Challenges for $\Lambda$CDM: An update

Abstract

A number of challenges to the standard $\Lambda$CDM model have been emerging during the past few years as the accuracy of cosmological observations improves. In this review we discuss in a unified manner many existing signals in cosmological and astrophysical data that appear to be in some tension ($2\sigma$ or larger) with the standard $\Lambda$CDM model as specified by the Cosmological Principle, General Relativity and the Planck18 parameter values. In addition to the well-studied $5\sigma$ challenge of $\Lambda$CDM (the Hubble $H_0$ tension) and other well known tensions (the growth tension, and the lensing amplitude $A_L$ anomaly), we discuss a wide range of other less discussed less-standard signals which appear at a lower statistical significance level than the $H_0$ tension some of them known as 'curiosities' in the data) which may also constitute hints towards new physics. For example such signals include cosmic dipoles (the fine structure constant $\alpha$, velocity and quasar dipoles), CMB asymmetries, BAO Ly$\alpha$ tension, age of the Universe issues, the Lithium problem, small scale curiosities like the core-cusp and missing satellite problems, quasars Hubble diagram, oscillating short range gravity signals etc. The goal of this pedagogical review is to collectively present the current status (2022 update) of these signals and their level of significance, with emphasis on the Hubble tension and refer to recent resources where more details can be found for each signal. We also briefly discuss theoretical approaches that can potentially explain some of these signals.

arXiv comment106 pages, 22 figures, 7 tables. 2022 update (updated tables, figures, models and model constraints). Comments and suggestions for next version are welcome

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• An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
• Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
• Hemispherical power asymmetry in the three-year Wilkinson Microwave Anisotropy Probe sky maps
• A precision calculation of relic neutrino decoupling
• Gaussian Process Cosmography
• Evidence of vorticity and shear at large angular scales in the WMAP data: a violation of cosmological isotropy?
• The small scatter of the baryonic Tully-Fisher relation
• On the large-angle anomalies of the microwave sky
• An Improved Distance to NGC 4258 and its Implications for the Hubble Constant
• New Extraction of the Cosmic Birefringence from the Planck 2018 Polarization Data
• Insights on Dark Matter from Hydrogen during Cosmic Dawn
• Gravitational waves and pulsating stars: What can we learn from future observations?
• Stable Operation of a 300-m Laser Interferometer with Sufficient Sensitivity to Detect Gravitational-Wave Events within our Galaxy
• Does the Hubble constant tension call for new physics?
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the Quasar sample between redshift 0.8 and 2.2
• The Clustering of the SDSS Main Galaxy Sample II: Mock galaxy catalogues and a measurement of the growth of structure from Redshift Space Distortions at $z=0.15$
• Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background Anisotropies
• A Test of the Cosmological Principle with Quasars
• Gravitational-Wave Stochastic Background from Kinks and Cusps on Cosmic Strings
• Weighing the Giants - I. Weak-lensing masses for 51 massive galaxy clusters: project overview, data analysis methods and cluster images
• The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
• On the possible running of the cosmological "constant"
• CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
• Implications of WMAP observations on Li abundance and stellar evolution models
• Cosmic flows in the nearby universe from Type Ia Supernovae
• Model independent evidence for dark energy evolution from Baryon Acoustic Oscillations
• Measurements of the E-Mode Polarization and Temperature-E-Mode Correlation of the CMB from SPT-3G 2018 Data
• To H0 or not to H0?
• Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
• Weighing the Giants - III. Methods and Measurements of Accurate Galaxy Cluster Weak-Lensing Masses
• Baryon acoustic oscillations from the complete SDSS-III Ly$\alpha$-quasar cross-correlation function at $z=2.4$
• Evidence for massive neutrinos from CMB and lensing observations
• Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
• Small scale problems of the $\Lambda$CDM model: a short review
• Increasing evidence for hemispherical power asymmetry in the five-year WMAP data
• BayesLine: Bayesian Inference for Spectral Estimation of Gravitational Wave Detector Noise
• Spatial variation in the fine-structure constant -- new results from VLT/UVES
• Early dark energy from massive neutrinos -- a natural resolution of the Hubble tension
• The scaling evolution of cosmological constant
• Cosmological Constraints from Galaxy Clusters in the 2500 square-degree SPT-SZ Survey
• Symmetron Cosmology
• A parametric model for dark energy
• X-ray emission from radio-quiet quasars in the SDSS Early Data Release. The alpha_ox dependence upon UV luminosity
• CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics
• Type II Supernovae as Standardized Candles
• Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
• ETHOS - An Effective Theory of Structure Formation: Dark matter physics as a possible explanation of the small-scale CDM problems
• The Baryon Content of Extremely Low Mass Dwarf Galaxies
• Large-angle anomalies in the CMB
• The Angular Trispectrum of the CMB
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• IndIGO and LIGO-India: Scope and Plans for Gravitational Wave Research and Precision Metrology in India
• Constraining Early Dark Energy with Large-Scale Structure
• Population III stars: hidden or disappeared ?
• Baryonic Signatures in Large-Scale Structure
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Too Big to Fail in the Local Group
• ETHOS - An Effective Theory of Structure Formation: From dark particle physics to the matter distribution of the Universe
• The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at $z\sim 1.4$
• Cosmology with x-matter
• A SHARP view of H0LiCOW: $H_0$ from three time-delay gravitational lens systems with adaptive optics imaging
• The Distribution of Satellite Galaxies: The Great Pancake
• Baryon acoustic oscillations from the cross-correlation of Ly$\alpha$ absorption and quasars in eBOSS DR14
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• KiDS+GAMA: Cosmology constraints from a joint analysis of cosmic shear, galaxy-galaxy lensing and angular clustering
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Elucidating $\Lambda$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
• Resolving the Hubble Tension with New Early Dark Energy
• On the scaling behavior of the cosmological constant and the possible existence of new forces and new light degrees of freedom
• Baryon acoustic oscillations at z = 2.34 from the correlations of Ly$\alpha$ absorption in eBOSS DR14
• STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354
• Local determination of the Hubble constant and the deceleration parameter
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• The mass function
• Time Delay Cosmography
• A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
• The Primordial Black Hole Dark Matter - LISA Serendipity
• Super-Planckian Spatial Field Variations and Quantum Gravity
• A Hubble Diagram for Quasars
• Maximal Localisation in the Presence of Minimal Uncertainties in Positions and Momenta
• Is the Hubble tension a hint of AdS phase around recombination?
• The DESI Experiment Part II: Instrument Design
• On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030
• Evolution of the $f{\sigma }_8$ tension with the Planck15/$\Lambda$CDM determination and implications for modified gravity theories
• Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z)\ge -1$ are tighter than those obtained in $\Lambda$CDM
• The Extreme Faint End of the UV Luminosity Function at $z\sim 6$ Through Gravitational Telescopes: a comprehensive assessment of strong lensing uncertainties
• TDCOSMO. I. An exploration of systematic uncertainties in the inference of $H_0$ from time-delay cosmography
• The dark matter crisis: falsification of the current standard model of cosmology
• The Hubble Space Telescope Key Project on the Extragalactic Distance Scale XXIV: The Calibration of Tully-Fisher Relations and the Value of the Hubble Constant
• Tension and constraints on modified gravity parametrizations of $G_{\text{eff}}(z)$ from growth rate and Planck data
• Neutrino mass from Cosmology
• Dark Radiation constraints on minicharged particles in models with a hidden photon
• Nonparametric Dark Energy Reconstruction from Supernova Data
• $\nu \Lambda$CDM: Neutrinos help reconcile Planck with the Local Universe
• Signs of Dark Matter at 21-cm?
• Local-Group tests of dark-matter Concordance Cosmology: Towards a new paradigm for structure formation
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights
• The Parkes Pulsar Timing Array
• Is there a "too big to fail" problem in the field?
• Equivalence Principle Implications of Modified Gravity Models
• The non-Gaussian Cold Spot in the 3-year WMAP data
• Scalar-Tensor Models of Normal and Phantom Dark Energy
• New Early Dark Energy
• The third data release of the Kilo-Degree Survey and associated data products
• Dark energy in Horndeski theories after GW170817: A review
• First evidence of running cosmic vacuum: challenging the concordance model
• Dark Energy and Dark Matter
• Testing Primordial Black Holes as Dark Matter through LISA
• Can vacuum decay in our Universe?
• Relieving the Hubble tension with primordial magnetic fields
• Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
• Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects: A Millimetre/Submillimetre Probe of the Warm and Hot Universe
• Quantifying discordance in the 2015 Planck CMB spectrum
• Spontaneous Isotropy Breaking: A Mechanism for CMB Multipole Alignments
• Dark Matter Cores and Cusps: The Case of Multiple Stellar Populations in Dwarf Spheroidals
• Reconciling CMB and structure growth measurements with dark energy interactions
• Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
• Standard Big-Bang Nucleosynthesis up to CNO with an improved extended nuclear network
• Evidence for anisotropy of cosmic acceleration
• Gravitational Lensing as a Probe of Quintessence
• Cosmology with a stiff matter era
• A buyer's guide to the Hubble Constant
• A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
• Cosmology with the lights off: Standard sirens in the Einstein Telescope era
• Cepheid Parallaxes and the Hubble Constant
• On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference
• Stability and Instability of Extreme Reissner-Nordström Black Hole Spacetimes for Linear Scalar Perturbations I
• The evidence for a spatially flat Universe
• A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies
• Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension
• The SPTpol Extended Cluster Survey
• Hubble Sinks In The Low-Redshift Swampland
• The baryonic Tully-Fisher relation for different velocity definitions and implications for galaxy angular momentum
• The Carnegie Supernova Project I: Third Photometry Data Release of Low-Redshift Type Ia Supernovae and Other White Dwarf Explosions
• The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
• A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
• The BAO+BBN take on the Hubble tension
• Strongly Coupled Chameleon Fields: New Horizons in Scalar Field Theory
• The SBF Survey of Galaxy Distances. I. Sample Selection, Photometric Calibration, and the Hubble Constant
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• KiDS-450: Testing extensions to the standard cosmological model
• KiDS-450: The tomographic weak lensing power spectrum and constraints on cosmological parameters
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample
• Can Late Dark Energy Transitions Raise the Hubble constant?
• Dark coupling
• A new measurement of the bulk flow of X-ray luminous clusters of galaxies
• Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
• Relativistic effects and dark matter in the Solar system from observations of planets and spacecraft
• The structure of voids
• A fresh look at linear cosmological constraints on a decaying dark matter component
• Distance determinations using type II supernovae and the expanding photosphere method
• Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
• Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant
• Galaxies as simple dynamical systems: observational data disfavor dark matter and stochastic star formation
• Running G and Λat low energies from physics at M_X: possible cosmological and astrophysical implications
• Revisiting a negative cosmological constant from low-redshift data
• Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
• The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant
• Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions
• Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1
• The DES Science Verification Weak Lensing Shear Catalogues
• Primordial black holes and second order gravitational waves from ultra-slow-roll inflation
• Evidence for a ~300 Mpc Scale Under-density in the Local Galaxy Distribution
• Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated $E_{\mathrm{p},\mathrm{i}}$ - $E_{\mathrm{iso}}$ correlation
• The importance of tides for the Local Group dwarf spheroidals
• Non-Abelian dark matter and dark radiation
• A Xylophone Configuration for a third Generation Gravitational Wave Detector
• The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
• 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
• Effective equation of state for dark energy: mimicking quintessence and phantom energy through a variable Lambda
• Cosmic Flows on 100 Mpc/h Scales: Standardized Minimum Variance Bulk Flow, Shear and Octupole Moments
• Constraints on Large-Scale Dark Acoustic Oscillations from Cosmology
• Fundamental photon orbits: black hole shadows and spacetime instabilities
• Review on Generalized Uncertainty Principle
• Coupled Variations of Fundamental Couplings and Primordial Nucleosynthesis
• The Atacama Cosmology Telescope: ACT-CL J0102-4915 "El Gordo," a Massive Merging Cluster at Redshift 0.87
• What Do Gravitational Lens Time Delays Measure?
• Does Hubble Tension Signal a Breakdown in FLRW Cosmology?
• How secret interactions can reconcile sterile neutrinos with cosmology
• Stability of the curvature perturbation in dark sectors' mutual interacting models
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• 2-Point Correlations in the COBE DMR 4-Year Anisotropy Maps
• The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
• Cosmology from large-scale structure: Constraining $\Lambda$CDM with BOSS
• Quasars as standard candles III. Validation of a new sample for cosmological studies
• Early dark energy is not excluded by current large-scale structure data
• The non-Gaussian Cold Spot in WMAP: significance, morphology and foreground contribution
• HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang
• Hot Axions and the $H_0$ tension
• The Time Delays of Gravitational Lens HE0435-1223: An Early-Type Galaxy With a Rising Rotation Curve
• On Quantum Field Theory with Nonzero Minimal Uncertainties in Positions and Momenta
• Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant
• Extragalactic Radio Sources and the WMAP Cold Spot
• Crossing the Phantom Divide Barrier with Scalar Tensor Theories
• Interacting Dark Sector and Precision Cosmology
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• Running Hubble Tension and a H0 Diagnostic
• The $H_0$ tension in light of vacuum dynamics in the Universe
• Cosmic radio dipole from NVSS and WENSS
• Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• Detection of the velocity dipole in the radio galaxies of the NRAO VLA Sky Survey
• Co-orbiting satellite galaxy structures are still in conflict with the distribution of primordial dwarf galaxies
• KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear
• Gravitational Lens Time Delays: A Statistical Assessment of Lens Model Dependences and Implications for the Global Hubble Constant
• Update on Coupled Dark Energy and the $H_0$ tension
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• A CMB Search for the Neutrino Mass Mechanism and its Relation to the $H_0$ Tension
• The Pseudo-$C_l$ method: Cosmic microwave background anisotropy power spectrum statistics for high precision cosmology
• Tighter Limits on Dark Matter Explanations of the Anomalous EDGES 21cm Signal
• Cosmic microwave background anisotropy power spectrum statistics for high precision cosmology
• Limits on $w$CDM from the EFTofLSS with the PyBird code
• The Standardized Candle Method for Type II Plateau Supernovae
• Dark energy: a quantum fossil from the inflationary Universe?
• The Gravitational-Wave Physics
• Structure formation in $f(T)$ gravity and a solution for $H_0$ tension
• Limits on Neutrino-Neutrino Scattering in the Early Universe
• Testing the Interaction between Dark Energy and Dark Matter with Planck Data
• Local Voids as the Origin of Large-angle Cosmic Microwave Background Anomalies I
• On the growth of linear perturbations
• Strong gravitational lensing of explosive transients
• The BayesWave analysis pipeline in the era of gravitational wave observations
• Backreacted Axion Field Ranges in String Theory
• The Three-Dimensional Structure of the M31 Satellite System; Strong Evidence for an Inhomogeneous Distribution of Satellites
• Dark sector interaction: a remedy of the tensions between CMB and LSS data
• Dark Energy with Phantom Crossing and the $H_0$ tension
• New constraints on Coupled Dark Energy from Planck
• E/B decomposition of finite pixelized CMB maps
• Correlation Function in Deep Redshift Space as a Cosmological Probe
• 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
• Searching for a Cosmological Preferred Axis: Union2 Data Analysis and Comparison with Other Probes
• Nonlocal gravity. Conceptual aspects and cosmological predictions
• Ram-pressure stripping of a kicked Hill sphere: Prompt electromagnetic emission from the merger of stellar mass black holes in an AGN accretion disk
• Large peculiar motion of the solar system from the dipole anisotropy in sky brightness due to distant radio sources
• Models of coupled dark matter to dark energy
• Observational Constraints on Teleparallel Dark Energy
• Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate
• Clarifying the Hubble constant tension with a Bayesian hierarchical model of the local distance ladder
• Galaxy-Galaxy Lensing in the Hubble Deep Field: The Halo Tully-Fisher Relation at Intermediate Redshift
• The LISA-Taiji network
• Deviations from the $1/r^2$ Newton law due to extra dimensions
• Dipoles in the Sky
• Tension with the flat ΛCDM model from a high redshift Hubble Diagram of supernovae, quasars and gamma-ray bursts
• Power asymmetry in WMAP and Planck temperature sky maps as measured by a local variance estimator
• The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant
• Using Quantitative Spectroscopic Analysis to Determine the Properties and Distances of Type II-Plateau Supernovae: SNe 2005cs and 2006bp
• Nonparametric Reconstruction of the Dark Energy Equation of State
• Expansion History with Decaying Vacuum: A Complete Cosmological Scenario
• Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion
• Constraining Dark Matter-Neutrino Interactions using the CMB and Large-Scale Structure
• A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
• The Angular Momentum Content of Dwarf Galaxies: New Challenges for the Theory of Galaxy Formation
• Hints of dynamical vacuum energy in the expanding Universe
• Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem
• 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
• Source-position transformation -- an approximate invariance in strong gravitational lensing
• Type Ia Supernovae, Evolution, and the Cosmological Constant
• Cosmic Birefringence from Planck Data Release 4
• Absolute-Magnitude Distributions of Supernovae
• Interacting models may be key to solve the cosmic coincidence problem
• Dynamical vacuum energy in the expanding Universe confronted with observations: a dedicated study
• Possible signals of vacuum dynamics in the Universe
• The ALP miracle: unified inflaton and dark matter
• Evidence for dark matter interactions in cosmological precision data?
• Search for Screened Interactions Associated with Dark Energy Below the 100 $\mu \mathrm{m}$ Length Scale
• 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
• Light-cone averaging in cosmology: formalism and applications
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• Non-parametric spatial curvature inference using late-universe cosmological probes
• Is the Jeffreys' scale a reliable tool for Bayesian model comparison in cosmology?
• The EDGES 21 cm Anomaly and Properties of Dark Matter
• A combined analysis of the $H_0$ late time direct measurements and the impact on the Dark Energy sector
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Complete Cosmic History with a dynamical Lambda(H) term
• Median statistics and the Hubble constant
• Neutrino mass in cosmology: status and prospects
• Early modified gravity in light of the $H_0$ tension and LSS data
• No large-angle correlations on the non-Galactic microwave sky
• Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies
• The Planes of Satellite Galaxies Problem, Suggested Solutions, and Open Questions
• LOSS Revisited - II: The relative rates of different types of supernovae vary between low- and high-mass galaxies
• A measurement of the Hubble constant from Type II supernovae
• Relaxing cosmological tensions with a sign switching cosmological constant
• Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension
• Dark energy from the string axiverse
• A rapid transition of $G_{\mathrm{eff}}$ at $z_t\simeq 0.01$ as a solution of the Hubble and growth tensions
• Neutrino cosmology and Planck
• Cosmological bounds on dark matter-neutrino interactions
• KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
• The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789
• The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy
• An improved model-independent assessment of the late-time cosmic expansion
• The dark matter halos of dwarf galaxies: a challenge for the LCDM paradigm?
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Unified framework for Early Dark Energy from $\alpha$-attractors
• New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• A tale of two modes: Neutrino free-streaming in the early universe
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• The CatWISE Preliminary Catalog: Motions from $WISE$ and $NEOWISE$ Data
• Low Scale Unification, Newton's Law and Extra Dimensions
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• A Detailed Description of the CamSpec Likelihood Pipeline and a Reanalysis of the Planck High Frequency Maps
• The Megamaser Cosmology Project: I. VLBI observations of UGC 3789
• Determining the Hubble constant from Hubble parameter measurements
• Modeling Angular-Momentum History in Dark-Matter Halos
• Stringent Limit on Primordial Magnetic Fields from the Cosmic Microwave Background Radiation
• Progress on Cosmological Magnetic Fields
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• Big Bang Nucleosynthesis with Long Lived Charged Massive Particles
• Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey
• The Allegro gravitational wave detector: Data acquisition and analysis
• Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses
• The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators
• Model-independent reconstruction of $f(T)$ gravity from Gaussian Processes
• High redshift radio galaxies and divergence from the CMB dipole
• Addressing the circularity problem in the $E_{\text{p}}-E_{\text{iso}}$ correlation of Gamma-Ray Bursts
• Converting non-relativistic dark matter to radiation
• Beyond $\Lambda$CDM with Low and High Redshift Data: Implications for Dark Energy
• Evolution of dark energy reconstructed from the latest observations
• Constraints from thermal Sunyaev-Zeldovich cluster counts and power spectrum combined with CMB
• Probing the Cosmological Principle in the counts of radio galaxies at different frequencies
• A larger value for $H_0$ by an evolving gravitational constant
• Observational Challenges for the Standard FLRW Model
• A model-independent determination of the Hubble constant from lensed quasars and supernovae using Gaussian process regression
• Should Type Ia Supernova Distances be Corrected for their Local Environments?
• Alleviating the $H_0$ and ${\sigma }_8$ anomalies with a decaying dark matter model
• Type IIP Supernovae as Cosmological Probes: A SEAM Distance to SN 1999em
• Interacting neutrinos in cosmology: exact description and constraints
• The constant density region of the dark halos of spiral galaxies
• Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
• Thermal Friction as a Solution to the Hubble Tension
• Gamma-ray Burst Cosmology
• Brans-Dicke gravity with a cosmological constant smoothes out $\Lambda$CDM tensions
• Gas-Rich Mergers in LCDM: Disk Survivability and the Baryonic Assembly of Galaxies
• The cosmological bulk flow: consistency with $\Lambda$CDM and $z\approx 0$ constraints on ${\sigma }_8$ and $\gamma$
• Interacting Quintessence, Cosmic Acceleration and the Coincidence Problem
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Revisiting the NVSS number count dipole
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release
• The Swampland Conjecture and F-term Axion Monodromy Inflation
• Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations
• LITTLE THINGS in 3D: robust determination of the circular velocity of dwarf irregular galaxies
• The 6dF Galaxy Velocity Survey: Cosmological constraints from the velocity power spectrum
• Determining the Hubble Constant from the Gravitational Lens PG 1115+080
• Constraints on the interacting vacuum -- geodesic CDM scenario
• Using The Baryonic Tully-Fisher Relation to Measure $H_o$
• Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipoles
• Is the Universe odd?
• Solving the small-scale structure puzzles with dissipative dark matter
• The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• Behavior of the Newtonian potential for ghost-free gravity and singularity-free gravity
• Too Big To Fail in Light of Gaia
• A Compendium of Chameleon Constraints
• Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
• Theoretical Physics Implications of Gravitational Wave Observation with Future Detectors
• A Sudden Gravitational Transition
• CMB temperature and polarisation pseudo-Cl estimators and covariances
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• Is there Correlation between Fine Structure and Dark Energy Cosmic Dipoles?
• Reconciling Planck results with low redshift astronomical measurements
• Velocity anti-correlation of diametrically opposed galaxy satellites in the low redshift universe
• The UVES Large Program for Testing Fundamental Physics: I Bounds on a change in alpha towards quasar HE 2217-2818
• Superrenormalizable gauge and gravitational theories
• Stellar Mixing and the Primordial Lithium Abundance
• Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$
• Neutrinos help reconcile Planck measurements with both Early and Local Universe
• Pseudoscalar - sterile neutrino interactions: reconciling the cosmos with neutrino oscillations
• Interacting models of soft coincidence
• Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model
• Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
• Generalizing the running vacuum energy model and comparing with the entropic-force models
• Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?
• M31 Satellite Masses Compared to LCDM Subhaloes
• Running vacuum against the $H_0$ and ${\sigma }_8$ tensions
• Modified gravity as an alternative for Lambda-CDM cosmology
• Can luminosity distance measurements probe the equation of state of dark energy
• Inferring the Age of the Universe with Globular Clusters
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies
• Head-on collision of ultrarelativistic particles in ghost-free theories of gravity
• Renormalizing the vacuum energy in cosmological spacetime: implications for the cosmological constant problem
• Sample variance in the local measurements of the Hubble constant
• Null tests of the cosmological constant using supernovae
• The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
• Testing modified gravity with Planck: the case of coupled dark energy
• The emptiness of voids: yet another over-abundance problem for the LCDM model
• Calibrating the cosmic distance scale ladder: the role of the sound horizon scale and the local expansion rate as distance anchors
• The Hubble sequence: just a vestige of merger events?
• Updated constraints on massive neutrino self-interactions from cosmology in light of the $H_0$ tension
• How early is early dark energy?
• Are peculiar velocity surveys competitive as a cosmological probe?
• Local Voids as the Origin of Large-angle Cosmic Microwave Background Anomalies: The Effect of a Cosmological Constant
• The Cosmological Constant Problem and Running Vacuum in the Expanding Universe
• Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
• Analyzing the $H_0$ tension in $F(R)$ gravity models
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• Modified Gravity Makes Galaxies Brighter
• A new method to build the (inverse) distance ladder
• Decaying dark matter and the tension in ${\sigma }_8$
• The $L-\sigma$ relation for massive bursts of star formation
• The significance of the integrated Sachs-Wolfe effect revisited
• Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
• Cosmography and flat $\Lambda$CDM tensions at high redshift
• Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension
• A $w-M$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension
• Interacting radiation after Planck and its implications for the Hubble Tension
• Density perturbations for running vacuum: a successful approach to structure formation and to the ${\sigma }_8$-tension
• A Determination of H_0 with the CLASS Gravitational Lens B1608+656: I. Time Delay Measurements with the VLA
• Primordial nucleosynthesis
• Field theoretic interpretations of interacting dark energy scenarios and recent observations
• Implications of a transition in the dark energy equation of state for the $H_0$ and ${\sigma }_8$ tensions
• Partially Acoustic Dark Matter, Interacting Dark Radiation, and Large Scale Structure
• The mass discrepancy acceleration relation in a $\Lambda$CDM context
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Negative cosmological constant in the dark sector?
• Statistical Study of Gamma-Ray Bursts with a Plateau Phase in the X-ray Afterglow
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
• Warm dark matter does not do better than cold dark matter in solving small-scale inconsistencies
• de Sitter Swampland, $H_0$ tension & observation
• Cosmological parameter analyses using transversal BAO data
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Effects of Massive Neutrinos on the Large-Scale Structure of the Universe
• The Impact of an Extra Background of Relativistic Particles on the Cosmological Parameters derived from Microwave Background Anisotropies
• Cosmic dissonance: new physics or systematics behind a short sound horizon?
• BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• Growth of matter perturbations in non-minimal teleparallel dark energy
• Big Bang nucleosynthesis revisited via Trojan Horse Method measurements
• The Megamaser Cosmology Project VIII. A Geometric Distance to NGC 5765b
• Seeing the First Supernovae at the Edge of the Universe with JWST
• Interacting Dark Energy in a closed universe
• A Step in Understanding the Hubble Tension
• Early-type Host Galaxies of Type Ia Supernovae. II. Evidence for Luminosity Evolution in Supernova Cosmology
• New constraints on time-dependent variations of fundamental constants using Planck data
• Quantifying the $S_8$ tension with the Redshift Space Distortion data set
• Dark matters on the scale of galaxies
• Dipole anisotropy in sky brightness and source count distribution in radio NVSS data
• Measuring dark energy with the $E_{\mathrm{iso}}-E_{\mathrm{p}}$ correlation of gamma-ray bursts using model-independent methods
• Gravitational waves from the Papaloizou-Pringle instability in black hole-torus systems
• An independent determination of the local Hubble constant
• Slope evolution of GRB correlations and cosmology
• First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release
• Constraints on decaying dark matter from the extragalactic gamma-ray background
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Solar Neutrino Constraints on the BBN Production of Li
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• Lack of large-angle TT correlations persists in WMAP and Planck
• Testing Screened Modified Gravity
• The low-mass end of the baryonic Tully-Fisher relation
• Dynamical dark energy or variable cosmological parameters?
• The core-cusp problem: a matter of perspective
• Asymmetric Dark Matter and Dark Radiation
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• Gaia EDR3 proper motions of Milky Way dwarfs I: 3D Motions and Orbits
• Large-scale alignments from WMAP and Planck
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Can f(R) Modified Gravity Theories Mimic a LCDM Cosmology?
• Photospheric Magnitude Diagrams for Type II Supernovae: A Promising Tool to Compute Distances
• Over-constrained Gravitational Lens Models and the Hubble Constant
• Cosmologies with a time dependent vacuum
• Relieving the $H_0$ tension with a new interacting dark energy model
• Swampland Distance Conjecture, Inflation and $\alpha$-attractors
• Dark matter component decaying after recombination: lensing constraints with Planck data
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• Cosmological model insensitivity of local $H_0$ from the Cepheid distance ladder
• Running vacuum in quantum field theory in curved spacetime: renormalizing ${\rho }_{vac}$ without $\sim m^4$ terms
• The High-$z$ Universe Confronts Warm Dark Matter: Galaxy Counts, Reionization and the Nature of Dark Matter
• Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
• The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data
• Detecting the integrated Sachs-Wolfe effect with stacked voids
• Non-extensive Statistics Solution to the Cosmological Lithium Problem
• Internal Robustness of Growth Rate data
• How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant
• Primordial black holes from long-range scalar forces and scalar radiative cooling
• Implication of the Hubble tension for the primordial Universe in light of recent cosmological data
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Cosmological Simulations of Decaying Dark Matter: Implications for Small-scale Structure of Dark Matter Halos
• Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation
• The Megamaser Cosmology Project. V. An Angular Diameter Distance to NGC 6264 at 140 Mpc
• The Past, Present and Future of the Resonant-Mass Gravitational Wave Detectors
• Frequency-Dependent Responses in 3rd Generation Gravitational-Wave Detectors
• New Early Dark Energy is compatible with current LSS data
• Majoron Dark Matter and Constraints on the Majoron-Neutrino Coupling
• Hints of a Local Matter Underdensity or Modified Gravity in the Low $z$ Pantheon data
• Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• Evidence for Emergent Dark Energy
• Sterile Neutrinos with Secret Interactions - Lasting Friendship with Cosmology
• Dark sector interaction and the supernova absolute magnitude tension
• All-inclusive interacting dark sector cosmologies
• Model-independent test of the FLRW metric, the flatness of the Universe, and non-local measurement of $H_0{r}_{\mathrm{d}}$
• The Atacama Cosmology Telescope: Constraints on Cosmic Birefringence
• A massive blow for $\Lambda$CDM $-$ the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology
• Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
• Emerging spatial curvature can resolve the tension between high-redshift CMB and low-redshift distance ladder measurements of the Hubble constant
• The ALP miracle revisited
• Three Ancient Halo Subgiants: Precise Parallaxes, Compositions, Ages, and Implications for Globular Clusters
• The 2-degree Field Lensing Survey: design and clustering measurements
• Assessing tension metrics with Dark Energy Survey and Planck data
• The Megamaser Cosmology Project. VI. Observations of NGC 6323
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Reconciling $H_0$ tension in a six parameter space?
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Late time approaches to the Hubble tension deforming $H(z)$, worsen the growth tension
• Can dark energy be dynamical?
• Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Cosmological Hints of Modified Gravity ?
• Kilobyte Cosmic Birefringence from ALP Domain Walls
• Interacting Dark Energy and the Cosmic Coincidence Problem
• Reconstructing the dark sector interaction with LISA
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Testing GRBs as Standard Candles
• Neutrino Mass Bounds in the era of Tension Cosmology
• Constraining interacting dark energy models with latest cosmological observations
• Measurements of $H_0$ in modified gravity theories: The role of lensed quasars in the late-time Universe
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from counts and stacked weak-lensing
• Gravitational and Chiral Anomalies in the Running Vacuum Universe and Matter-Antimatter Asymmetry
• Cosmological Models and Gamma-Ray Bursts Calibrated by Using Pade Method
• Limits on the dependence of the fine-structure constant on gravitational potential from white-dwarf spectra
• Chameleon Field Theories
• Cosmological constraints on neutrino self-interactions with a light mediator
• The XXL Survey XXV. Cosmological analysis of the C1 cluster number counts
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• $H_0$ Tension, Swampland Conjectures and the Epoch of Fading Dark Matter
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM
• WMAP Constraints on Decaying Cold Dark Matter
• Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
• Is cosmic acceleration proven by local cosmological probes?
• Revealing the Nature of Dark Energy Using Bayesian Evidence
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• Cosmological constant, renormalization group and Planck scale physics
• Dark Sector to Restore Cosmological Concordance
• Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
• Parallax Beyond a Kiloparsec from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope
• Revisiting Neutrino Self-Interaction Constraints from $Z$ and $\tau$ decays
• Coupled quintessence with a $\Lambda$CDM background: removing the ${\sigma }_8$ tension
• New constraints on Parity Symmetry from a re-analysis of the WMAP-7 low resolution power spectra
• What can Machine Learning tell us about the background expansion of the Universe?
• Determining Model-independent $H_0$ and Consistency Tests
• Broken Isotropy from a Linear Modulation of the Primordial Perturbations
• Euclid Assessment Study Report for the ESA Cosmic Visions
• Detection of isolated population III stars with the James Webb Space Telescope
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• H0 tension or T0 tension?
• Constraining cosmological parameters by Gamma Ray Burst X - ray afterglow lightcurves
• Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
• A Near-Infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance Ladder
• Resonant Destruction as a Possible Solution to the Cosmological Lithium Problem
• Type Ia supernovae, standardisable candles, and gravity
• The UVES Large Program for testing fundamental physics - III. Constraints on the fine-structure constant from 3 telescopes
• Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure
• Standardizing Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Early mass varying neutrino dark energy: Nugget formation and Hubble anomaly
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• The $H_0$ tension: $\Delta G_N$ vs. $\Delta N_{\mathrm{eff}}$
• No Slip Gravity
• Gamma Ray Burst afterglow and prompt-afterglow relations: an overview
• Cosmic microwave background anomalies in an open universe
• More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
• Residual Non-Abelian Dark Matter and Dark Radiation
• The Hubble tension and a renormalizable model of gauged neutrino self-interactions
• Hubble flow variance and the cosmic rest frame
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• The trouble beyond $H_0$ and the new cosmic triangles
• Theories of Dark Energy with Screening Mechanisms
• The local and distant Universe: stellar ages and $H_0$
• Observational constraints on the deceleration parameter in a tilted universe
• No-go guide for the Hubble tension : Late-time solutions
• The Hubble Tension Revisited: Additional Local Distance Ladder Uncertainties
• The Milky Way Cepheid Leavitt law based on Gaia DR2 parallaxes of companion stars and host open cluster populations
• Constraining the Dark Energy Equation of State with HII Galaxies
• The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation
• Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• Searching for Anisotropic Cosmic Birefringence with Polarization Data from SPTpol
• Addressing $H_0$ tension by means of VCDM
• Think Global, Act Local: The Influence of Environment Age and Host Mass on Type Ia Supernova Light Curves
• Soundness of Dark Energy properties
• Dark matter-radiation interactions: the structure of Milky Way satellite galaxies
• Late time transitions in the quintessence field and the $H_0$ tension
• KiDS+VIKING-450: Improved cosmological parameter constraints from redshift calibration with self-organising maps
• Running of the Spectral Index and Violation of the Consistency Relation Between Tensor and Scalar Spectra from trans-Planckian Physics
• Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies
• Cosmological constraints on multi-interacting dark matter
• The ACS Virgo Cluster Survey IV: Data Reduction Procedures for Surface Brightness Fluctuation Measurements with the Advanced Camera for Surveys
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• The Limits of Extended Quintessence
• Test of the cosmic evolution using Gaussian processes
• The lensing and temperature imprints of voids on the Cosmic Microwave Background
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Falsifying $\Lambda$CDM: Model-independent tests of the concordance model with eBOSS DR14Q and Pantheon
• HII Galaxies as deep cosmological probes
• Disks in the sky: A reassessment of the WMAP "cold spot"
• Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
• Neutrino Self-Interactions and Double Beta Decay
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• Stellar Oscillations in Modified Gravity
• Tests of redshift-space distortions models in configuration space for the analysis of the BOSS final data release
• Looking for interactions in the cosmological dark sector
• New quantum aspects of a vacuum-dominated universe
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• $T_0$ censorship of early dark energy and AdS vacua
• Quasars as standard candles II: The non linear relation between UV and X-ray emission at high redshifts
• Observational Constraints on Oscillating Dark-Energy Parametrizations
• Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?
• Effect of quark-mass variation on big bang nucleosynthesis
• A Multi-component Matched Filter Cluster Confirmation Tool for eROSITA: Initial Application to the RASS and DES-SV Datasets
• New Nuclear Physics for Big Bang Nucleosynthesis
• Model-independent reconstruction of the linear anisotropic stress $\eta$
• Relaxing the ${\sigma }_8$-tension through running vacuum in the Universe
• The Early Dark Sector, the Hubble Tension, and the Swampland
• Constraining neutrino mass with weak lensing Minkowski Functionals
• The stacked ISW signal of rare superstructures in ΛCDM
• Can a supervoid explain the Cold Spot?
• Equation of State of Oscillating Brans-Dicke Scalar and Extra Dimensions
• The Infrared Surface Brightness Fluctuation Hubble Constant
• Unveiling Chameleons in Tests of Gravitational Inverse-Square Law
• Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
• A low CMB variance in the WMAP data
• COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses II. SDSS J0924+0219: the redshift of the lensing galaxy, the quasar spectral variability and the Einstein rings
• Gravitational lensing model degeneracies: Is steepness all-important?
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Independent Cosmological Constraints from high-z HII Galaxies
• The baryonic Tully-Fisher relation and galactic outflows
• Addressing the cosmological $H_0$ tension by the Heisenberg uncertainty
• Conjoined constraints on modified gravity from the expansion history and cosmic growth
• Constraining fundamental constant evolution with HI and OH lines
• Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
• Concordance cosmology without dark energy
• Constraining dark energy with gamma-ray bursts
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Neutrino-Assisted Early Dark Energy: Theory and Cosmology
• Distances from Surface Brightness Fluctuations
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• Parallax of Galactic Cepheids from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope: The Case of SS Canis Majoris
• Model independent inference of the expansion history and implications for the growth of structure
• The distribution of mass components in simulated disc galaxies
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• A Critique of Holographic Dark Energy
• Towards a Precision Cosmology from Starburst Galaxies at z>2
• Can scale-dependent cosmology alleviate the $H_0$ tension?
• Spherically symmetric static solutions in a non-local infrared modification of General Relativity
• Quantum Stability of Chameleon Field Theories
• The Hubble constant from eight time-delay galaxy lenses
• CMB Maximum Temperature Asymmetry Axis: Alignment with Other Cosmic Asymmetries
• Large-Scale Cosmic Shear Measurements
• A search for sterile neutrinos with the latest cosmological observations
• Hot New Early Dark Energy
• Constraining Teleparallel Gravity through Gaussian Processes
• Self-interacting inelastic dark matter: A viable solution to the small scale structure problems
• The Cosmophenomenology of Axionic Dark Radiation
• Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
• HICOSMO - Cosmology with a complete sample of galaxy clusters: II. Cosmological results
• Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
• AIC and BIC for cosmological interacting scenarios
• Self-interacting neutrinos: solution to Hubble tension versus experimental constraints
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• Resolving the $H_0$ tension with diffusion
• Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State
• Measurements of the Hubble constant and cosmic curvature with quasars: ultra-compact radio structure and strong gravitational lensing
• Large-Angle Correlations in the Cosmic Microwave Background
• Galaxy and Mass Assembly (GAMA): Redshift Space Distortions from the Clipped Galaxy Field
• Environmental Dependence of Type Ia Supernova Luminosities from a Sample without a Local-Global Difference in Host Star Formation
• Big Bang Nucleosynthesis constraints on sterile neutrino and lepton asymmetry of the Universe
• HST Proper Motions of NGC 147 and NGC 185: Orbital Histories and Test of Dynamically Coherent Andromeda Satellite Plane
• Can Non-standard Recombination Resolve the Hubble Tension?
• New cosmological bounds on hot relics: Axions $\&$ Neutrinos
• A Strategy to Measure the Dark Energy Equation of State using the HII galaxy Hubble Relation & X-ray AGN Clustering: Preliminary Results
• Constraining the Cosmology of the Phantom Brane using Distance Measures
• Cosmological Horizons, Uncertainty Principle and Maximum Length Quantum Mechanics
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Constraining dark matter-neutrino interactions with IceCube-170922A
• Quantum Anomalies in String-Inspired Running Vacuum Universe: Inflation and Axion Dark Matter
• Cosmological constant vis-a-vis dynamical vacuum: bold challenging the $\Lambda$CDM
• Warm Decaying Dark Matter and the Hubble Tension
• The Linear Growth of Structure in the R_h=ct Universe
• The Road to Precision Cosmology
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Cosmic bulk flows on 50 {h}^{-1}Mpc scales: A Bayesian hyper-parameter method and multishells likelihood analysis
• Chameleon Dark Energy
• Gaussian processes reconstruction of dark energy from observational data
• Stringy-Running-Vacuum-Model Inflation: from primordial Gravitational Waves and stiff Axion Matter to Dynamical Dark Energy
• 2MTF IV. A bulk flow measurement of the local Universe
• The resilience of the Etherington-Hubble relation
• Gaussian processes reconstruction of modified gravitational wave propagation
• Improved constraints on the dark energy equation of state using Gaussian processes
• Dark Energy, $H_0$ and Weak Gravity Conjecture
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Cosmological bounds on dark matter-photon coupling
• Measuring the Properties of Dark Energy with Photometrically Classified Pan-STARRS Supernovae. I. Systematic Uncertainty from Core-Collapse Supernova Contamination
• A comprehensive overview of the Cold Spot
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Site-selection criteria for the Einstein Telescope
• An analysis of the $H_0$ tension problem in a universe with a viscous dark fluid
• Late-time decaying dark matter: constraints and implications for the $H_0$-tension
• Sterile neutrino self-interactions: $H_0$ tension and short-baseline anomalies
• Simple-graduated dark energy and spatial curvature
• Cosmological Constraint on ${\Omega }_m$ and ${\sigma }_8$ from Cluster Abundances using the $GalWCat19$ Optical-Spectroscopic SDSS Catalog
• Solving the curvature and Hubble parameter inconsistencies through structure formation-induced curvature
• Parity Asymmetry in the CMBR Temperature Power Spectrum
• Testing the effect of $H_0$ on $f{\sigma }_8$ tension using a Gaussian Process method
• Hints for a gravitational constant transition in Tully-Fisher data
• Inflationary physics and transplanckian conjecture in the Stringy Running-Vacuum-Model: from the phantom vacuum to the true vacuum
• Minimal length, maximal momentum and the entropic force law
• Is there really a Hubble tension?
• Planck 2015 constraints on spatially-flat dynamical dark energy models
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• Ultralight Scalar Decay and the Hubble Tension
• A Hubble diagram from Type II Supernovae based solely on photometry: the Photometric-Colour Method
• Testing the Mutual Consistency of the Pantheon and SDSS/eBOSS BAO Data Sets with Gaussian Processes
• Can Early Dark Energy Explain EDGES?
• Acceleration of the universe, vacuum metamorphosis, and the large-time asymptotic form of the heat kernel
• Hidden Charged Dark Matter and Chiral Dark Radiation
• Shedding light on the small-scale crisis with CMB spectral distortions
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Constraining Fundamental Physics with Future CMB Experiments
• Hints of Modified Gravity in Cosmos and in the Lab?
• Screened fifth forces lower the TRGB-calibrated Hubble constant too
• Hubble diagram at higher redshifts: Model independent calibration of quasars
• 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
• Latest astronomical constraints on some nonlinear parametric dark energy models
• Sub-millimeter Spatial Oscillations of Newton's Constant: Theoretical Models and Laboratory Tests
• Post-Newtonian limit of Teleparallel Horndeski gravity
• The HII Galaxy Hubble Diagram Strongly Favors $R_{\mathrm{h}}=ct$ over $\Lambda$CDM
• Dark Radiation or Warm Dark Matter from long lived particle decays in the light of Planck
• Modelling and testing the equation of state for (Early) dark energy
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• The First Billion Years of a Warm Dark Matter Universe
• Bayesian Evidence against Harrison-Zel'dovich spectrum in tension cosmology
• Primordial nucleosynthesis with varying fundamental constants: Improved constraints and a possible solution to the Lithium problem
• Cosmological Effects of Radion Oscillations
• A loophole to the universal photon spectrum in electromagnetic cascades: application to the "cosmological lithium problem"
• Search for new resonant states in 10C and 11C and their impact on the cosmological lithium problem
• Multi-interacting dark energy and its cosmological implications
• Updated constraints on decaying cold dark matter
• Probing Axion-like Particles via CMB Polarization
• Axions and the Galactic Angular Momentum Distribution
• A measurement of the Hubble constant using galaxy redshift surveys
• Gravity in the infrared and effective nonlocal models
• On the Tensor/Scalar Ratio in Inflation with UV Cutoff
• Variability and the X-ray/UV ratio of Active Galactic Nuclei
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• The Baryonic Tully Fisher Relation
• Gravitational Lens Time Delays in CDM
• Self-interacting dark matter from late decays and the $H_0$ tension
• Constraints on modified gravity from the observed X-ray luminosity function of galaxy clusters
• The full Boltzmann hierarchy for dark matter-massive neutrino interactions
• Cosmological test using the Hubble diagram of high-z quasars
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• Planck CMB Anomalies: Astrophysical and Cosmological Secondary Effects and the Curse of Masking
• Dynamical Dark sectors and Neutrino masses and abundances
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Brane world corrections to Newton's law
• Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing
• The Axiverse Extended: Vacuum Destabilisation, Early Dark Energy and Cosmological Collapse
• The Vast Polar Structure of the Milky Way Attains New Members
• An upper limit to the variation in the fundamental constants at redshift z = 5.2
• Sterile neutrinos with pseudoscalar self-interactions and cosmology
• Consistency of the local Hubble constant with the cosmic microwave background
• Time Crystals from Minimum Time Uncertainty
• Possibility of realizing weak gravity in redshift space distortion measurements
• Covariance of CMB anomalies
• Searching for a dipole modulation in the large-scale structure of the Universe
• Dark energy interactions near the galactic centre
• The part and the whole: voids, supervoids, and their ISW imprint
• Model-independent cosmological constraints from growth and expansion
• Dark matter component decaying after recombination: Sensitivity to BAO and RSD probes
• Reconstructing Horndeski theories from phenomenological modified gravity and dark energy models on cosmological scales
• Measurement of the expansion rate of the Universe from γ-ray attenuation
• Measuring the Hubble constant with black sirens
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Hot New Early Dark Energy: Towards a Unified Dark Sector of Neutrinos, Dark Energy and Dark Matter
• A light particle solution to the cosmic lithium problem
• A new era of fine structure constant measurements at high redshift
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• Cosmological distance indicators
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• Cannibal Dark Matter and Large Scale Structure
• A large disparity in cosmic reference frames determined from the sky distributions of radio sources and the microwave background radiation
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• Testing dynamical vacuum models with CMB power spectrum from Planck
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Gas dynamics in dwarf galaxies as testbeds for dark matter and galaxy evolution
• A dipole anisotropy of galaxy distribution: Does the CMB rest-frame exist in the local universe?
• Detection strategies for the first supernovae with JWST
• Power Asymmetries in the Cosmic Microwave Background Temperature and Polarization patterns
• Friction in Gravitational Waves: a test for early-time modified gravity
• Cosmological inference from standard sirens without redshift measurements
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Unbiased clustering estimate with VIPERS slit assignment
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Large-Angle CMB Suppression and Polarization Predictions
• Massive photons from Super and Lorentz symmetry breaking
• Is the Hubble diagram of quasars in tension with concordance cosmology?
• Over-constrained Models of Time Delay Lenses Redux: How the Angular Tail Wags the Radial Dog
• The integrated Sachs-Wolfe effect in the AvERA cosmology
• Six Puzzles for LCDM Cosmology
• Axi-Higgs Cosmology
• Implications of the Cosmic Birefringence Measurement for the Axion Dark Matter Search
• The first simultaneous measurement of Hubble constant and post-Newtonian parameter from Time-Delay Strong Lensing
• Minimally entangled typical thermal states versus matrix product purifications for the simulation of equilibrium states and time evolution
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
• Thermonuclear reaction rates and primordial nucleosynthesis
• Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
• Lensing-like tensions in the Planck legacy release
• The Chandra view of the relation between X-ray and UV emission in quasars
• The Dark UNiverse Explorer (DUNE): Proposal to ESA's Cosmic Vision
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Hubble tension vs two flows
• Reconstruction of the HII Galaxy Hubble Diagram using Gaussian Processes
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• Quintessence Axion Dark Energy and a Solution to the Hubble Tension
• Small-scale clumping at recombination and the Hubble tension
• Testing Einstein's gravity and dark energy with growth of matter perturbations: Indications for new Physics?
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• First measurement of the Hubble parameter from bright binary black hole GW190521
• A hint of matter underdensity at low $z$?
• Resolving Hubble Tension by Self-Interacting Neutrinos with Dirac Seesaw
• Reconstructing inflation in scalar-torsion $f(T,\varphi )$ gravity
• Big Bang Nucleosynthesis with an Inhomogeneous Primordial Magnetic Field Strength
• Chameleon field and the late time acceleration of the universe
• Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data
• SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
• A new coupled three-form dark energy model and implications for the $H_0$ tension
• No H_0 Assistance from Assisted Quintessence
• Reconstruction of the dark sectors' interaction: A model-independent inference and forecast from GW standard sirens
• The deceleration parameter in `tilted' Friedmann universes
• Testing dark energy after pre-recombination early dark energy
• Revised Big Bang Nucleosynthesis with long-lived negatively charged massive particles: updated recombination rates, primordial 9Be nucleosynthesis, and impact of new 6Li limits
• Accuracy of the growth index in the presence of dark energy perturbations
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• The size of our causal Universe
• Cosmology With Low-Redshift Observations: No Signal For New Physics
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Optical Surface Brightness Fluctuations of shell galaxies towards 100 Mpc
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Comprehensive Study of Neutrino-Dark Matter Mixed Damping
• Unexpected Topology of the Temperature Fluctuations in the Cosmic Microwave Background
• Microphysics of Early Dark Energy
• Consistency of Modified Gravity with a decreasing $G_{\mathrm{eff}}(z)$ in a $\Lambda$CDM background
• Proca in the sky
• Generalized LTB model with Inhomogeneous Isotropic Dark Energy: Observational Constraints
• On cosmological signatures of baryons-dark energy elastic couplings
• Perceiving the equation of state of Dark Energy while living in a Cold Spot
• Origin of Delta N_eff as a Result of an Interaction between Dark Radiation and Dark Matter
• Two-point Correlation Function of WMAP 9 year data
• Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
• The Hubble constant and new discoveries in cosmology
• Influence of the Bounds of the Hyperparameters on the Reconstruction of Hubble Constant with Gaussian Process
• Supersymmetry Breaking as a new source for the Generalized Uncertainty Principle
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• Reconstructing gravitational wave signals from binary black hole mergers with minimal assumptions
• Cosmological solutions to the Lithium problem: Big-bang nucleosynthesis with photon cooling, $X$-particle decay and a primordial magnetic field
• Wandering in the Lyman-alpha Forest: A Study of Dark Matter-Dark Radiation Interactions
• Photon sector analysis of Super and Lorentz symmetry breaking: effective photon mass, bi-refringence and dissipation
• Inflation Model Selection meets Dark Radiation
• Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra
• Neutrino Masses and Hubble Tension via a Majoron in MFV
• Determination of the Local Hubble Constant from Virgo Infall Using TRGB Distances
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Sources of $H_0$-tensions in dark energy scenarios
• Probing the Gravitational Dependence of the Fine-Structure Constant from Observations of White Dwarf Stars
• Evidence for cosmic acceleration with next-generation surveys: A model-independent approach
• Non-parametric reconstruction of interaction in the cosmic dark sector
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Inflation Wars: A New Hope
• Boosted Neutrinos and Relativistic Dark Particles as Messengers from Reheating
• The improved Amati correlations from Gaussian copula
• The $H_0$ Tension in Non-flat QCDM Cosmology
• Towards testing CMB anomalies using the kinetic and polarized Sunyaev Zel'dovich effects
• Directional dependence of LCDM cosmological parameters
• The homogeneity scale and the growth rate of cosmic structures
• Linear scale bounds on dark matter--dark radiation interactions and connection with the small scale crisis of cold dark matter
• Evidence for galaxy dynamics tracing background cosmology below the de Sitter scale of acceleration
• Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum
• Evaporating primordial black holes as varying dark energy
• Possible Hints of Sterile Neutrinos in Recent Measurements of the Hubble Parameter
• X-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance Simulations
• Constraints on Spatially Oscillating Sub-mm Forces from the Stanford Levitated Microsphere Experiment Data
• The dark side of the torsion: Dark Energy from propagating torsion
• Classification of Teleparallel Horndeski Cosmology via Noether Symmetries
• Can varying the gravitational constant alleviate the tensions ?
• Short Distance Physics of the Inflationary de Sitter Universe
• Growth of matter perturbations in the extended viscous dark energy models
• Constraints on inflation revisited: An analysis including the latest local measurement of the Hubble constant
• Hot thermal universe endowed with massive dark vector fields and the Hubble tension
• Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
• Does Quartessence Ease Tensions?
• The look-elsewhere effect from a unified Bayesian and frequentist perspective
• On Problems with Cosmography in Cosmic Dark Ages
• Debiasing Cosmic Gravitational Wave Sirens
• Can the cosmological "constant" run? - It may run
• Violation of statistical isotropy and homogeneity in the 21-cm power spectrum
• Constraining power of cosmological observables: blind redshift spots and optimal ranges
• Cosmology and the massive photon frequency shift in the Standard-Model Extension
• Defying the laws of Gravity I: model-independent reconstruction of the Universe expansion from growth data
• Measuring the Galactic Cosmic Ray Flux with the LISA Pathfinder Radiation Monitor
• Time Dependent Quark Masses and Big Bang Nucleosynthesis Revisited
• Gravitational transitions via the explicitly broken symmetron screening mechanism
• Generalized covariant prescriptions for averaging cosmological observables
• Degenerate Sub-keV Fermion Dark Matter from a Solution to the Hubble Tension
• A comment on power-law inflation with a dark radiation component
• Big Bang nucleosynthesis in scalar tensor gravity: the key problem of the ${}^7$Li abundance
• Using spatial curvature with HII galaxies and cosmic chronometers to explore the tension in $H_0$
• 21-cm observations and warm dark matter models
• Super-CMB fluctuations and the Hubble tension
• Torsion in string-inspired cosmologies and the universe dark sector
• Decaying dark matter, the $H_0$ tension, and the lithium problem
• Short distance modification of the quantum virial theorem
• Growth of matter overdensities in non-minimal torsion-matter coupling theories
• Phantom braneworld and the Hubble tension
• Cosmological constraints on non-adiabatic dark energy perturbations
• Well-tempered teleparallel Horndeski cosmology: a teleparallel variation to the cosmological constant problem
• The GUP and quantum Raychaudhuri equation
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Isolating the Lyman Alpha Forest BAO Anomaly
• Physical constraints on interacting dark energy models
• H_0 tension: clue to common nature of dark sector?
• Non-uniqueness in quasar absorption models and implications for measurements of the fine structure constant
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Newton potential in deSitter braneworld
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Easing cosmic tensions with an open and hotter universe
• The Hubble constant tension with next-generation galaxy surveys
• Unified dark sectors in scalar-torsion theories of gravity
• Peculiar motion of the solar system derived from a dipole anisotropy in the redshift distribution of distant quasars
• The Cosmological Constant as a Zero Action Boundary
• Redshift evolution of the Amati relation: calibrated results from the Hubble diagram of quasars at high redshifts
• TRGB distances to galaxies in front of the Virgo cluster
• The hemispherical asymmetry from a scale-dependent inflationary bispectrum
• When FIMPs Decay into Neutrinos: The $N_{\mathrm{eff}}$ Story
• Measuring the integrated Sachs-Wolfe effect from the low-density regions of the universe
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Surface Brightness Fluctuations as Primary and Secondary Distance Indicators
• The role of CMB spectral distortions in the Hubble tension: a proof of principle
• Faraday Rotation as a diagnostic of Galactic foreground contamination of CMB maps
• How rare is the Bullet Cluster (in a $\Lambda$CDM universe)?
• Optimal analysis of the CMB trispectrum
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Cosmic variance of $H_0$ in light of forthcoming high-redshift surveys
• Update constraints on neutrino mass and mass hierarchy in light of dark energy models
• North-South non-Gaussian asymmetry in PLANCK CMB maps
• Primordial Power Spectra of Cosmological Fluctuations with Generalized Uncertainty Principle and Maximum Length Quantum Mechanics
• Implications of a frame dependent dark energy for the spacetime metric, cosmography, and effective Hubble constant
• Could multiple voids explain the Cosmic Microwave Background Cold Spot anomaly?
• Hemispherical Anomaly from Asymmetric Initial States
• Future constraints on the gravitational slip with the mass profiles of galaxy clusters
• Dynamics in interacting scalar-torsion theory
• Early Modified Gravity: Implications for Cosmology
• Litmus Test for Cosmic Hemispherical Asymmetry in the Cosmic Microwave Background B-mode polarization
• eROSITA cluster cosmology forecasts: cluster temperature substructure bias
• Gaia EDR3 proper motions of Milky Way dwarfs. II: Velocities, Total Energy and Angular Momentum
• Shedding Light on Dark Matter and Neutrino Interactions from Cosmology
• Decay of multiple dark matter particles to dark radiation in different epochs does not alleviate the Hubble tension
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
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• A Model of Interacting Dark Matter and Dark Radiation for $H_0$ and ${\sigma }_8$ Tensions
• Can $f(R)$ gravity relieve $H_0$ and ${\sigma }_8$ tensions?
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• Measurement of Redshift Space Power Spectrum for BOSS galaxies and the Growth Rate at redshift 0.57
• Unbiased likelihood-free inference of the Hubble constant from light standard sirens
• Constraining Dark-Matter Ensembles with Supernova Data
• Cosmology from weak lensing alone and implications for the Hubble tension
• Can the Hubble tension be resolved by bulk viscosity?
• Breaking Be: a sterile neutrino solution to the cosmological lithium problem
• Emergent dark energy from unparticles
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• Model-independent constraints on Type Ia supernova light-curve hyper-parameters and reconstructions of the expansion history of the Universe
• Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
• The Spectrum of Dark Radiation as a Probe of Reheating
• Roles of ${}^7$Be$(n,p{)}^7$Li resonances in big bang nucleosynthesis with time-dependent quark mass and Li reduction by a heavy quark mass
• Frames of most uniform Hubble flow
• A null test of the Cosmological Principle with BAO measurements
• Reconstruction of late-time cosmology using Principal Component Analysis
• Inflationary universe in the presence of a minimal measurable length
• Gravitational wave constraints on the observable inflation
• Interacting Scalar Radiation and Dark Matter in Cosmology
• Dark Energy Detected with Supervoids and Superclusters
• Generating $\fnl$ at $\ell\lsim 60$
• Determining $H_0$ with the latest HII galaxy measurements
• Local properties of WMAP Cold Spot
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• Notes on the Missing Satellites Problem
• On the Evolution of Cosmological Type Ia Supernovae and the Gravitational Constant
• Using the Extragalactic Gamma-Ray Background to Constrain the Hubble Constant and Matter Density of the Universe
• The variance of the CMB temperature gradient: a new signature of a multiply connected Universe
• Gravitational Wave Astronomy
• Optical Observations of Type II Supernovae
• Explaining Excess Dipole in NVSS Data Using Superhorizon Perturbation
• Ultralight dark photon as a model for early universe dark matter
• Analysis of the apparent lack of power in the cosmic microwave background anisotropy at large angular scales
• A Two-point Diagnostic for the HII Galaxy Hubble Diagram
• Charged Dark Matter and the $H_0$ tension
• Cosmology of an Axion-Like Majoron
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• Strongly scale-dependent CMB dipolar asymmetry from super-curvature fluctuations
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Lifshitz cosmology: quantum vacuum and Hubble tension
• Measuring bulk motion of X-ray clusters via the kinematic Sunyaev-Zeldovich effect: summarizing the "dark flow" evidence and its implications
• Frequency variation for in vacuo photon propagation in the Standard-Model Extension
• Implications of the CMB power asymmetry for the early universe
• The ISW effect and the lack of large-angle CMB temperature correlations
• Cuspy dark matter density profiles in massive dwarf galaxies
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Early-Universe Model Building
• Interacting Dark Sectors in Anisotropic Universe: Observational Constraints and $H_0$ Tension
• Is there evidence for a hotter Universe?
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• Scale-dependent dipolar modulation and the quadrupole-octopole alignment in the CMB temperature
• Shan--Chen interacting vacuum cosmology
• The shape of CMB temperature and polarization peaks on the sphere
• Existence and Stability of Static Spherical Fluid Shells in a Schwarzschild-Rindler-anti-de Sitter Metric
• Early-time thermalization of cosmic components? A hint for solving cosmic tensions
• Resolving Hubble tension with the Milne model
• Weak gravity on a $\Lambda$CDM background
• Cosmological constraints with the Effective Fluid approach for Modified Gravity
• Late-time and Big Bang nucleosynthesis constraints for generic modify gravity surveys
• The effect of screening mechanisms on black hole binary inspiral waveforms
• Bayesian Reconstruction of Gravitational-wave Signals from Binary Black Holes with Nonzero Eccentricities
• No evidence for EDE from Planck data in extended scenarios
• Scale-dependent CMB power asymmetry from primordial speed of sound and a generalized $\delta$N formalism
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Testing the scale-dependent hemispherical asymmetry with the 21-cm power spectrum from the epoch of reionization
• Primordial anisotropies from cosmic strings during inflation
• A Solution to Lithium Problem by Long-Lived Stau
• Micro-orbits in a many-branes model and deviations from $1/r^2$ Newton's law
• Topology and the suppression of CMB large-angle correlations
• Constraining the magnetic field on white dwarf surfaces; Zeeman effects and fine structure constant variation
• Exact general solutions for cosmological scalar field evolution in a background-dominated expansion
• Modern Cosmology, an Amuse-Gueule
• An approach to cold dark matter deviation and the $H_0$ tension problem by using machine learning
• The cosmological lithium problem, varying constants and the $H_0$ tension
• Surface Tension: Accelerated Expansion, Coincidence Problem & Hubble Tension
• Gravitation And the Universe from large Scale-Structures: The GAUSS mission concept
• Statistical anisotropies in temperature and polarization fluctuations from a scale-dependent trispectrum
• The fate of Newton's law in brane-world scenarios
• The Hubble Constant in the Axi-Higgs Universe
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• Hubble Hullabaloo and String Cosmology
• Improved Cosmological Constraints from SDSS redMaPPer Clusters via X-ray Follow-up of a Complete Subsample of Systems
• Cluster Cosmology with the Velocity Distribution Function of the HeCS-SZ Sample
• Hemispherical Variance Anomaly and Reionization Optical Depth
• Effects of Massive Neutrinos and Dynamical Dark Energy on the Cluster Mass Function
• Scalar tachyonic instabilities in gravitational backgrounds: Existence and growth rate
• The Pantheon+ Analysis: Dependence of Cosmological Constraints on Photometric-Zeropoint Uncertainties of Supernova Surveys
• Transient weak gravity in scalar-tensor theories
• Polarizations of CMB and the Hubble tension
• Running vacuum interacting with dark matter or with running gravitational coupling. Phenomenological implications
• A Uniform Type Ia Supernova Distance Ladder with the Zwicky Transient Facility: Absolute Calibration Based on the Tip of the Red Giant Branch (TRGB) Method
• Interacting dark energy from redshift-space galaxy clustering

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• Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A${}^{\ast }$
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Is the Observable Universe Consistent with the Cosmological Principle?
• DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Rock 'n' Roll Solutions to the Hubble Tension
• Cosmology in $f(Q)$ gravity: A unified dynamical system analysis at background and perturbation levels
• Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• Restoring cosmological concordance with early dark energy and massive neutrinos?
• Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0{w}_a$CDM cosmological parameterization result
• Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• Dark energy in light of the early JWST observations: case for a negative cosmological constant?
• Anomalies in Physical Cosmology
• Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• Gravitational-wave imprints of compact and galactic-scale environments in extreme-mass-ratio binaries
• Evidence of a decreasing trend for the Hubble constant
• New constraints on interacting dark energy from DESI DR2 BAO observations
• The state of the dark energy equation of state circa 2023
• On the homogeneity of SnIa absolute magnitude in the Pantheon+ sample
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Omnipotent dark energy: A phenomenological answer to the Hubble tension
• Non-metricity with bounday terms: $f(Q,C)$ gravity and cosmology
• Late-time cosmology with phantom dark-energy in $f(Q)$ gravity
• Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the ${\sigma }_8$ and $H_0$ tensions
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• Revealing the effects of curvature on the cosmological models
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model
• Breakdown of the Newton-Einstein Standard Gravity at Low Acceleration in Internal Dynamics of Wide Binary Stars
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Model-independent cosmological inference post DESI DR1 BAO measurements
• Towards hybrid inflation with $n_s=1$ in light of Hubble tension and primordial gravitational waves
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• Equation of state of the running vacuum
• The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• Phantom matter: a challenging solution to the cosmological tensions
• Is the Harrison-Zel'dovich spectrum coming back? ACT preference for $n_s\sim 1$ and its discordance with Planck
• $S_8$ increases with effective redshift in $\Lambda$CDM cosmology
• Data reconstruction of the dynamical connection function in $f(Q)$ cosmology
• Constraints on modified gravity from the BOSS galaxy survey
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• Composite Dark Energy and the Cosmological Tensions
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• KiDS-1000: Cosmology with improved cosmic shear measurements
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• Is the dark energy equation of state parameter singular?
• Accelerating cosmological models in $f(Q)$ gravity and the phase space analysis
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• On the dynamics of a dark sector coupling
• The Mira Distance to M101 and a 4% Measurement of H0
• Early Dark Energy with Power-law F(R) Gravity
• Constraints on the transition redshift from the calibrated Gamma-ray Burst $E_{\mathrm{p}}$-$E_{\mathrm{iso}}$ correlation
• Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances
• Constraints on Primordial-black-hole Population and Cosmic Expansion History from GWTC-3
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Gamma ray burst constraints on cosmological models from the improved Amati correlation
• Cosmology with 6 parameters in the Stage-IV era: efficient marginalisation over nuisance parameters
• Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements
• Implications of the Cosmic Birefringence Measurement for the Axion Dark Matter Search
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Running vacuum in QFT in FLRW spacetime: The dynamics of ${\rho }_{\mathrm{vac}}(H)$ from the quantized matter fields
• Cosmological constraints on ${\Lambda }_{\mathrm{s}}$CDM scenario in a type II minimally modified gravity
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• An Effective Sign Switching Dark Energy: Lotka-Volterra Model of Two Interacting Fluids
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Cosmographic view on the $H_0$ and ${\sigma }_8$ tensions
• Measuring the reionization optical depth without large-scale CMB polarization
• An effective description of Laniakea: impact on cosmology and the local determination of the Hubble constant
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• Is the $w_0{w}_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Constraining spatial curvature with large-scale structure
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• A comprehensive numerical study on four categories of holographic dark energy models
• Inevitable manifestation of wiggles in the expansion of the late Universe
• From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
• Observational Constraints on Dark Energy Models with $\Lambda$ as an Equilibrium Point
• Exploring the Hubble tension with a late time Modified Gravity scenario
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• Testing $\Lambda$-Free f(Q) Cosmology
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• Interacting dark energy from the joint analysis of the power spectrum and bispectrum multipoles with the EFTofLSS
• Neural Network Reconstruction of $H^{\prime }(z)$ and its application in Teleparallel Gravity
• Phantom scalar-tensor models and cosmological tensions
• ${\Lambda }_{\mathrm{s}}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties
• Gravitational transitions via the explicitly broken symmetron screening mechanism
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Exploring the cosmological synergy between galaxy cluster and cosmic void number counts
• Towards a possible solution to the Hubble tension with Horndeski gravity
• New cosmological constraints on $f(T)$ gravity in light of full Planck-CMB and type Ia supernovae data
• Novel constraints on fifth forces and ultralight dark sector with asteroidal data
• Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter
• Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
• Observational Constraints on Dynamical Dark Energy Models
• Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
• Impact of the Hubble tension on the $r$-$n_s$ contour
• New late-time constraints on $f(R)$ gravity
• On de Sitter Spacetime and String Theory
• Observational test for $f(Q)$ gravity with weak gravitational lensing
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• Fractional Holographic Dark Energy
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Constraints on $f(Q)$ logarithmic model using gravitational wave standard sirens
• Exploring new physics in the late Universe's expansion through non-parametric inference
• Mapping the ${\Lambda }_{\mathrm{s}}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate
• Primordial Black Holes and Gravitational Waves in Multi-Axion-Chern-Simons Inflation
• Exploring the stability of $f(Q)$ cosmology near general relativity limit with different connections
• Consistency tests between SDSS and DESI BAO measurements
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Cosmological forecasts for future galaxy surveys with the linear point standard ruler: Toward consistent BAO analyses far from a fiducial cosmology
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Measuring Hubble constant in an anisotropic extension of $\Lambda$CDM model
• Running vacuum versus Holographic dark energy: a cosmographic comparison
• Key drivers of the preference for dynamic dark energy
• Equivalence of $f(Q)$ cosmology with quintom-like scenario: the phantom field as effective realization of the non-trivial connection
• Does DESI DR2 challenge $\Lambda$CDM paradigm ?
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Covariant cosmography: the observer-dependence of the Hubble parameter
• Hydrodynamical structure formation in Milgromian cosmology
• Neural network reconstruction of cosmology using the Pantheon compilation
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Alleviating $H_0$ tension in scalar-tensor and bi-scalar-tensor theories
• Joint reconstructions of growth and expansion histories from stage-IV surveys with minimal assumptions. II. Modified gravity and massive neutrinos
• Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample
• Cosmological Perturbation Theory in Metric-Affine Gravity
• Dark Stars Powered by Self-Interacting Dark Matter
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• Cosmological models in scale-independent energy-momentum squared gravity
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• A critical discussion on the $H_0$ tension
• 21cmFirstCLASS I. Cosmological tool for $\Lambda$CDM and beyond
• An exponential equation of state of dark energy in the light of 2018 CMB Planck data
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Holographic and Gravity-Thermodynamic Approaches in Entropic Cosmology: Bayesian Assessment using late-time Data
• Spatial curvature in coincident gauge $f(Q)$ cosmology
• Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
• Probing Cosmology with 92 Localized Fast Radio Bursts and DESI BAO
• Reconciling early dark energy with a Harrison-Zeldovich spectrum
• Stability of symmetric teleparallel scalar-tensor cosmologies with alternative connections
• Hubble tension in a nonminimally coupled curvature-matter gravity model
• Addressing Cosmological Tensions by Non-Local Gravity
• A novel model-marginalized cosmological bound on the QCD axion mass
• Cosmography of the Local Universe by Multipole Analysis of the Expansion Rate Fluctuation Field
• Stability of $f(Q,B)$ Gravity via Dynamical System Approach: a Comprehensive Bayesian Statistical Analysis
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• Early dark energy by dark Higgs, and axion-induced non-thermal trapping
• Observational bounds on extended minimal theories of massive gravity: New limits on the graviton mass
• Unexplored regions in teleparallel $f(T)$ gravity: Sign-changing dark energy density
• The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
• D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models
• Type Ia supernovae data with scalar-tensor gravity
• A comparison between axion-like and power law potentials in cosmological background
• Probing dark matter interactions with 21cm observations
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Testing Quintessence Axion Dark Energy with Recent Cosmological Results
• Cosmology in Minkowski space
• A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
• Spatial and orbital planes of the Milky Way satellites: unusual but consistent with $\Lambda$CDM
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• Phase-space analysis of dark energy models in non-minimally coupled theories of gravity
• New cosmological constraints on the evolution of dark matter energy density
• Neutrino mass tension or suppressed growth rate of matter perturbations?
• Testing scale-invariant inflation against cosmological data
• Discriminating power of milli-lensing observations for dark matter models
• In search of an interaction in the dark sector through Gaussian Process and ANN approaches
• A short survey of matter-antimatter evolution in the primordial universe
• Bayesian analysis of a Unified Dark Matter model with transition: can it alleviate the $H_0$ tension?
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations
• On the interacting dark energy scenarios $-$ the case for Hubble constant tension
• DESI constraints on $\alpha$-attractor inflationary models
• Generalized Uncertainty Principle mimicking dynamical Dark Energy: matter perturbations and gravitational wave data analysis
• Constraints on Cosmological Models from Quasars Calibrated with Type Ia Supernova by a Gaussian Process
• Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions
• Thin-wall vacuum decay in the presence of a compact dimension meets the $H_0$ and $S_8$ tensions
• Using machine learning to compress the matter transfer function $T(k)$
• Hubble tensions: a historical statistical analysis
• Torsion at different scales: from materials to the Universe
• Anisotropic universe with anisotropic dark energy
• Spatial Curvature and Thermodynamics
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Astrophysical and Cosmological Searches for Lorentz Invariance Violation
• Big bang nucleosynthesis and early dark energy in light of the EMPRESS $Y_p$ results and the $H_0$ tension
• Exploring departures from Schwarzschild black hole in $f(R)$ gravity
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• f(R) Gravity in an Ellipsoidal Universe
• Geometric and topological corrections to Schwarzschild black hole
• Does the fraction of dark matter diminish with early dark energy?
• Cosmological constraints of Palatini $f(\mathcal{R})$ gravity
• Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from MgII and CIV reverberation-mapped quasar data
• Minimal model dependent constraints on cosmological nuisance parameters and cosmic curvature from combinations of cosmological data
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Unveiling the Hubble Constant through Galaxy Cluster Gas Mass Fractions
• Linear matter density perturbations in the ${\Lambda }_{\mathrm{s}}$CDM model: Examining growth dynamics and addressing the $S_8$ tension
• Conformal Killing cosmology -- Geometry, dark sector, growth of structures, and big rip
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Testing the standardizability of, and deriving cosmological constraints from, a new Amati-correlated gamma-ray burst data compilation
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• A possible late-time transition of $M_B$ inferred via neural networks
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• Interacting phantom dark energy: new accelerating scaling attractors
• Reconstructing the growth index $\gamma$ with Gaussian Processes
• Universal scaling laws and density slope for dark matter haloes
• Narrowing down the Hubble tension to the first two rungs of distance ladders
• Do we need wavelets in the late Universe?
• Quintessential early dark energy
• Cosmographic analysis of sign-switching dark energy
• Variation of the fine structure constant in the light of recent helium abundance measurement
• Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
• Gravity- and temperature-driven phase transitions in a model for collapsed axionic condensates
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• Evaluating Lyman-$\alpha$ Constraints for General Dark-Matter Velocity Distributions: Multiple Scales and Cautionary Tales
• General parametrization for energy density of quintessence field
• Constraints on sterile neutrinos and the cosmological tensions
• Weak field and slow motion limits in energy-momentum powered gravity
• Constraining deviations from $\Lambda$CDM in the Hubble expansion rate
• Interacting Models of Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity
• ${\Lambda }_{\mathrm{s}}$CDM cosmology from a type-II minimally modified gravity
• Addressing the Hubble tension in Yukawa cosmology?
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• Unveiling Neutrino Halos with CMB Lensing
• Machine learning unveils the linear matter power spectrum of modified gravity
• Is there a dynamical tendency in H0 with late time measurements?
• Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes
• Galaxy-galaxy lensing data: $f(T)$ gravity challenges General Relativity
• Extended Uncertainty Principle: A Deeper Insight into the Hubble Tension?
• Effects of a local physics change on the SH0ES determination of $H_0$
• Quintessential Implications of the presence of AdS in the Dark Energy sector
• Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
• Reconstructing FHDE with Scalar and Gauge Fields
• Maximum entropy distributions of dark matter in $\Lambda$CDM cosmology
• Revisiting CPL with sign-switching density: To cross or not to cross the NECB
• Redshift drift in a universe with structure II: Light rays propagated through a Newtonian N-body simulation
• Coupled Quintessence scalar field model in light of observational datasets
• Exploring Alternative Cosmologies with the LSST: Simulated Forecasts and Current Observational Constraints
• Revisiting Friedmann-like cosmology with torsion: newest constraints from high-redshift observations
• Fireball baryogenesis from early structure formation due to Yukawa forces
• Effects of anisotropy in an anisotropic extension of $w$CDM model
• Measuring the matter fluctuations in the Local Universe with the ALFALFA catalog
• Fundamental Physics and Cosmology with TianQin
• Solution of the dark matter riddle within standard model physics: From black holes, galaxies and clusters to cosmology
• Dark energy with a shift-symmetric scalar field: obstacles, loophole hunting and dead ends
• Coupled scalar field cosmology with effects of curvature
• Exploring Modified Gravity: Constraints on the $\mu$ and $\Sigma$ Parametrization with WMAP, ACT, and SPT
• Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Low- and high-redshift H II starburst galaxies obey different luminosity-velocity dispersion relations
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Fitting of supernovae without dark energy
• Investigating the $w$CDM Model with Latest DESI BAO Observations
• Empirical Validation: Investigating the ${\Lambda }_s$CDM Model with new DESI BAO Observations
• The cosmological lithium problem
• Testing $f(T)$ Gravity with Cosmological Observations: Confronting the Hubble Tension and Implications for the Late-Time Universe
• Revisiting model-independent constraints on spatial curvature and cosmic ladders calibration: updated and forecast analyses
• Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude
• Can the sound horizon-free measurement of $H_0$ constrain early new physics?
• Non-parametric reconstructions of cosmic curvature: current constraints and forecasts
• 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
• On the Hubble expansion in a Big Bang quantum cosmology
• Clifford algebra Cl(0,6) approach to beyond the standard model and naturalness problems
• Baryogenesis: A Symmetry Breaking in the Primordial Universe Revisited
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Relativistic binary systems in scale-independent energy-momentum squared gravity
• Spatially Homogeneous Universes with Late-Time Anisotropy
• Thawing k-essence dark energy in the PAge space
• Late-Time Anisotropy Sourced by a 2-Form Field Non-Minimally Coupled to Cold Dark Matter
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• On exotic objects made of dark energy and dark matter: Mass-to-radius profiles and tidal Love numbers
• Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions
• Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity
• Non-parametric reconstruction of the fine structure constant with galaxy clusters
• Coherent Self-Interactions of Dark Matter in the Bullet Cluster
• Linking the $R_{K^{(\ast )}}$ anomalies to the Hubble tension via a single right-handed neutrino
• A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Measuring the speed of light with cosmological observations: current constraints and forecasts
• Resilience and implications of adiabatic CMB cooling
• Reconstructing the parameter space of non-analytical cosmological fixed points
• Enhancing Cosmological Model Selection with Interpretable Machine Learning
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• Thermal leptogenesis in anisotropic cosmology
• An Independent Measure of the Kinematic Dipole from SDSS
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Traversable wormholes in bi-metric gravity
• asimulation: Domain formation and impact on observables in resolved cosmological simulations of the (a)symmetron
• Impact of Low ell's on Large Scale Structure Anomalies
• A solution to the S8 tension through neutrino-dark matter interactions
• A new parametrization of Hubble function and Hubble tension
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• On Evidence for Elastic Interactions in the Dark Sector
• A test of invariance of dark matter halo surface density using multiwavelength mock galaxy catalogues
• Running vacuum and H^4-inflation
• On the convergence of cosmographic expansions in Lemaitre-Tolman-Bondi models
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Cosmological Evolution in Bimetric Gravity: Observational Constraints and LSS Signatures
• Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity
• Revisiting coupled CDM-massive neutrino perturbations in diverse cosmological backgrounds
• Angular correlations on causally-coherent inflationary horizons
• Teleparallel dark energy in a nonflat universe
• Tilted non-spatially-flat inflation
• Evidence for the dynamical dark energy with evolving Hubble constant
• Emergent universe: tensor perturbations within the CSL framework
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Fab-Four cosmography to tackle the Hubble tension
• Constraining Cosmology with Double-source-plane Strong Gravitational Lenses from the AGEL Survey
• Barrow holographic dark energy interacting model in the presence of radiation and matter
• Measuring the Hubble constant through the galaxy pairwise peculiar velocity
• Constructing Viable Interacting Dark Matter and Dark Energy Models: A Dynamical Systems Approach
• Inflation in non-local hybrid metric-Palatini gravity
• Sensitivity of the Global 21-cm Signal to Dark Matter-Baryon Scattering
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• The Impact of ${\Omega }_{m0}$ Prior Bias on Cosmological Parameter Estimation: Reconciling DESI DR2 BAO and Pantheon+ SNe Data Combination Results
• Special Issue on Modified Gravity Approaches to the Tensions of $\Lambda$CDM: Goals and Highlights
• On the origin of the BAOtr-DESI tension
• High-redshift Galaxies from JWST Observations in More Realistic Dark Matter Halo Models
• Kinematic Distortions of the High-Redshift Universe as Seen from Quasar Proper Motions
• Anisotropic power-law inflation for a generalized model of two scalar and two vector fields
• Conventionalism, cosmology and teleparallel gravity
• A test for the redshift dependence of ${\sigma }_8$ using $f{\sigma }_8$ measurements
• Star-Crossed Labours: Checking Consistency Between Current Supernovae Compilations
• Thermodynamics of the Primordial Universe
• Mimetic-$f(Q)$ gravity: cosmic reconstruction and energy conditions
• Friedmann cosmology with hyperfluids
• Can the NANOGrav observations constrain the geometry of the universe?
• Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results
• Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts
• Forecasting 21-cm power spectrum sensitivity to dark Matter-baryon scattering
• Testing the consistency of new Amati-correlated gamma-ray burst dataset cosmological constraints with those from better-established cosmological data
• The gravitational force field of proto-pancakes
• Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff
• Non-Parametric Analysis for the Dark Matter Density Evolution
• CURLING -- II. Improvement on the $H_0$ Inference from Pixelized Cluster Strong Lens Modeling
• Modified propagation of gravitational waves from the early radiation era
• Local Limit of Nonlocal Gravity: A Teleparallel Extension of General Relativity
• Effective field theory of coupled dark energy and dark matter
• Viability of general relativity and modified gravity cosmologies using high-redshift cosmic probes
• When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior
• Defrosting and Blast Freezing Dark Matter
• The model of the local Universe in the framework of the second-order perturbation theory
• DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS
• Testing Refracted Gravity with kinematics of galaxy clusters
• Kinetic recoupling of dark matter
• Characterizing the equivalence between dark energy and radiation using gamma-ray bursts
• Remarks on overestimating the effects of inhomogeneities on the Hubble constant
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• Clusternets: A deep learning approach to probe clustering dark energy
• Velocity dispersion of dark matter deficient ultra-diffuse galaxies: A case for modified gravity
• Consistent cosmological structure formation on all scales in relativistic extensions of MOND
• Constraints on cosmological parameters and CMB first acoustic peak in conformal Killing gravity
• Probing dark fluids and modified gravity with gravitational lensing
• Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• Covariant Predictions for Planck-Scale Features in Primordial Power Spectra
• Pantheon+ tomography and Hubble tension
• Unraveling the Hubble tension with warm inflation
• Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective
• Constraints on Tsallis cosmology using recent low and high redshift measurements
• Non-linear structure formation with elastic interactions in the dark sector
• Do JWST reionization (optical depth) puzzle, cosmological tensions, and CMB anomalies imply Harrison-Zel'dovich spectrum?
• Bending the web: exploring the impact of modified gravity on the density field and halo properties within the cosmic web
• ${\mathbf{\Omega }}_1{\mathbf{\Omega }}_2$-$\mathbf{\Lambda }$CDM: A promising phenomenological extension of the standard model of cosmology
• Anisotropic power-law inflation for the Sáez-Ballester theory non-minimally coupled to a vector field
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Matter Creation Cosmologies and Accelerated Expansion
• A mechanism to generate varying speed of light via Higgs-dilaton coupling: Theory and cosmological applications
• A Review on Resolving the Hubble Tension via Late-Universe Physics
• Homology reveals significant anisotropy in the cosmic microwave background
• Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data
• Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
• Distinguishing thermal histories of dark matter from structure formation
• Analysis of Pantheon+ supernova data suggests evidence of sign-changing pressure of the cosmological fluid
• Signature of $f\left(R\right)$ gravity via Lemaître-Tolman-Bondi inhomogeneous perturbations
• Detecting Relativistic Doppler by Multi-Tracing a Single Galaxy Population
• The dynamics of vacuum, gravity and matter: Implications on the fundamental constants
• Can an Extra Degree of Freedom in Scalar-Tensor Non-Metricity Gravity Account for the Evolution of the Universe?
• Ultra-light dark matter with non-canonical kinetics reopening the mass window
• Comparison of $\Lambda$CDM and $R_h=ct$ with updated galaxy cluster $f_{gas}$ measurements using Bayesian inference
• Galaxy cluster count cosmology with simulation-based inference
• Cosmology in $R^2$-gravity: Effects of a Higher Derivative Scalar Condensate Background
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Forecast cosmological constraints from the number counts of Gravitational Waves events
• Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: ${\Lambda }_{\mathrm{s}}$CDM versus $\Lambda$CDM
• Testing Lens Models of PLCK G165.7+67.0 Using Lensed SN H0pe
• Reheating constraints and the $H_0$ tension in Quintessential Inflation
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• Dynamical Shortcomings in the Generalized SU(2) Proca Theory: Challenges for Cosmic Acceleration
• DESI constraints on two-field quintessence with exponential potentials
• Crosschecking Cosmic Distances from DESI BAO and DES SNe
• Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
• Impact of Redshift Space Distortion on Persistent Homology of cosmic matter density field
• One-point Statistics in various cosmic environments in the presence of massive neutrinos
• New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
• Gas of thin tubes of massless scalar field as a possible model of unified dark fluid
• Cosmological observational tests in the JWST Era. I: angular size - redshift
• Cosmological effect of coherent oscillation of ultralight scalar fields in a multicomponent universe
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Is Dark Energy Increasing or Decreasing in the Late Universe?
• Effects of dynamical friction on perturbations for evolving dark energy
• A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter
• Measuring cosmic dipole with the GRB luminosity-time relation
• Thermodynamics of sign-switching dark energy models
• A semi-cosmographic approach to study cosmological evolution in phase space
• Theoretical filters for shift-symmetric Horndeski gravities
• Exploring Cosmological Implications of the Modified Raychaudhuri Equation in Non-Gravitating Vacuum Energy Theory
• The cosmological Mass Varying Neutrino model in the late universe
• Conformal Killing Gravity: New Constraints from DESI DR2 BAO datasets
• The peculiar case of the Viaggiu holographic dark energy
• Cosmological constraints on the big bang quantum cosmology model
• Towards a Machine Learning Solution for Hubble Tension: Physics-Informed Neural Network (PINN) Analysis of Tsallis Holographic Dark Energy in Presence of Neutrinos
• A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension
• Probing dynamical embeddings in a five-dimensional spacetime in light of DESI BAO
• Is it possible to separate baryonic from dark matter within the $\Lambda$-CDM formalism?
• Scalar perturbation and density contrast evolution in $f(Q,C)$ gravity
• Horndeski in motion
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Massive black hole binaries in LISA: constraining cosmological parameters at high redshifts
• A robust assessment of the local anisotropy of the Hubble constant
• Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx
• Cosmological Frequency Combs
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Testing the Anton-Schmidt dark energy model with the DESI DR2 measurements
• Cosmological perturbations on an averaged background
• Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values
• Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime
• Hermitian formulation for mass dimension one fermions: Flat and curved space-times
• Evolution of matter perturbations in the context of cosmic slowing down
• Safely simplifying redshift drift computations in inhomogeneous cosmologies: Insights from LTB Swiss-cheese models
• The averaging problem on the past null cone in inhomogeneous dust cosmologies
• Constraints on the Modified Emergent Dark Energy Model Using DESI DR2 BAO
• Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology
• Hubble's Law in Heavy Ion Collisions
• On the detection of stellar wakes in the Milky Way: a deep learning approach
• Viaggiu holographic dark energy in light of DESI DR2
• CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
• How Holographic is the Dark Energy? A Spline Nodal reconstruction approach
• Quasinormal Modes of Black holes in the generalized Schwarzschild-de Sitter solution of $f(R)$ gravity
• Matter-antimatter asymmetry in a rotating universe: Dirac spinors in axisymmetric Bianchi IX cosmology
• $S_8$ from peculiar velocities: agreement with Planck for Tully--Fisher and supernovae, tension for the fundamental plane
• Quasinormal modes of regular black holes surrounded by skewed dark matter distributions
• Bouncing Cosmologies in modified gravity with space time torsion
• On the True Significance of the Hubble Tension: A Bayesian Error Decomposition Accounting for Information Loss
• Current constraints on the minimally extended varying speed of light model through the cosmic distance duality relation
• Einstein, tea leaves, meandering rivers, and the origin of supermassive black holes in ekpyrotic universe
• Cosmology of Cubic Poincaré Gauge gravity
• Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI
• Cosmic acceleration driven by dark matter self-interactions: a phenomenological treatment
• Propagation of tensor perturbation in Horndeski-like gravity
• Globally Stable Dark Energy in $F(R)$ Gravity
• Extended datasamples under the lens of Brane World Theory
• Addressing Dipole Tension via Clustering in $\Lambda$CDM and beyond
• Detector induced anisotropies on the angular distribution of gravitational wave sources and opportunities of constraining horizon scale anisotropies
• Production of Primordial Gravitational Waves in Teleparallel Gravity
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Background dynamics and observational constraints of flat and non-flat $\Lambda (t)$CDM models from $H(z)$ and DESI DR2 BAO measurements
• Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families
• A new magnitude--redshift relation based on Type Ia supernovae
• Crunching, Bouncing, and Cyclical Cosmologies from Dark Sector Interactions
• Revisiting observational constraints on coupled exponential quintessence with energy and momentum transfers: degeneracy with massive neutrinos
• Galaxy number-count dipole and superhorizon fluctuations
• Expected redshift drift for tilted observers
• Constraining Spatial Curvature with Priors from Swampland Conjectures
• Finite time pseudo-rip singularity in cosmology
• Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
• 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
• Gravitational-wave standard sirens and application in cosmology
• Kiselev black hole and the ultra-slow evaporating behavior
• Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae
• Thermodynamic reconstruction in observationally constrained dynamical dark energy models