
• A one-parameter formula for testing slow-roll dark energy: observational prospects
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• K-mouflage effects on clusters of galaxies
• Reconstructing the baryon acoustic oscillations using biased tracers
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• AGN and QSOs in the eROSITA All-Sky Survey -- Part II: The large-scale structure
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Dynamical Stability in presence of non-minimal derivative dependent coupling of $k$-essence field with a relativistic fluid
• Dynamics and constraints of the Unified Dark Matter flat cosmologies
• Exploring hints for dark energy density evolution in light of recent data
• Is Dynamical Dark Energy Necessary? DESI BAO and Modified Recombination
• First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Effects of Chromatic Corrections to Supernova Photometry on Measurements of Cosmological Parameters
• Constraints on CDM cosmology from galaxy power spectrum, CMB and SNIa evolution
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• Parameterizing scalar-tensor theories for cosmological probes
• In Pursuit of LSST Science Requirements: A Comparison of Photometry Algorithms
• Searching for modified gravity with baryon oscillations: from SDSS to wide field multiobject spectroscopy (WFMOS)
• Delayed Recombination and Cosmic Parameters
• Graviton corrections to the Newtonian potential using invariant observables
• Bouncing cosmologies and stability analysis in symmetric teleparallel $f(Q)$ gravity
• Dark Energy, A Cosmological Constant, and Type Ia Supernovae
• Analytical and EZmock covariance validation for the DESI 2024 results
• Constraints on cosmic curvature with lensing time delays and gravitational waves
• Coupled vector dark energy
• A conventional approach to the dark-energy concept
• Late-time acceleration with a scalar field source: Observational constraints and statefinder diagnostics
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Nonparametric reconstruction of the Om diagnostic to test LCDM
• A new model for the full shape of the large-scale power spectrum
• Dark energy survivals in massive gravity after GW170817: SO(3) invariant
• Bouncing Universe and phantom crossing in Modified Gravity and its reconstruction
• New parametrization of the dark-energy equation of state with a single parameter
• Thermodynamics of phantom energy in the presence of a Reissner-Nordstrom black hole
• Dark Energy: The Shadowy Reflection of Dark Matter?
• Cosmological models with Yang-Mills fields
• Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature
• Polarization Alignment in JVAS/CLASS flat spectrum radio surveys
• A new extended quintessence
• A Robust Distance Measurement and Dark Energy Constraints from the Spherically-Averaged Correlation Function of Sloan Digital Sky Survey Luminous Red Galaxies
• Noether gauge symmetry for the Bianchi type I model in f(T) gravity
• Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
• Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies
• How well can (renormalized) perturbation theory predict dark matter clustering properties?
• Investigating Dark Energy Equation of State With High Redshift Hubble Diagram
• Effects of Linear Redshift Space Distortions and Perturbation Theory on BAOs: A 3D Spherical Analysis
• RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Anisotropic f(Q) gravity model with bulk viscosity
• Modeling cosmic acceleration with a generalized varying deceleration parameter
• Galaxy correlations and the BAO in a void universe: structure formation as a test of the Copernican Principle
• Constraints on accelerating universe using ESSENCE and Gold supernovae data combined with other cosmological probes
• Precision Cosmology: Successes and Challenges
• Ly alpha escape during cosmological hydrogen recombination: the 3d-1s and 3s-1s two-photon processes
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• Extending the halo mass resolution of $N$-body simulations
• Constraints on Steep Equation of State for the Dark Energy using BAO
• Kinematic Constraints on Spatial Curvature from Supernovae Ia and Cosmic Chronometers
• Effects of long-wavelength fluctuations in large galaxy surveys
• Modified recombination and the Hubble tension
• Cardassian Universe Constrained by Latest Observations
• Astrophysical Tests of Dark Matter Self-Interactions
• Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity
• Inhomogeneity-induced variance of cosmological parameters
• Density-dependent clustering: I. Pulling back the curtains on motions of the BAO peak
• A detection of baryon acoustic oscillations from the distribution of galaxy clusters
• Constraints on anisotropic properties of the universe in $f(Q,T)$ gravity theory
• Cosmic Velocity Field Reconstruction Using AI
• Testing CCC+TL Cosmology with Observed BAO Features
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• Gödel-type universes in f(T) gravity
• Barry and the BAO Model Comparison
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Probing bulk viscous matter-dominated models with Gamma-ray bursts
• On Reconstruction of Extended Teleparallel Gravity from the Cosmological Jerk Parameter
• A new $f(Q)$ cosmological model with $H(z)$ quadratic expansion
• The Unsettled Number: Hubble's Tension
• $\Lambda$CDM is alive and well
• Ghost condensates and pure kinetic $k$-essence condensates in presence of field-fluid non-minimal coupling in the dark sector
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• Key drivers of the preference for dynamic dark energy
• Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis
• 21st Century Statistical and Computational Challenges in Astrophysics
• Inner radius and energy conditions of dark matter halos surrounding Schwarzschild black holes
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Quantifying the accuracy of the Alcock-Paczynski scaling of baryon acoustic oscillation measurements
• Extended $\Lambda$CDM model
• The scale of cosmic homogeneity as a standard ruler
• PeV IceCube signals and Dark Matter relic abundance in modified cosmologies
• The Linear Point Standard Ruler for galaxy survey data: validation with mock catalogues
• Correlation function of the luminosity distances
• Reconstructing QCD ghost $f(R,T)$ models
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• Traversable holographic dark energy wormholes constrained by astronomical observations
• Large scale distribution of total mass versus luminous matter from Baryon Acoustic Oscillations: First search in the SDSS-III BOSS Data Release 10
• An Accurate Cluster Selection Function for the J-PAS Narrow-Band wide-field survey
• Group theoretical interpretation of the modified gravity in de Sitter space
• Observational constraints on a generalized equation of state model
• Exploring Universe acceleration through observational constraints via Hubble parameter reconstruction
• A comprehensive parametrization approach for the Hubble parameter in scalar field dark energy models
• Casimir Dark Energy, Stabilization of the Extra Dimensions and Gauss-Bonnet Term
• A dynamical system representation of generalized Rastall gravity
• Rip cosmologies, Wormhole Solutions and Big Trip in the $f(T,\mathcal{T})$ theory of gravity
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
• Is the Cosmic Transparency Spatially Homogeneous?
• Precise Measurement of the Radial Baryon Acoustic Oscillation Scales in Galaxy Redshift Surveys
• Observational constraints on the oscillating dark energy cosmologies
• A 3% Determination of $H_0$ at Intermediate Redshifts
• Vacuum energy as dark matter
• Non-Gaussian Error in Galaxy Survey (Part 1)
• Future dynamics in f(R) theories
• An accurate determination of the Hubble constant from Baryon Acoustic Oscillation datasets
• Constraint on Cosmological Model with Matter Creation Using Complementary Astronomical Observations
• Generation of large-scale magnetic fields from inflation in teleparallelism
• Testing the interaction model with cosmological data and gamma-ray bursts
• Cosmological constraints from Radial Baryon Acoustic Oscillation measurements and Observational Hubble data
• Consistency of LCDM with Geometric and Dynamical Probes
• A model-independent dark energy reconstruction scheme using the geometrical form of the luminosity-distance relation
• Revised WMAP constraints on neutrino masses and other extensions of the minimal $\Lambda$CDM model
• Dark energy interacting with dark matter and unparticle
• Geometrical Diagnostics for Generalized Chaplygin Gas
• Cosmology With Non-Minimally Coupled K-Field
• Disorder on the landscape
• Observational Bounds on Modified Gravity Models
• Tension between SN and BAO: current status and future forecasts
• Does DESI DR2 challenge $\Lambda$CDM paradigm ?
• The classical and quantum implications of the Raychaudhuri Equation in f(T)-gravity
• Spherical accretion by normal and phantom Einstein--Maxwell--dilaton black holes
• Inflection Points and the Power Spectrum
• The growth of matter perturbations in the f(T) gravity
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• Photometric Selection of Emission Line Galaxies, Clustering Analysis and a Search for the ISW effect
• Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Cosmological bounds on oscillating dark energy models
• The assembly bias of emission line galaxies
• Spatial Ricci scalar dark energy model
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Two scalar field cosmology from coupled one-field models
• Inflationary susceptibilities, duality and large-scale magnetic fields generation
• Evidence for baryon acoustic oscillations from galaxy-ellipticity correlations
• Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
• On measuring the absolute scale of baryon acoustic oscillations
• Does accelerating universe indicates Brans-Dicke theory
• Is the baryon acoustic oscillation peak a cosmological standard ruler?
• Magnetic field in holographic superconductor with dark matter sector
• The signature of the scattering between dark sectors in large scale cosmic microwave background anisotropies
• Study of Tsallis holographic dark energy model in the framework of Fractal cosmology
• A Faster Fourier Transform? Computing Small-Scale Power Spectra and Bispectra for Cosmological Simulations in $\mathcal{O}(N^2)$ Time
• Dynamical System Analysis for a phantom model
• A stable flat universe with variable Cosmological constant in f(R,T) Gravity
• Cosmological and Solar-System Tests of f(R) Modified Gravity
• The tight-coupling approximation for baryon acoustic oscillations
• Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae
• Consistency Test of Dark Energy Models
• The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps
• Gamma Rays Bursts: A Viable Cosmological Probe?
• Host Galaxy Spectra and Consequences for SN Typing From The SDSS SN Survey
• Cosmological Constant and Local Gravity
• The luminosity-redshift relation in brane-worlds: I. Analytical results
• Observational constraints on the generalized $\alpha$ attractor model
• Fitting oscillating string gas cosmology to supernova data
• Constraints on supernovae dimming from photon-pseudo scalar coupling
• Removing BAO-peak Shifts with Local Density Transforms
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• Cosmological evolution of equation of state for dark energy in G-essence models
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• Effective equation of state in modified gravity and observational constraints
• Detection and Fundamental Applications of Individual First Galaxies
• Weak Lensing of Baryon Acoustic Oscillations
• Elementary Theorems Regarding Blue Isocurvature Perturbations
• Weakly-Gravitating Objects in dynamical Chern-Simons gravity and Constraints with Gravity Probe B
• Improved calculation of relic gravitational waves
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• An 8-mm diameter Fiber Robot Positioner for Massive Spectroscopy Surveys
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Cosmic evolution in f(T) gravity theory
• Weak Lensing Effects on the Galaxy Three-Point Correlation Function
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Toward a direct measurement of the cosmic acceleration: roadmap and forecast on FAST
• The Kiselev solution in power-Maxwell electrodynamics
• A study of phantom scalar field cosmology using Lie and Noether symmetries
• Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
• Optimal Transport Reconstruction of Baryon Acoustic Oscillations
• Testing MOG, Non-Local Gravity and MOND with rotation curves of dwarf galaxies
• Extension and estimation of correlations in Cold Dark Matter models
• Spherical collapse model in agegraphic dark energy cosmologies
• Constraints on the DGP Universe Using Observational Hubble parameter
• Homogeneous Gödel-type solutions in hybrid metric-Palatini gravity
• Cosmological constraints on dynamical dark energy model in $F(Q)$ gravity
• A critical discussion on the $H_0$ tension
• Ultra-large-scale approximations and galaxy clustering: debiasing constraints on cosmological parameters
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• GCG Parametrization for Growth Function and Current Constraints
• Observational Constraints on Growth Index with Cosmography
• Validation of semi-analytical, semi-empirical covariance matrices for two-point correlation function for Early DESI data
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• Effects of biasing on the galaxy power spectrum at large scales
• Testing $f(R)$ Gravity With Scale Dependent Cosmic Void Velocity Profiles
• Observational Constraints on a Variable Dark Energy Model
• Constraints on the exponential $f(R)$ model from latest Hubble parameter measurements
• Mimetic Compact Stars
• Perturbations for transient acceleration
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• The Effect of Substructure on Mass Estimates of Galaxies
• Observational constraints on modified gravity models and the Poincaré dodecahedral topology
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) gravity
• Using newest VLT-KMOS HII Galaxies and other cosmic tracers to test the $\Lambda$CDM tension
• Clustering of SZ clusters on a past light-cone: acoustic oscillations and constraints on dark energy
• Inflation with F(T) Teleparallel Gravity
• Disformally Coupled Quintessence
• Testing dark matter warmness and quantity via the reduced relativistic gas model
• Cosmology in modified $f(\mathcal{G})$ gravity: a late time cosmic phenomena
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Anisotropic Baryon Acoustic Oscillations measurements in Fourier-space with optimal redshift weights
• Rotating a Curvaton Brane in a Warped Throat
• On the Emergence of Accelerating Cosmic Expansion in f(R) Theories of Gravity
• $\Lambda (t)$CDM Model as a Unified Origin of Holographic and Agegraphic Dark Energy Models
• Dilaton dominance in the early Universe dilutes Dark Matter relic abundances
• Cosmological constraints on polytropic gas model
• Dark Energy Survey Year 3 Results: Measurement of the Baryon Acoustic Oscillations with Three-dimensional Clustering
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• Probing the constancy of the speed of light with future galaxy survey: the case of SKA and Euclid
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Conservative Estimates of the Mass of the Neutrino from Cosmology
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Constraints on dark energy models from radial baryon acoustic scale measurements
• On the consistency of tachyon warm inflation with viscous pressure
• Cosmology-informed neural networks to solve the background dynamics of the Universe
• Implications of the lens redshift distribution of strong lensing systems: cosmological parameters and the global properties of early-type galaxies
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Relation between standard perturbation theory and regularized multi-point propagator method
• Cosmological constraints on the generalized holographic dark energy
• Using Lagrangian perturbation theory for precision cosmology
• A Method to Measure the Mass of Damped Ly-alpha Absorber Host Galaxies Using Fluctuations in 21cm Emission
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• Cosmological implications of Rastall-$f(R)$ theory
• Distance-redshift from an optical metric that includes absorption
• Two fluid anisotropic dark energy models in a scale invariant theory
• Reconstructing the properties of dark energy from recent observations
• Fermionic Isocurvature Perturbations
• SELCIE: A tool for investigating the chameleon field of arbitrary sources
• Gravitational collapse in the Schrödinger-Poisson system
• Raytracing simulations of coupled dark energy models
• Luminous Red Galaxies: Selection and classification by combining optical and infrared photometry
• A Hybrid Fast Multipole Method for Cosmological N-body Simulations
• Accurate Baryon Acoustic Oscillations reconstruction via semi-discrete optimal transport
• Constraints from the CMB temperature and other common observational data-sets on variable dark energy density models
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Modelling non-linear evolution using Lagrangian Perturbation Theory (LPT) re-expansions
• Extragalactic Point Source Search in WMAP 61 and 94 GHz Data
• Cosmological Parameter Estimation from SN Ia data: a Model-Independent Approach
• The relation between cosmological redshift and scale factor for photons
• Cosmological perturbations during the Bose-Einstein condensation of dark matter
• Is the $W$-boson mass enhanced by the axion-like particle, dark photon, or chameleon dark energy?
• Observational Constraints on Modified Chaplygin Gas in Horava-Lifshitz Gravity
• QCD modified ghost scalar field dark energy models
• Deviation from $\Lambda$CDM: Pressure Parametrization
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Discovery of a Supercluster at $z\sim$0.91 and Testing the $\Lambda$CDM Cosmological Model
• Cosmological constraints on the new holographic dark energy model with action principle
• Accuracy of analytical models of the large-scale matter distribution
• Reconstructing Cosmological Matter Perturbations using Standard Candles and Rulers
• Velocity reconstruction in the era of DESI and Rubin (part I): Exploring spectroscopic, photometric & hybrid samples
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
• Detection of Lyβauto-correlations and Lyα-Lyβcross-correlations in BOSS Data Release 9
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Cosmological implications of conformal field theory
• Constraints on dark energy models from the Horndeski theory
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• Breaking through the high redshift bottleneck of Observational Hubble parameter Data: The Sandage-Loeb signal Scheme
• Observational constraints on unified dark matter including Hubble parameter data
• Type Ia supernova parameter estimation: a comparison of two approaches using current datasets
• Are the 2dFGRS superstructures a problem for hierarchical models?
• Quintessence-like features in the late-time cosmological evolution of $f(Q)$ symmetric teleparallel gravity
• Differentiating dark interactions with perturbation
• A new parametrization of dark energy equation of state leading to double exponential potential
• Constraining Thawing Quintessence
• Growth of perturbations in dark energy parametrization scenarios
• Covariance of the redshift-space matter power spectrum after reconstruction
• Wavelet analysis of baryon acoustic structures in the galaxy distribution
• Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
• Prospects and pitfalls of gravitational lensing in large supernova surveys
• Probing Dark Energy Inhomogeneities with Supernovae
• From model dynamics to oscillating dark energy parameterisation
• Exploiting scale dependence in cosmological averaging
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Effect of model-dependent covariance matrix for studying Baryon Acoustic Oscillations
• Constraining dark energy via baryon acoustic oscillations in the (an)isotropic light-cone power spectrum
• The redshift-space galaxy two-point correlation function and baryon acoustic oscillations
• On the Gravitational Energy-Momentum Vector in f(T) Theories
• Future constraints on the Hu-Sawicki modified gravity scenario
• On FRW Model in Conformal Teleparallel Gravity
• Analytic Solutions and Observational support: A study of $f(R,T)$ gravity with $f(R,T)=R+h(T)$
• Equation of State of Neutron Stars with Junction Conditions in the Starobinsky Model
• Application of the iterative reconstruction to simulated galaxy fields
• Direct cosmological inference from three-dimensional correlations of the Lyman-$\alpha$ forest
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Structure formation in dark energy cosmologies described by PADE parameterization
• Cosmological neutrino mass limit and the dynamics of dark energy
• Determining $H_0$ with the latest HII galaxy measurements
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• Vacuum Solution of a Linear Red-Shift Based Correction in $f(R)$ Gravity
• Forward Modeling of Spectroscopic Galaxy Surveys: Application to SDSS
• Late-time acceleration in Higher Dimensional Cosmology
• Limitations of Bayesian Evidence Applied to Cosmology
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Thawing Versus. Tracker Behaviour: Observational Evidence
• Cosmological constraint on Brans-Dicke Model
• Improved cosmological constraints on the curvature and equation of state of dark energy
• Vacuum stability and scalar masses in the superweak extension of the standard model
• Lensing as a Probe of Early Universe: from CMB to Galaxies
• Volume Statistics as a Probe of Large-Scale Structure
• Probing large scale homogeneity and periodicity in the LRG distribution using Shannon entropy
• Noether symmetry in a nonlocal f(T) Gravity
• Full forward model of galaxy clustering statistics with AbacusSummit lightcones
• Intermediate homogenization of the Universe and the problem of gravitational entropy
• Thermodynamical Behaviour of Inhomogeneous Universe with Varying $\Lambda$ in Presence of Electromagnetic Field
• The number of dwarf satellites of disk galaxies versus their bulge mass in the standard model of cosmology
• Dynamics and constraints of the dissipative Liouville cosmology
• A critical assessment of some inhomogeneous pressure Stephani models
• Redshift-space correlation functions in large galaxy cluster surveys
• Testing averaged cosmology with type Ia supernovae and BAO data
• Holographic dark energy described at the Hubble length
• Eulerian and Lagrangian propagators for the adhesion model (Burgers dynamics)
• Dynamics and Constraints of the Massive Gravitons Dark Matter Flat Cosmologies
• Sterile neutrino dark matter in a U(1) extension of the standard model
• Detecting Baryon Acoustic Oscillations
• Influences of Dark Energy and dark matter on Gravitational Time Advancement
• Modified cosmology in $f(Q,L_m)$ gravity
• Observational constrains on the DGP brane-world model with a Gauss-Bonnet term in the bulk
• A new class of holographic dark energy models in LRS Bianchi Type-I
• Baryon acoustic oscillation methods for generic curvature: Application to the SDSS-III Baryon Oscillation Spectroscopic Survey
• Rosella: A mock catalogue from the P-Millennium simulation
• Statistical recovery of the BAO scale from multipoles of the beam-convolved 21cm correlation function
• Clustering with general photo-$z$ uncertainties: Application to Baryon Acoustic Oscillations
• Cosmological Constraints on Ghost Dark Energy in the Brans-Dicke Theory by Using MCMC Approach
• Reducing the Variance of Redshift Space Distortion Measurements from Mock Galaxy Catalogues with Different Lines of Sight
• Inhomogeneous Bulk Viscous Fluid Universe with Electromagnetic Field and Variable $\Lambda$-Term
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Viscous Self Interacting Dark Matter Cosmology For Small Redshift
• Quantum corrections for spinning particles in de Sitter
• The Nature of the Faint Low-Frequency Radio Source Population
• Testing Dark Energy with the Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics
• Testing and selection of cosmological models with $(1+z{)}^6$ corrections
• Testing Emergent Gravity with Isolated Dwarf Galaxies
• De-Sitter nonlinear sigma model and accelerating universe
• Testing the cosmic conservation of photon number with type Ia supernovae and ages of old objects
• Delayed Recombination and Standard Rulers
• Constraints on sigma_8 from galaxy clustering in N-body simulations and semi-analytic models
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• Thermodynamical properties of dark energy with the equation of state
• Recovering a redshift-extended VSL signal from galaxy surveys
• Charged Anti-de Sitter BTZ black holes in Maxwell-$f(T)$ gravity
• Is Thick Brane Model Consistent with the Recent Observations?
• Observational tests of a two parameter power-law class modified gravity in Palatini formalism
• A new parametrization for dark energy density and future deceleration
• Chebyshev cosmography in the framework of extended symmetric teleparallel theory
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Cosmological reconstruction and {\it Om} diagnostic analysis of Einstein-Aether Theory
• Five-dimensional metric $f(R)$ gravity and the accelerated universe
• Constraints on Cosmological Models from Quasars Calibrated with Type Ia Supernova by a Gaussian Process
• Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
• Cosmological Constraints on the DGP braneworld model with Gamma-ray bursts
• Sudden Future Singularity models as an alternative to Dark Energy?
• Dependence on supernovae light-curve processing in void models
• Bayesian analysis of CCDM Models
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Observational constraints to a phenomenological $f\left(R,\nabla R\right)$-model
• New parameterization for unified dark matter and dark energy
• Cosmological Constraints from the Anisotropic Clustering Analysis using BOSS DR9
• Spectro-Imaging Forward Model of Red and Blue Galaxies
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Measuring BAO and non-Gaussianity via QSO clustering
• Cosmological aspects of a unified dark energy and dust dark matter model
• Distance Probes of Dark Energy
• An updated analysis of two classes of f(R) theories of gravity
• Iterative removal of redshift space distortions from galaxy clustering
• Holographic Dark Energy Characterized by the Total Comoving Horizon and Insights to Cosmological Constant and Coincidence Problem
• Asymptotic Analysis of the Boltzmann Equation for Dark Matter Relics
• Multiband Probabilistic Cataloging: A Joint Fitting Approach to Point Source Detection and Deblending
• The Reactor Anomaly after Daya Bay and RENO
• FLRW accelerating universe with interactive dark energy
• Cosmological Information Contents on the Light-Cone
• Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations
• Do recent observations favor a cosmological event horizon: A thermodynamical prescription?
• Acceleration of the Universe driven by the Casimir force
• Coupled quintessence with a possible transient accelerating phase
• The impact and mitigation of broad absorption line quasars in Lyman$-\alpha$ forest correlations
• Satellites in the field and lens galaxies: SDSS/COSMOS vs. SLACS/CLASS
• Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• An optimal basis system for cosmology: data analysis and new parameterisation
• Signatures of the Baryon Acoustic Oscillations on 21cm Emission Background
• Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
• Line confusion in spectroscopic surveys and its possible effects: Shifts in Baryon Acoustic Oscillations position
• MEDUSA: Minkowski functionals estimated from Delaunay tessellations of the three-dimensional large-scale structure
• Measuring Baryon Acoustic Oscillations with Millions of Supernovae
• Is there a standard measuring rod in the Universe?
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Noether Symmetries of a Modified Model in Teleparallel Gravity and a New Approach for Exact Solutions
• Dark Matter Studies Entrain Nuclear Physics
• Understanding the Reconstruction of the Biased Tracer
• The Imprint of Cosmic Reionization on Galaxy Clustering
• GRBs and fundamental physics
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• The study of the angular and spatial distribution of radio selected AGNs and star-forming galaxies in the ELAIS N1 field
• Cosmological constraints from low-redshift data
• Hybrid dark energy
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• Observational constraints on a cosmological model with Lagrange multipliers
• Model-independent estimation of the cosmography parameters using cosmic chronometers
• Parametrizations of Dark Energy Models in the Background of General Non-canonical Scalar Field in $D$-dimensional Fractal Universe
• Cosmological homogeneity scale estimates are dressed
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• An analytic approach to baryon acoustic oscillations
• Probing violation of the Copernican principle via the integrated Sachs-Wolfe effect
• Cross-correlation between the cosmic microwave and infrared backgrounds for integrated Sachs-Wolfe detection
• Growth of non-linear structures and spherical collapse in the Galileon Ghost Condensate model
• Statistical properties of SZ and X-ray cluster detections
• An FLRW interacting dark energy model of the Universe
• Bayesian methods for fitting Baryon Acoustic Oscillations in the Lyman-$\alpha$ forest
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• A single parameterization for dark energy and modified gravity models
• Periodic Cosmological Evolutions of Equation of State for Dark Energy
• What kind of science is cosmology?
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• Warm Inflation in $f(R,T)$ gravity
• Thawing quintessence from the inflationary epoch to today
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Surveying the dark side
• Parameter Estimation with BEAMS in the presence of biases and correlations
• Constraints on Dark Energy Models Using Late Universe Probes
• Phenomenology of BAO evolution from Lagrangian to Eulerian Space
• Dark energy, integrated Sachs-Wolfe effect and large-scale magnetic fields
• Cosmological constraints on time-varying cosmological terms: A study of FLRW universe models with $\Lambda (t)$CDM cosmology
• Geometric and dynamic distortions in anisotropic galaxy clustering
• Odd-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories
• Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen
• Supernova, baryon acoustic oscillations, and CMB surface distance constraints on f(G) higher order gravity models
• Correlations between 21 cm Radiation and the CMB from Active Sources
• Constraints on $\Lambda (t)$CDM models as holographic and agegraphic dark energy with the observational Hubble parameter data
• Extracting Spectral Index of Intergalactic Magnetic Field from Radio Polarizations
• The Hubble constant and dark energy from cosmological distance measures
• Observational constraints on finite scale factor singularities
• Shell-like structures in our cosmic neighbourhood
• 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
• Exploring cosmological evolution and constraints in $f(T)$ teleparallel gravity
• Current lookback time-redshift bounds on dark energy
• Supernovae as probes of cosmic parameters: estimating the bias from under-dense lines of sight
• The dark side of curvature
• Is a Bose-Einstein Condensate a good candidate for Dark Matter? A test with Galaxy Rotation Curves
• Configurational Entropy and braneworlds in f(T,B) gravity
• Forecast and analysis of the cosmological redshift drift
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• ISW-Galaxy Cross Correlation:A probe of Dark Energy clustering and distribution of Dark Matter tracers
• Cosmological Parameter Estimation Using Current and Future Observations of Strong Gravitational Lensing
• Performance study of Lagrangian methods: reconstruction of large scale peculiar velocities and baryonic acoustic oscillations
• Does Planck mass run on the cosmological horizon scale?
• Interacting holographic Ricci dark energy as running vacuum
• Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments
• Dynamics and statefinder analysis of a class of sign-changeable interacting dark energy scenarios
• FRW dark energy cosmological model with hybrid expansion law
• Planting a Lyman alpha forest on AbacusSummit
• Can brane dark energy model be probed observationally by distant supernovae?
• A Coarse-Grained Field Theory for Density Fluctuations and Correlation Functions of Galactic Objects
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• Whether Lyra's Manifold Itself is a Hidden Source of Dark Energy
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• Systematics in the Gamma Ray Bursts Hubble diagram
• Baryonic matter perturbations in decaying vacuum cosmology
• Cosmology With A Dark Refraction Index
• Transient acceleration in $f(T)$ gravity
• High Redshift Investigation On The Dark Energy Equation of State
• Using variability and VLBI to measure cosmological distances
• Cosmic Acceleration and Anisotropic models with Magnetic field
• Effects of NII and H$\alpha$ Line Blending on the WFIRST Galaxy Redshift Survey
• Clustering in the Simulated H$\alpha$ Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
• HI intensity mapping with the MIGHTEE survey: power spectrum estimates
• The Phase of the BAO on Observable Scales
• Analyzing Baryon Acoustic Oscillations in Sparse Spectroscopic Samples via Cross-Correlation with Dense Photometry
• On existence of a possible Lorentz invariant modified gravity in Weitzenböck spacetime
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Large Blue Spectral Isocurvature Spectral Index Signals Time-Dependent Mass
• Bulk viscous cosmological model in $f(T,\mathcal{T})$ modified gravity
• Distinguishing f(R) theories from general relativity by gravitational lensing effect
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Quantifying effects of inhomogeneities and curvature on gravitational wave standard siren measurements of $H(z)$
• Optimising Spectroscopic and Photometric Galaxy Surveys: Same-sky Benefits for Dark Energy and Modified Gravity
• Complete density perturbations in the Jordan-Fierz-Brans-Dicke theory
• Cosmic Variation of Proton to Electron Mass Ratio with an interacting Higgs Scalar Field
• Bounds from ISW-galaxy cross-correlations on generalized covariant Galileon models
• On The Temporal Evolution of Particle Production in $f(T)$ Gravity
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Assessment of the Systematic Uncertainties in the Cosmological Analysis of the SDSS Supernovae Photometric Sample
• Interacting generalized ghost dark energy in non-flat universe
• Constraints on a special running vacuum model
• Deviation From ΛCDM With Cosmic Strings Networks
• Constraints on the Hubble Parameter from galaxy clusters and the Validity of the Cosmic Distance Duality Relation
• How accurately can we measure the baryon acoustic oscillation feature?
• Nonlinear $E$-mode clustering in Lagrangian space
• Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
• Parametrizing the transition to the phantom epoch with Supernovae Ia and Standard Rulers
• From inflation to late time acceleration with a decaying vacuum coupled to radiation or matter
• A new approach to cosmological perturbations in f(R) models
• Light mass galileon and late time acceleration of the Universe
• Anisotropic Extinction Distortion of the Galaxy Correlation Function
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• Standardizing the Gamma-ray burst as a standard candle and applying to the cosmological probes: constraints on the two-component dark energy model
• The $k$-essence scalar field in the context of Supernova Ia Observations
• Information Content in the Angular Power Spectrum of Weak Lensing: Wavelet Method
• Parametrization for the Scale Dependent Growth in Modified Gravity
• Dynamics of viable $f(R)$ dark energy models in the presence of Curvature-Matter interactions
• Observational tests for oscillating expansion rate of the Universe
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Hydrodynamic Vacuum Sources of Dark Matter Self-Generation in Accelerated Universe without Big Bang
• Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
• Effects of structure formation on the expansion rate of the Universe: An estimate from numerical simulations
• Dynamical system analysis of LRS-BI Universe with f(Q) gravity theory
• Observational constrained Weyl type $f(Q,T)$ gravity cosmological model and the dynamical system analysis
• Towards observational constraints on negative (1+z)^4 type contribution in the Friedmann equation
• Wide Field Surveys and Astronomical Discovery Space
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• Constraints on the Phase Plane of the Dark Energy Equation of State
• Prospects in Constraining the Dark Energy Potential
• Cosmology in Brans-Dicke-de Rham-Gabadadze-Tolley massive gravity
• Simplified Quartessence Cosmology
• Reconstructing the interaction between the dark matter and holographic dark energy
• Matching the mass function of Milky Way satellites in competing dark matter models
• Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
• Probing the cosmic acceleration history and the properties of dark energy from the ESSENCE supernova data with a model independent method
• Cosmological Scaling Solutions with Tachyon:Modified Gravity Model
• Squared torsion $f(T,\mathcal{T})$ gravity and its cosmological implications
• Relaxing the Cosmological Constraints on Unparticle Dark Component
• Reconstructing the extended structure of multiple sources strongly lensed by the ultra-massive elliptical galaxy SDSS J0100+1818
• Probing for variation of neutrino mass with current observations
• Trans-Planckian enhancements of the primordial non-Gaussianities
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Observational constraints on the braneworld model with brane-bulk energy exchange
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• Relativistic Effects on Galaxy Redshift Samples due to Target Selection
• Revisiting cosmic acceleration with DESI BAO
• Cosmology With Axionic-quintessence Coupled with Dark Matter
• Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data
• Constraints on the Transition Redshift using Hubble Phase Space Portrait
• Astrophysics in 2006
• Alternative High-z Cosmic Tracers and the Dark Energy Equation of State
• Predictions for BAO distance estimates from the cross-correlation of the Lyman-alpha forest and redshifted 21-cm emission
• Future evolution in a backreaction model and the analogous scalar field cosmology
• Cosmological Constraint and Analysis on Holographic Dark Energy Model Characterized by the Conformal-age-like Length
• Observational Constraints on Axions as Quintessence in String Theory
• Detecting baryon acoustic oscillations by 3d weak lensing
• Hubble-rate-dependent Dark Energy in Brans-Dicke Cosmology
• Combining Optical and X-ray Observations of Galaxy Clusters to Constrain Cosmological Parameters
• Designing Future Dark Energy Space Missions: II. Photometric Redshift of Space Weak Lensing Optimized Survey
• Baryogenesis through Asymmetric Hawking Radiation from Primordial Black Holes as Dark Matter
• Spatial and Kinematic Clustering of Stars in the Galactic Disk
• Cosmological constraints on Agegraphic dark energy in DGP braneworld gravity
• Testing the consistency between cosmological measurements of distance and age
• DBI Galileon and Late time acceleration of the universe
• Figure of Merit and Different Combinations of Observational Data Sets
• Fast, large volume, GPU enabled simulations for the Ly-alpha forest: power spectrum forecasts for baryon acoustic oscillation experiments
• Can the Universe decelerate in the future?
• Decaying dark energy in light of the latest cosmological dataset
• Probing signatures of bounce inflation with current observations
• Quantum cosmology for non-minimally coupled scalar field in FLRW space-time: A symmetry analysis
• Probing Weyl-type $f(Q,T)$ gravity: Cosmological implications and constraints
• Investigating the effect of cosmic opacity on standard candles
• Testing Standard Cosmology with Large Scale Structure
• Implications of JLA data for $k-$essence model of dark energy with given equation of state
• Non-existence of Extended Holographic Dark Energy with Hubble Horizon
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• Baryon Acoustic Oscillations in the Lyman Alpha Forest
• Slow-roll inflation in $f(T,\mathcal{T})$ modified gravity
• Bulk viscous matter in $f(T)$ gravity: A path to cosmic acceleration
• Uncertainty in 2-point correlation function estimators and BAO detection in SDSS DR7
• Halting eternal acceleration with an effective negative cosmological constant
• Probing Dark Sectors with Neutron Stars
• Cosmic acceleration and phantom crossing in $f(T)$-gravity
• Bouncing universe of entropy-corrected Friedmann equations
• Deep uGMRT observations of the ELAIS-North 1 field: statistical properties of radio--infrared relations up to $z\sim$2
• Cosmic jerk parameter in symmetric teleparallel cosmology
• Observationally constrained accelerating cosmological model with higher power of non-metricity and squared trace
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• Closed inflationary universe with tachyonic field
• Dark energy and dark matter perturbations in singular universes
• How much cosmological information can be measured?
• Signature flips in time-varying $\Lambda (t)$ cosmological models with observational data
• Measuring galaxy [OII] emission line doublet with future ground-based wide-field spectroscopic surveys
• The interacting generalized Ricci dark energy model in non-flat universe
• Cosmological tests of gravity with latest observations
• Cosmological constraints on unparticle dark matter
• The redshifted HI 21 cm signal from the post-reionization epoch: Cross-correlations with other cosmological probes
• Reconstructing $f(T)$ modified gravity from ECHDE and ECNADE models
• Holographic Λ(t)CDM model in a non-flat universe
• Dilaton dominance relaxes LHC and cosmological constraints in supersymmetric models
• Stability, dark energy parameterization and swampland aspect of Bianchi Type-$V{I}_h$ cosmological models with f(R, T)-gravity
• Gas mass fraction from XMM-Newton and Chandra high redshift clusters and its use as a cosmological test
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Cosmological forecasts from photometric measurements of the angular correlation function
• Distance-duality in theories with a nonminimal coupling to gravity
• Robustness of $H_0$ determination at intermediate redshifts
• Bulk viscous fluid in symmetric teleparallel cosmology: theory versus experiment
• Reference level of the vacuum energy density of the Universe and astrophysical data
• Gluon condensate, modified gravity, and the accelerating Universe
• Holographic Ricci dark energy as running vacuum
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Fractal Bubble Cosmology: A concordant cosmological model?
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Functors of actions
• No evidence for EDE from Planck data in extended scenarios
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• The Square Kilometer Array: cosmology, pulsars and other physics with the SKA
• Viscous fluid cosmology in symmetric teleparallel gravity
• Observational Constraints on Varying Alpha in $\Lambda (\alpha )$CDM Cosmology
• Locating the Baryon Acoustic Peak
• Fitting cosmological data to the function $q(z)$ from GR Theory: Modified Chaplygin Gas
• Constraining Perturbative Early Dark Energy with Current Observations
• Interacting Models of Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity
• Alignment in the orientation of LOFAR radio sources
• Peaks in the CMBR power spectrum. I. Mathematical analysis of the associated real space features
• Stability analysis in Modified Non-Local Gravity
• Cosmological constraints on dark energy
• Constraints on Cardassian universe from Gamma ray bursts
• Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
• Physical condition for the slowing down of cosmic acceleration
• Interacting Agegraphic Dark Energy Model in DGP Braneworld Cosmology: Dynamical System Approach
• Thermodynamics of Black holes With Higher Order Corrected Entropy
• Measuring the BAO peak position with different galaxy selections
• The interacting vacuum and tensions: a comparison of theoretical models
• Euclid preparation. XXVII. A UV-NIR spectral atlas of compact planetary nebulae for wavelength calibration
• Current cosmological constraints on the curvature, dark energy and modified gravity
• Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
• Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
• Testing feasibility of scalar-tensor gravity by scale dependent mass and coupling to matter
• Viscous Dark Energy and Phantom Field in An Anisotropic Universe
• Magnetic Field of a Compact Spherical Star under f(R,T) Gravity
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• The parameter space of Cubic Galileon models for cosmic acceleration
• Shadows of black holes at cosmological distances in the co-varying physical couplings framework
• Dark Energy and Modified Scale Covariant Theory of Gravitation
• Emergence of space and expansion of universe
• Parametrizing growth in dark energy and modified gravity models
• Challenges in Constraining Gravity with Cosmic Voids
• Discriminating Electroweak-ino Parameter Ordering at the LHC and Its Impact on LFV Studies
• An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
• Phantom dark energy with tachyonic instability: metric perturbations
• An extension of the cosmological standard model with a bounded Hubble expansion rate
• Skewness as a probe of Baryon Acoustic Oscillations
• Integrated perturbation theory for cosmological tensor fields. II. Loop corrections
• Galaxy-galaxy lensing data: $f(T)$ gravity challenges General Relativity
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• Photo-z Quality Cuts and their Effect on the Measured Galaxy Clustering
• Simultaneous effect of Modified Gravity and Primordial Non-Gaussianity in Large Scale Structure Observations
• The cluster-galaxy cross-spectrum: an additional probe of cosmological and halo parameters
• Signatures of the Baryon Acoustic Oscillations on the Convergence Power Spectrum of Weak lensing by Large Scale Structure
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• Absence of solid angle deficit singularities in beyond-generalized Proca theories
• Upper Limit on Dimming of Cosmological Sources by Intergalactic Grey Dust from the Soft X-ray Background
• Black hole entropy arising from massless scalar field with Lorentz violation induced by the coupling to Einstein tensor
• Age problem in holographic dark energy
• Reconstructing the Hubble diagram of gamma-ray bursts using deep learning
• New initial condition of the new agegraphic dark energy model
• Interacting warm dark matter
• Improved parametrization of the growth index for dark energy and DGP models
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Dark Energy as a Critical Period in Binary Motion: Bounds from Multi-scale Binaries
• Effects on the two-point correlation function from the coupling of quintessence to dark matter
• The universe is accelerating. Do we need a new mass scale?
• Effect of low anisotropy on cosmological models by using supernova data
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Observational data fitting to constrain Variable Modified Chaplygin Gas in the background of Horava-Lifshitz Gravity
• Non-Gaussian error bars in galaxy surveys -- II
• Large scale distribution of mass versus light from Baryon Acoustic Oscillations: Measurement in the final SDSS-III BOSS Data Release 12
• Model Selection with Baryonic Acoustic Oscillations in the Lyman-alpha Forest
• Reconstruction of small-scale galaxy cluster substructure with lensing flexion
• Constraining Modified Chaplygin gas parameters
• Study of Some Parameters of Modified Chaplygin Gas in Galileon Gravity Theory from Observational Perspective
• Assessing the foundation and applicability of some dark energy fluid models in the Dirac-Born-Infeld framework
• Turnaround density as a probe of the cosmological constant
• Barrow holographic dark energy models in $f\left(Q\right)$ symmetric teleparallel gravity with Lambert function distribution
• Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
• Resolving FLRW cosmology through effective equations of state in $f(T)$ gravity
• Observational Constraints on Visser's Cosmological Model
• Cosmology from String T-duality and zero-point length
• Cosmological analytic solutions with reduced relativistic gas
• Square-Root parametrization of dark energy in $f(Q)$ cosmology
• A study on the Clustering Properties of Radio-Selected sources in the Lockman Hole Region at 325 MHz
• Knot Universes in Bianchi Type I Cosmology
• Late transient acceleration of the universe in string theory on $S^1/Z_2$
• What have we learned from observational cosmology ?
• Cosmological perturbation and matter power spectrum in bimetric massive gravity
• Challenges in Cosmology from the Big Bang to Dark Energy, Dark Matter and Galaxy Formation
• Determining $H_0$ using a model-independent method
• Cosmological solutions in spatially curved universes with adiabatic particle production
• Cosmology with cosmic web environments II. Redshift-space auto and cross power spectra
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• Cosmological implications of different baryon acoustic oscillation data
• Interacting parametrized post-Friedmann method
• Dynamical analysis of coupled curvature-matter scenario in viable $f(R)$ dark energy models at de Sitter phase
• Exploring Alternative Cosmologies with the LSST: Simulated Forecasts and Current Observational Constraints
• Observational Constraints of Homogeneous Higher Dimensional Cosmology with Modified Chaplygin Gas
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• Bootstrapping from inflationary magnetogenesis to CMB initial conditions
• Angular Correlation Function Estimators Accounting for Contamination from Probabilistic Distance Measurements
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• Energy conditions in $f(Q,L_m)$ gravity
• Clustering GCG: a viable option for unified dark matter-dark energy?
• Coupled Quintessence scalar field model in light of observational datasets
• Trans-Planckian signals from the breaking of local Lorentz invariance
• The viable f(G) gravity models via reconstruction from the observations
• Non-singular inflation with vacuum decay
• The Alcock Paczynski test with 21cm intensity field
• Fundamental Physics and Cosmology with TianQin
• Evolution mapping II: describing statistics of the non-linear cosmic velocity field
• Dynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space Analysis
• Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations
• What do we learn from CMB observations
• Model independent measurement of the growth rate from the consistency relations of the LSS
• Newman-Penrose formalism and exact vacuum solutions to conformal Weyl gravity
• Cosmology from one galaxy in a void?
• Scalar - Tensor gravity with scalar -matter direct coupling and its cosmological probe
• Posing Constraints on the Free Parameters of a New Model of Dark Energy EoS : Responses Through Cosmological Behaviours
• Reconstructing FHDE with Scalar and Gauge Fields
• On Dark Matter Explanations of the Gamma-Ray Excesses from the Galactic Center and M31
• Modelling Time-varying Dark Energy with Constraints from Latest Observations
• Constraining Temporal Oscillations of Cosmological Parameters Using Type Ia Supernovae
• Cosmology of the interacting Tsallis holographic dark energy in $f(R,T)$ gravity framework
• Latest Observational Constraints on Cardassian Models
• Constraints on Dark Energy Models from Weak Gravity Conjecture
• Study on the mapping of halo clustering from real space to redshift space
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• Statistical and Observation Comparison of Weyl-Type $f(Q,T)$ Models with the $\Lambda$CDM Paradigm
• Differentiating small-scale subhalo distributions in CDM and WDM models using persistent homology
• Temperature Structure and Mass-Temperature Scatter In Galaxy Clusters
• Re-examining the role of curvature in the slowing down acceleration scenario
• Dark Energy, Dark Matter and Gravity
• The Cosmology of Asymmetric Brane Modified Gravity
• Unveiling the Universe with Emerging Cosmological Probes
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Impacts on Cosmological Constraints from Degeneracies
• Non-minimally coupled scalar field in Kantowski--Sachs model and symmetry analysis
• Tachyon field inspired dark energy and supernovae constraints
• Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
• Forecasting cosmological constraints from age of high-z galaxies
• Cosmological perturbations in the $\Lambda$CDM-like limit of a polytropic dark matter model
• Dark Matter Annihilation Feedback in cosmological simulations I: Code convergence and idealised halos
• Smoothing the redshift distributions of random samples for the baryon acoustic oscillations : applications to the SDSS-III BOSS DR12 and QPM mock samples
• New constraints on H_0 and Omega_M from SZE/X-RAY data and Baryon Acoustic Oscillations
• Characteristic Functions for Cosmological Cross-Correlations
• Structure formation in clustering DBI dark energy model with constant sound speed
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• Constraining Parameters for the Accelerating Universe in $f(R,{\mathcal{L}}_m)$ Gravity
• Observational constraint on dynamical evolution of dark energy
• Tidal Dwarf Galaxies at Intermediate Redshifts
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• Testing the local-void alternative to dark energy using galaxy pairs
• A possible role for the merger of clusters/voids in the cosmological expansion
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Super-horizon cosmic string correlations
• Cosmological implications of the KATRIN experiment
• Constraining Parameters of Generalized Cosmic Chaplygin Gas in Loop Quantum Cosmology
• Expansion and Growth of Structure Observables in a Macroscopic Gravity Averaged Universe
• Quasi-periodical features in the distribution of Luminous Red Galaxies
• The catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST
• Hubble flow variations as a test for inhomogeneous cosmology
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints
• The phase transition of Rastall AdS black hole with cloud of strings and quintessence
• Constraints on the Combined Models with $R^{2-q}$ Inflation and Viable $f(R)$ Dark Energy
• What can be learned about dark energy evolution?
• The mass-size relation of LRGs from BOSS and DECaLS
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• cp3-bench: A tool for benchmarking symbolic regression algorithms tested with cosmology
• Validation of Emission-Line Galaxies Target Selection Algorithms for the Dark Energy Spectroscopic Instrument Using the MMT Binospec
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Analysis cosmological tachyon and fermion model and observation data constraints
• Two-point statistics without bins: A continuous-function generalization of the correlation function estimator for large-scale structure
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• Anti-screening of the Galileon force around a disk center hole
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• Litmus tests of the flat $\Lambda$CDM model and model-independent measurement of $H_0{r}_{\mathrm{d}}$ with LSST and DESI
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Observational Constraints of Modified Chaplygin Gas in RS II Brane
• CCDM Model with Spatial Curvature and The Breaking of "Dark Degeneracy"
• Scalar field description of a parametric model of dark energy
• Improved two-point correlation function estimates using glass-like distributions as a reference sample
• Does spatial flatness forbid the turnaround epoch of collapsing structures?
• Homogeneous and Isotropic space-time, Modified torsion field and Complete cosmic scenario
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• "Expansion" around the vacuum: how far can we go from Lambda?
• A More Accurate and Competitive Estimative of $H_0$ in Intermediate Redshifts
• Conditions for spontaneous homogenization of the Universe
• Constraining dark energy using observational growth rate data
• The unphysical character of dark energy fluids
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• Reconstruction of $f(R)$ lagrangian from a massive scalar field
• Gaussian Mixture Models for Blended Photometric Redshifts
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Fourier space analysis
• Observational constraints on G-corrected holographic dark energy using a Markov chain Monte Carlo method
• Observational constraints on Tsallis holographic dark energy with Ricci horizon cutoff
• Dynamical Casimir Effect with Semi-Transparent Mirrors, and Cosmology
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• Constraining some $r^{-n}$ extra-potentials in modified gravity models with LAGEOS-type laser-ranged geodetic satellites
• Neutral compact spherically symmetric stars in teleparallel gravity
• Chi-square versus median statistics in SNIa data analysis
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Future cosmological evolution in $f(R)$ gravity using two equations of state parameters
• Observational Constraints on the Model Parameters of a Class of Emergent Universe
• The Two-Point Correlation Function of Gamma-ray Bursts
• Addressing the $r_d$ Tension using Late-Time Observational Measurements in a Novel deceleration Parametrization
• On 1 + 3 covariant perturbations of the quasi-Newtonian space-time in modified Gauss-Bonnet gravity
• Investigating the Possibility of a Turning Point in the Dark Energy Equation of State
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• Isochronous Cosmologies
• Infrared (in)sensitivity of relativistic effects in cosmological observable statistics
• A new parametrization of Hubble function and Hubble tension
• Holographic dark energy at the Ricci scale
• Black holes and wormholes in $f(R)$ gravity with a kinetic curvature scalar
• Shear Dynamics in Higher Dimensional FLRW Cosmology
• Scalar field dark energy: Insights into cosmological evolution and black hole accretion
• Inflation driven by q-de Sitter
• Local measurement of Λ using pulsar timing arrays
• Reconstructing thawing quintessence with multiple datasets
• Cosmological Model-independent Gamma-ray Bursts Calibration and its Cosmological Constraint to Dark Energy
• Baryon acoustic scale at $z_{\eff} = 0.166$ with the SDSS blue galaxies
• Probing the cosmic acceleration from combinations of different data sets
• Equilibrium boundary conditions, dynamic vacuum energy, and the Big Bang
• The effect of curvature in thawing models
• Validity of Thermodynamical Laws in Dark Energy Filled Universe
• Cosmological implications of non-minimally coupled f(Q) gravity
• A Fast and Accurate Analytic Method of Calculating Galaxy Two-point Correlation Functions
• Signals of Inflation in a Friendly String Landscape
• Bose-Einstein condensation as an alternative to inflation
• Cosmological science enabled by Planck
• Kaniadakis entropy-based characterization of IceCube PeV neutrino signals
• Time Variable Cosmological Constant from Renormalization Group Equations
• Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• Cosmological constant constraints from observation-derived energy condition bounds and their application to bimetric massive gravity
• Model Selection using Baryon Acoustic Oscillations in the Final SDSS-IV Release
• On the cosmological gravitational waves and cosmological distances
• The Bianchi type-V Dark Energy Cosmology in Self Interacting Brans Dicke Theory of Gravity
• Constraining $f(T,B,T_G,B_G)$ gravity by dynamical system analysis
• Complementarity of Future Dark Energy Probes
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Revisiting kink-like parametrization and constraints using OHD/Pantheon+/BAO samples
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories
• Understanding Galaxy Formation and Evolution
• Scalar Mode Quadrupole Radiation from Astronomical Sources in $F(R)$ Modified Gravity
• Baryon acoustic oscillations with the cross-correlation of spectroscopic and photometric samples
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys
• Probing Quintessence using BAO imprint on the cross-correlation of weak lensing and post-reionization HI 21 cm signal
• Cosmic scenarios in $f(R)$ gravity: a complete evolution
• On the viability of a certain vector-tensor theory of gravitation
• Analysis of recent type Ia supernova data based on evolving dark energy models
• A comprehensive analysis of the compact phase space for Hu-Sawicki $f(R)$ dark energy models including spatial curvature
• On the $2^{\text{nd}}$ feature of the matter two-point function
• Holographic Dark Energy with Curvature
• Dark Energy: is it `just' Einstein's Cosmological Constant Lambda?
• Holographic inflation and holographic dark energy from entropy of the anti-de Sitter black hole
• Observational constraints on tachyonic chameleon dark energy model
• The coincidence problem in $f(R)$ gravity models
• Impact of dark energy on the equation of state in light of the latest cosmological data
• The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sample
• Growth rate of matter perturbations as a probe of large-scale magnetism
• Galaxy formation from a timescale perspective
• Constraints on Dark Energy from New Observations including Pan-STARRS
• Relaxing cosmological constraints on current neutrino masses
• Spectral Distortion in a Radially Inhomogeneous Cosmology
• Deep learning for cosmological parameter inference from a dark matter halo density field
• Testing the coincidence problem with strong gravitational lens, Type Ia supernovae and Hubble parameter observational data
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• Complementary cosmological tests of RSII brane models
• Noether Symmetry Approach in Eddington-inspired Born-Infeld gravity
• Accelerating behavior from dynamical system analysis parameters
• Consistency of $f(R)$ gravity models around solar polytropes
• Cosmic Void Baryon Acoustic Oscillation Measurement: Evaluation of Sensitivity to Selection Effects
• Galaxy And Mass Assembly (GAMA): $\mathbf{z}\sim 0$ Galaxy Luminosity Function down to $\mathbf{L}\sim 10^6{\mathbf{L}}_{\odot }$ via Clustering Based Redshift Inference
• Sub-eV upper limits on neutrino masses from cosmology
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Precision Cosmology from X-ray AGN clustering
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• A new method to probe the mass density and the cosmological constant using configuration entropy
• Bias of reconstructing the dark energy equation of state from the Pad$\acute{e}$ cosmography
• Cosmological future singularities in massive gravity and massive bigravity
• Constraints on the unified dark energy-dark matter model from latest observational data
• Dark energy effects on realistic neutron stars
• Testing Dvali-Gabadadze-Porrati Gravity with Planck
• Cosmological Study in Myrzakulov $F(R,T)$ Quasi-dilaton Massive Gravity
• A Study of Selection Methods for H alpha Emitting Galaxies at z~1.3 for the Subaru/FMOS Galaxy Redshift Survey for Cosmology (FastSound)
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• Conditions for the Absence of Infrared Sensitivity in Cosmological Probes in Any Gravity Theories
• Some Specific Wormhole Solutions in Extended $f(R,G,T)$ Gravity
• Improving Constraint on ${\Omega }_m$ from SDSS Using Marked Correlation Functions
• The Schr$\ddot{o}$dinger-Poisson equations as the large-N limit of the Newtonian N-body system: applications to the large scale dark matter dynamics
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
• An introduction to the dark energy problem
• de Sitter field equations from quadratic curvature gravity: A group theoretical approach
• Measurement of the baryonic acoustic oscillation scale in 21 cm intensity fluctuations during the reionisation era
• Can the coincidence problem be solved by a cosmological model of coupled dark energy and dark matter?
• Observational constraints on viscous cosmology in $f(T,L_m)$ gravity
• Barrow holographic dark energy interacting model in the presence of radiation and matter
• Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
• Bayesian analysis of running holographic Ricci dark energy
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Modeling dark energy through an Ising fluid with network interactions
• Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
• Expressing the equation of state parameter in terms of the three dimensional cosmic shear
• Probing cosmology via the clustering of critical points
• The redshift distribution of absorption-line systems in QSO spectra
• Modified Friedmann equations via conformal Bohm -- De Broglie gravity
• Emergent D-instanton as a source of Dark Energy
• 2D BAO vs 3D BAO: Hints for new physics?
• Role of generalized Ricci dark energy on Chameleon field in the emergent universe
• Second order invariants and holography
• Ray-tracing log-normal simulation for weak gravitational lensing: application to the cross-correlation with galaxies
• Constraining Red-shift Parametrization Parameters in Brans-Dicke Theory: Evolution of Open Confidence Contours
• Constraints on Holographic cosmologies from strong lensing systems
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• The Friedmann equations in deformed Hořava-Lifshitz gravity and Debye model
• Large-scale periodicity in the distribution of QSO absorption-line systems
• Comparison of Supernovae datasets Constraints on Dark Energy
• Cosmological Evolution of Viscous Dark Energy in f(Q,C) Gravity: Two-Fluid Approach
• Shadows and Observational Images of a Schwarzschild-like Black Hole Surrounded by a Dehnen-type Dark Matter Halo
• Geometric Interpretations of the $k$-Nearest Neighbour Distributions
• Tensor B mode and stochastic Faraday mixing
• Early dark energy in the pre- and post-recombination epochs
• Observing Baryon Oscillations with Cosmic Shear
• Cosmic Evolution of the Kantowski-Sachs Universe in the Context of a Bulk Viscous String in Teleparallel Gravity
• Mass-Dependent Baryon Acoustic Oscillation Signal and Halo Bias
• Modified Gravity with Nonminimal Curvature-Matter Couplings: A Framework for Gravitationally Induced Particle Creation
• Detection significance of Baryon Acoustic Oscillations peaks in galaxy and quasar clustering
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Observational constraints on a Yang-Mills condensate dark energy model
• Distance Duality Test: The Evolution of Radio Sources Mimics a Nonexpanding Universe
• A Study of Universal Thermodynamics in Massive Gravity: Modified Entropy on the Horizons
• Uncertainty in the visibility mask of a survey and its effects on the clustering of biased tracers
• Generalized Ghost Pilgrim Dark Energy Fractal Cosmology with Observational Constraint
• Multiscalar field cosmological model and possible solutions using Noether symmetry approach
• The establishment of the Standard Cosmological Model through observations
• Cosmological dynamics of interacting dark energy and dark matter in $f(Q)$ gravity
• Constraints on dark energy evolution
• Spectrophotometric redshifts for $\mathrm{z}\sim 1$ galaxies and predictions for number densities with WFIRST and Euclid
• Lensing of 21cm Absorption "Halos" of $z\sim$20-30 First Galaxies
• Experimental status of particle and astroparticle searches for supersymmetry
• Spinor quintom cosmology with intrinsic spin
• Thermodynamics of a Non-canonical $f(\bar{R},\bar{T})$ gravity
• Cosmography from accurate mass modeling of the lens group SDSS J0100+1818: five sources at three different redshifts
• Galaxy Superclusters and Their Complexes in the Cosmic Web
• Analytical considerations about the cosmological constant and dark energy
• Universal conditional distribution function of [OII] luminosity of galaxies, and prediction for the [OII] luminosity function at redshift $z<3$
• WIMP dark matter in bulk viscous non-standard cosmologies
• On the propagation of gravitational waves in a $\Lambda$CDM universe
• Improving the accuracy of estimators for the two-point correlation function
• Optimizing BAO measurements with non-linear transformations of Lyman-alpha forest
• Stochastic contribution to the growth factor in the LCDM model
• Constraining the runaway dilaton and quintessential dark energy
• Euclid preparation. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey
• Cosmic Reionization Study : Principle Component Analysis After Planck
• Cosmology with voids from the Nancy Grace Roman Space Telescope
• Angular Correlation Function from sample covariance with BOSS and eBOSS LRG
• New measures to test modified gravity cosmologies
• Forecasting 21-cm power spectrum sensitivity to dark Matter-baryon scattering
• The SDSS DR7 Galaxy Angular Power Spectrum: Volume-Limits and Galaxy Morphology
• Lognormal semi-numerical simulations of the Lyman-$\alpha$ forest: comparison with full hydrodynamic simulations
• Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars
• Globular clusters as cosmic clocks: new cosmological hints from their integrated light
• Expanding, shearing and accelerating isotropic plane symmetric universe with conformal Kasner geometry
• Effects of Angular Momentum on Halo Profiles
• Non-singular bouncing cosmology in $f(T,\mathcal{T})$ gravity with energy condition violations
• Dynamical Oscillations in Dark Energy: Joint Constraints on the $w_{sin}$CDM Model from DESI, OHD, and Supernova Samples
• Analysis on a General Class of Holographic Type Dark Energy Models
• A comprehensive analysis of Barrow holographic Chaplygin gas model reconstruction and its cosmological consequences
• A class of regular bouncing cosmologies
• Transients from initial conditions based on Lagrangian perturbation theory in $N$-body simulations II: the effect of the transverse mode
• Realizing the phantom-divide crossing with vector and scalar fields
• Optimizing the Recovery of Fisher Information in the Dark Matter Power Spectrum
• Small cosmological constant in seesaw mechanism with breaking down SUSY
• BBN to Late-Time Acceleration in $f(T,{\mathcal{L}}_m)$ Gravity
• SUSY SU(5) $\times S_4$ GUT Flavor Model for Fermion Masses and Mixings with Adjoint, Large ${\theta }_{13}^{PMNS}$
• Pseudo Newtonian Potential For a Rotating Kerr Black Hole Embedded in Quintessence
• Infrared divergence of pure Einstein gravity contributions to cosmological density power spectrum
• Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results
• Incompatibility of Standard Galaxy Bias Models in General Relativity
• Estimations of the cosmological parameters from the observational variation of the fine structure constant
• Confronting the damping of the baryon acoustic oscillations with observation
• Quasi-periodical components in the radial distributions of cosmologically remote objects
• Cosmic distance determination from photometric redshift samples using BAO peaks only
• Breaking the ${\tau }_{\mathrm{T}}-f$ degeneracy of the kinetic Sunyaev Zel'dovich cosmology in redshift space
• Probing Dark Energy Properties in $fQ,C)$ Gravity with FLRW Cosmological Models
• Isochronous Spacetimes
• Nonparametric determination of redshift evolution index of Dark Energy
• Effective field theory of coupled dark energy and dark matter
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Exploring the deviation of cosmological constant by a generalized pressure dark energy model
• On the origin of the BAOtr-DESI tension
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• The reconstruction of dark energy with Ridge Regression Approach
• Observational Study of Higher Dimensional Magnetic Universe in Non-linear Electrodynamics
• Data Analysis and Phenomenological Cosmology
• Latest Cosmological Constraints on Cardassian expansion models including the updated Gamma-ray bursts
• Observational Constraints on Phantom Crossing DGP Gravity
• Reconstructing the Cosmic Expansion History with a Monotonicity Prior
• Non-Affine Extensions of the Raychaudhuri Equation in the K-essence Framework
• Gravitational Bounce from the Quantum Exclusion Principle
• Interacting dark sector with quadratic coupling: theoretical and observational viability
• Baryon Acoustic Oscillations analyses with Density-Split Statistics
• Anisotropic cosmology in Bumblebee gravity theory
• Reconstruction of 5D Cosmological Model From Recent Observations
• Power-law solutions for TeVeS
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Growth of matter perturbations for realistic $F(R)$ models
• Cosmology with Galaxy Correlations
• Euclid: Fast two-point correlation function covariance through linear construction
• Asymptotic Cosmological Behavior of Scalar-Torsion Mode in Poincare Gauge Theory
• Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys
• Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• Statistical Nuances in BAO Analysis: Likelihood Formulations and Non-Gaussianities
• Voids as Alternatives to Dark Energy and the Propagation of Gamma Rays through the Universe
• Using dust to constrain dark matter models
• An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data
• Characterizing the equivalence between dark energy and radiation using gamma-ray bursts
• Gravitational Lensing of Dark Energy Models and $\Lambda$CDM Using Observational data in Loop Quantum Cosmology
• de Sitter spacetime with a Becchi-Rouet-Stora quartet
• Observational constraints on cosmological parameters in the Bianchi type III Universe with f(R,T) gravity theory
• A comparison of cosmological models with high-redshift quasars
• Mixing Bispectrum Multipoles Under Geometric Distortions
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Cosmological constraints in symmetric teleparallel gravity with bulk viscosity
• Inferring the density and membership of stellar streams with flexible models: The GD-1 stream in Gaia Data Release 3
• Constraining Chaplygin models using diffuse supernova neutrino background
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Stellar Profile Independent Determination of the Dark Matter Distribution of the Fornax Local Group Dwarf Spheroidal Galaxy
• An Algorithm to locate the centers of Baryon Acoustic Oscillations
• Upper limits on neutrino masses from cosmology
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• Observational constraints on models of the Universe with time variable Gravitational and Cosmological constants along MOG
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Probing the time variation of the effective Newton's constant with optimal redshift weights
• Exact Solutions and Constraints on the Dark Energy Model in FRW Universe
• Unification of Dark Matter and Dark Energy in a Modified Entropic Force Model
• Densified pupil spectrograph as high-precision radial velocimetry: From direct measurement of the Universe's expansion history to characterization of nearby habitable planet candidates
• Coupling q-deformed dark energy to dark matter
• On the correctness of cosmology from quantum potential
• Cosmology with type-Ia supernovae
• Hubble Expansion as an Einstein Curvature
• Observational Constraints on the Cosmology with Holographic Dark Fluid
• Asymptotically Static Universe
• Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis
• Multipole analysis in the radiation field for linearized $f(R)$ gravity with irreducible Cartesian tensors
• Higher Dimensional Cosmology with Some Dark Energy Models in Emergent, Logamediate and Intermediate Scenarios of the Universe
• APSIS - an Artificial Planetary System in Space to probe extra-dimensional gravity and MOND
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 $<$ z $<$ 0.45 -- status update
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples
• Cosmological constraints with the linear point from the BOSS survey
• $f(T)$ gravity from holographic Ricci dark energy model with new boundary conditions
• Effects of high-order operators in non-relativistic Lifshitz holography
• FIMP Dark Matter in bulk viscous non-standard cosmologies
• Eigenmode analysis of perurbations in the primordial medium at and before recombination
• Cosmological constraints from galaxy clustering
• A New Approach to Testing Dark Energy Models by Observations
• The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks
• Tomographic Alcock-Paczynski Method with Redshift Errors
• The Hubble constant and dark energy
• Viscous fluid dynamics with decaying vacuum energy density
• Embedded Lensing Time Delays, the Fermat Potential, and the Integrated Sachs-Wolfe Effect
• Can MONDian vector theories explain the cosmic speed up ?
• A unification of RDE model and XCDM model
• Quintessence like behavior of symmetric teleparallel dark energy: Linear and nonlinear model
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Measuring $H_0$ with pulsar timing arrays
• Cosmic expansion beyond $\Lambda$CDM: Investigating power-law and logarithmic corrections
• Is non-particle dark matter equation of state parameter evolving with time?
• Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope
• Constraining the Nonextensive Mass Function of Halos from BAO, CMB and X-ray data
• Classical and quantum cosmology in $f(T)$-gravity theory: A Noether symmetry approach
• Barboza-Alcaniz Equation of State Parametrization : Constraining the Parameters in Different Gravity Theories
• Constraining Recent Oscillations in Quintessence Models with Euclid
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• Observational constraints on thawing quintessence scalar field model
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• An Alcock-Paczynski Test on Reionization Bubbles for Cosmology
• Noether symmetry approach in non-minimal derivative coupling gravity
• On the maximum volume of collapsing structures
• How does Inflation Depend Upon the Nature of Fluids Filling Up the Universe in Brane World Scenario
• Investigating the Redshift Evolution of Lensing Galaxy Density Slopes via Model-Independent Distance Ratios
• Constraints on scalar-tensor theories from observations
• Variable Modified Chaplygin Gas in Anisotropic Universe with Kaluza-Klein Metric
• 5-dimensional braneworld with gravitating Nambu-Goto matching conditions
• Evolution of Cluster Alignments as Evidence of Large-scale Structure Formation in the Universe
• Modelling the covariance matrix for the power spectra before and after the BAO reconstruction
• Mass scaling relations for dark halos from an analytic universal outer density profile
• Monopole Fluctuations in Galaxy Surveys
• Thermodynamics and holography of tachyon cosmology
• Reconstructing cosmic evolution with a density parametrization
• Photo-z optimization for measurements of the BAO radial direction
• Dark aspects of massive spinor electrodynamics
• A new consistency test for $\Lambda$CDM cosmology using galaxy surveys
• Generalized second law of thermodynamics in massive gravity
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
• The general expression for $f(T)$ in a charged cylindrical spacetime with diverse dimensions
• Cosmological scenario based on the particle creation and holographic equipartition
• Toward a Measurement of the Transverse Peculiar Velocity of Galaxy Pairs
• Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
• Holographic F(Q,T) Gravity with Lambert Solution
• Cuscuton-like contribution to dark energy evolution
• New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
• Cosmological Reconstructions in Einstein--Cartan--Myrzakulov Gravity with Torsion and Non-Metricity in the Weitzenböck Geometrical Sector
• Traces of Anisotropic Quasi-Regular Structure in the SDSS Data
• Constraining the Equation of State of Dark Energy with Gamma Rays
• Hubble Diagrams in the Jordan and Einstein Frames
• Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
• Symmetry and Conserved Quantities in $f(R)$-Gravity: Mei vs. Noether Approaches
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Primordial fluctuations from deformed quantum algebras
• A cosmic speed-trap: a gravity-independent test of cosmic acceleration using baryon acoustic oscillations
• Colliders and Cosmology
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Braneworlds with timelike extra-dimension
• Dark Energy Survey: DESI-Independent Angular BAO Measurement
• Dynamics of the universe as a "test 3-brane" in a 5D bulk
• Holographic Principle and the Second Law in Stephani Cosmology Revisited
• Degeneracy and Discreteness in Cosmological Model Fitting
• New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• Phantom scalar field cosmologies constrained by early cosmic measurements
• Non-vacuum relativistic extensions of MOND using metric theories of gravity with curvature-matter couplings and their applications to the accelerated expansion of the Universe without dark components
• Red-shift parametrizations of dark energy and observational constraint on their parameters: Galileon gravity as background
• Revisiting the effect of lens mass models in cosmological applications of strong gravitational lensing
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Geometric sigma model of the Universe
• Angular Diameter Distance Measurement with Galaxy Clustering in the Multipole Space
• On the possibility of Baryon Acoustic Oscillation measurements at redshift $z>7.6$ with the Roman Space Telescope
• Constraint on the growth factor of the cosmic structure from the damping of the baryon acoustic oscillation signature
• Assessing the Robustness of the CPL Parametrization to Basis and Prior Variations: Insights from DESI DR2 BAO Data
• Wald Entropy in Extended Modified Myrzakulov Gravity Theories: \(f(R, T, Q, R_{μν}T^{μν}, R_{μν}Q^{μν}, \dots)\)
• The Effect of Interstellar Absorption on Measurements of the Baryon Acoustic Peak in the Lyman-α Forest
• Development of a model to investigate the effect of the bias in SNIa measurements related to the inhomogeneity of space
• 21-cm power spectrum and ionization bias as a probe of long-mode modulated non Gaussian sky
• Constraining bouncing cosmology caused by Casimir effect
• Post-Newtonian Gravitational Waves with cosmological constant $\Lambda$ from the Einstein-Hilbert theory
• Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data
• Probing the Type 3 interacting dark-energy model using matter pairwise velocity
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• Broad Brush Cosmos
• Electrovac Universes with a Cosmological Constant
• Impact of a Rapid Diluted Energy Density on the halo mass function
• The equation and solution of 4-point correlation function of galaxies in Gaussian approximation and its parity-odd part
• A new approach to modified-gravity models
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Holographic Ricci DE as running vacuum with nonlinear interactions
• Exploring the Universe Expansion History with f(R,T) Gravity: Constraints on Cosmological Parameters
• The Impact of Spectroscopic Redshift Errors on Cosmological Measurements
• Oscillating universe in massive bigravity
• A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Largest scales from the largest galaxy surveys: the pseudo Karhunen-Loève method
• Cosmological constraints on the big bang quantum cosmology model
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• A semi-cosmographic approach to study cosmological evolution in phase space
• Constraints on a scalar-tensor model with Gauss-Bonnet coupling from SN Ia and BAO observations
• Constraining super-critical string/brane cosmologies with astrophysical data
• On the fairness of the main galaxy sample of SDSS
• Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement
• A dynamical dark energy model with a given luminosity distance
• Cosmology with CMB anisotropy
• Agegraphic dark energy from entropy of the anti-de Sitter black hole
• Modified scaling in $k$-essence model in interacting dark energy - dark matter scenario
• Gravitational waves in massive Horndeski theory with a potential
• Constraints on dark energy and cosmic topology
• On the baryon acoustic oscillation amplitude as a probe of radiation density
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Cold Collapse and Bounce of an FLRW Cloud
• Cluster optical depth and pairwise velocity estimation using machine learning
• Challenges to the cosmological constant model following results from the Dark Energy Survey
• On Nash theory of gravity with matter contents
• The Effects of Spatial Curvature on Cosmic Evolution
• Sub-percentage measure of distances to redshift of 0.1 by a new cosmic ruler
• Cosmological Constraints on the Undulant Universe
• A comprehensive dynamical and phenomenological analysis of structure growth in curvature-modulated coupled quintessence scenario
• Static, Cylindrically Symmetric Spacetimes in the Coincident f(Q) Gravity
• Fluids in cosmology
• Cosmic expansion history analysis with Hubble parametrization in $Q^n$ gravity
• Probing the integrated Sachs-Wolfe effect using embedded lens models
• Accelerating BAO Scale Fitting Using Taylor Series
• Phase space of multi-fluid universe in $F(T)$-gravity and some enhancements for the oscillating interaction model
• Perturbations with bulk viscosity in modified chaplygin gas cosmology
• Estimating Third-Order Moments for an Absorber Catalog
• Dark Energy Behavior from Static Equation of State in Non-Minimally Coupled Gravity with Scalar Deformation
• Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (Ω_{m0}) Measurements
• Isochronous solutions of Einstein's equations and their Newtonian limit
• The Dark Energy Survey Supernova Program results: Type Ia Supernova brightness correlates with host galaxy dust
• Semi-holographic model revisited
• Spinor-Unit Field Representation of Electromagnetism Applied to a Model Inflationary Cosmology
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• Scale-free power spectrums in the delayed cosmology
• Solar System Tests of a New Class of $f(z)$ Theory
• Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ~ 0.8 with BOSS and DESI
• Cosmological solutions and observational constraints on 5-dimensional braneworld cosmology with gravitating Nambu-Goto matching conditions
• Exact solutions of embedding the 4D Universe in a 5D Einstein manifold
• Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law $f(Q)$ Gravity with Quasars
• Comparing LambdaCDM, wCDM, and w0waCDM models with DESI DR2 BAO: Redshift-Resolved Diagnostics and the Role of rd
• Dark energy with oscillatory tracking potential: Observational Constraints and Perturbative effects
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• Testing General Relativity on Galactic Scales via DESI-BAO and Strong Lensing: Circumventing Assumptions on the Hubble Constant, Sound Horizon, and Dark Energy
• Cosmology in the presence of diffeomorphism-violating, nondynamical background fields
• Phase space analysis of Rényi Holographic dark energy model
• A Spectrum of Cosmological Rips and Their Observational Signatures
• Observational Constraints and Cosmological Dynamics of Interacting Fractional Holographic Dark Energy in Light of DESI DR2
• Relativistic Angular Redshift Fluctuations embedded in Large Scale Varying Gravitational Potentials
• `Standard' Cosmological model & beyond with CMB
• Observational and Thermodynamic aspects of one-dimensional Dark Energy EoS parametrization models
• A lightcone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
• Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity
• Accurate and efficient likelihood modeling for large-scale CMB data
• Can we remove the systematic error due to isotropic inhomogeneities?
• Cosmological constraints from the density gradient weighted correlation function
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• From Redshift to Real Space: Combining Linear Theory With Neural Networks
• Using the large scale quasar clustering to constrain flat quintessential universes
• New effective theories of gravitation and their phenomenological consequences
• Constraining effective neutrino species with bispectrum of large scale structures
• Tomographic Alcock-Paczynski Test with Marked Correlation Functions
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging
• Phase space analysis of Bianchi III Universe with $f(R,T)$ gravity theory
• Implications of the correlation between bulge-to-total baryonic mass ratio and the number of satellites for SAGA galaxies
• A Study on Ricci Dark Energy in Bulk-Brane Interaction
• The impact of the locally measured Hubble parameter on the mass of Sterile neutrino
• Holographic dark energy in Einstein-Cartan spin cosmology
• Baryon Acoustic Oscillations in tomographic Angular Density and Redshift Fluctuations
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• Geometric formulation of $k$-essence and late-time acceleration
• Optimizing Gaussian Process Kernels Using Nested Sampling and ABC Rejection for H(z) Reconstruction
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• On Generalized Theories of Varying Fine Structure Constant
• Gamma-Ray Bursts, Supernovae Ia and Baryon Acoustic Oscillations: a binned cosmological analysis
• Confusing dark matter particle properties with modifications to General Relativity
• A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation
• Cosmological quests in the CMB sky
• Exploring the Viability of $f(Q,T)$ Gravity: Constraining Parameters with Cosmological Observations
• Friedmann-free limits on spatial curvature
• Generalized Noether Theorem for Gauss-Bonnet Cosmology
• From Geometry to Observation: Gravitational Waves and the Raychaudhuri Equation
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• A comparative study of emergent dark energy models
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey quasar sample: Testing observational systematics on the Baryon Acoustic Oscillation measurement
• Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB
• Is the $\Lambda$CDM Model in Crisis?
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Comparative Study of $f(T)$ Gravity Models with Observational Constraints from \textit{OHD} and \textit{Pantheon+ datasets}
• Exploring the constraints on cosmological models with CosmoEJS
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
• Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse
• Generalized Eddington--Finkelstein Coordinates and Exact Vaidya-Type Solutions in Weyl Conformal Gravity
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• Extended datasamples under the lens of Brane World Theory
• Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS
• Cosmological solutions of Tensor-Vector theories of gravity with varying the space-time-matter coupling constant
• A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background
• Sector-Resolved Bayesian Model Averaging for DESI-Era Cosmology
• Testing the CCC+TL cosmology with cosmic-chronometer measurements of the Hubble parameter
• Finding High-Redshift Galaxies with JWST
• Shadows and photon spheres of static black holes embedded in a Dehnen-(1,4,5/2)-type dark matter halo with a quintessential field
• Hubble Expansion Signature on Simulated Halo Density Profiles: A Path to Observing the Turnaround Radius
• The nonlinear equation of correlation function of galaxies in the expanding universe and the solution in linear approximation
• Effect of the cosmological parameters on gravitational waves: general analysis
• Cosmic chronometers with galaxy clusters: a new avenue for multi-probe cosmology
• Effective $\Lambda$CDM model emerging from $f(Q,T)$ under a special EOS limit in symmetric cosmology with Bayesian and ANN observational constraints
• Constraining the Hubble Constant with a Simulated Full Covariance Matrix Using Neural Networks
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• Cosmology of Cubic Poincaré Gauge gravity
• Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space
• Linearized Treatment of Scalar perturbations in the Asymptotic Cosmological Model
• Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum
• Non-singular Bouncing Cosmology in $f(R,G,T)$--Quintom model
• Fluctuation of the Hubble parameter
• Dynamics of quasi de Sitter and linear combination of exponential models in extended gravity
• The BAO scale -- how standard is the standard ruler?
• A speed limit on tachyon fields from cosmological and fine-structure data
• Probing late-time annihilations of oscillating asymmetric dark matter via rotation curves of galaxies
• Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
• Late-Time Cosmic Acceleration in Ricci-Gauss-Bonnet Gravity via Gradient Descent Optimization
• Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole
• Relativistic Langevin Equation derived from a particle-bath Lagrangian
• Energy conditions and entropy density of the universe
• Systematic treatment of non-linear effects in Baryon Acoustic Oscillations