The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Abstract

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades. This concordance model is constructed by a universal cosmological constant and supported by a matter sector described by the standard model of particle physics and a cold dark matter contribution, as well as very early-time inflationary physics, and underpinned by gravitation through general relativity. There have always been open questions about the soundness of the foundations of the standard model. However, recent years have shown that there may also be questions from the observational sector with the emergence of differences between certain cosmological probes. In this White Paper, we identify the key objectives that need to be addressed over the coming decade together with the core science projects that aim to meet these challenges. These discordances primarily rest on the divergence in the measurement of core cosmological parameters with varying levels of statistical confidence. These possible statistical tensions may be partially accounted for by systematics in various measurements or cosmological probes but there is also a growing indication of potential new physics beyond the standard model. After reviewing the principal probes used in the measurement of cosmological parameters, as well as potential systematics, we discuss the most promising array of potential new physics that may be observable in upcoming surveys. We also discuss the growing set of novel data analysis approaches that go beyond traditional methods to test physical models. [Abridged]

416 pages, 81 figures

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• Dark matter halos of massive elliptical galaxies at $z\sim 0.2$ are well described by the Navarro-Frenk-White profile
• Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
• On the consistency of universally non-minimally coupled $f(R,T,R_{\mu \nu }{T}^{\mu \nu })$ theories
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• New models and Big Bang Nucleosynthesis constraints in $f(Q)$ gravity
• LXCDM: a cosmon model solution to the cosmological coincidence problem?
• New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
• Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics
• The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Analysis and Data Release 2
• Interacting neutrinos in cosmology: exact description and constraints
• A measurement of Hubble's Constant using Fast Radio Bursts
• DES Y3 results: Blending shear and redshift biases in image simulations
• Metacalibration: Direct Self-Calibration of Biases in Shear Measurement
• Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles
• Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations
• Constraints on a Bianchi type I spacetime extension of the standard $\Lambda$CDM model
• Spectral sirens: cosmology from the full mass distribution of compact binaries
• Shadows of Sgr A${}^{\ast }$ Black Hole Surrounded by Superfluid Dark Matter Halo
• CMB multipole measurements in the presence of foregrounds
• Using The Baryonic Tully-Fisher Relation to Measure $H_o$
• First Batch of Candidate Galaxies at Redshifts 11 to 20 Revealed by the James Webb Space Telescope Early Release Observations
• Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
• Cosmological implications of the anisotropy of ten galaxy cluster scaling relations
• A dynamical model of the local cosmic expansion
• Heavy spin-2 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
• Blue-tilted Tensor Spectrum and Thermal History of the Universe
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
• Preheating in Palatini Higgs inflation
• First results from the OSQAR photon regeneration experiment: No light shining through a wall
• The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies
• Direct neutrino-mass measurement based on 259 days of KATRIN data
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• 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
• A Compendium of Chameleon Constraints
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• Model Independent Reconstruction of the Expansion History of the Universe and the Properties of Dark Energy
• The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses
• Improved constraints on H0 from a combined analysis of gravitational-wave and electromagnetic emission from GW170817
• Imprints of Dark Matter on Black Hole Shadows using Spherical Accretions
• Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant
• Cosmological Effects of Nonlinear Electrodynamics
• Restoring cosmological concordance with early dark energy and massive neutrinos?
• Cosmology with self-interacting sterile neutrinos and dark matter - A pseudoscalar model
• Cosmographic Hubble fits to the supernova data
• Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
• Running vacuum against the $H_0$ and ${\sigma }_8$ tensions
• Modelling the Sgr A* Black Hole Immersed in a Dark Matter Spike
• Early recombination as a solution to the $H_0$ tension
• An 8\% Determination of the Hubble Constant from localized Fast Radio Bursts
• Stochastic star formation in early galaxies: JWST implications
• Phenomenology of D-Brane Inflation with General Speed of Sound
• Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model
• Photometric Redshifts for Next-Generation Surveys
• Hints of FLRW Breakdown from Supernovae
• The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae
• Sample variance in the local measurements of the Hubble constant
• Updated constraints on massive neutrino self-interactions from cosmology in light of the $H_0$ tension
• The $\bar{\Lambda }CDM$ cosmology: from inflation to dark energy through running $\Lambda$
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• The Cosmological Constant Problem and Running Vacuum in the Expanding Universe
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• Star formation histories of UV-luminous galaxies at $z\simeq 6.8$: implications for stellar mass assembly at early cosmic times
• The Tully-Fisher relation for S0 galaxies
• The Cosmic Radio Dipole: Estimators and Frequency Dependence
• The Young Supernova Experiment: Survey Goals, Overview, and Operations
• Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of ${\sigma }_8$
• Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?
• A new tension in the cosmological model from primordial deuterium?
• The $L-\sigma$ relation for massive bursts of star formation
• Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
• EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension
• The Chandra COSMOS legacy survey: Energy Spectrum of the Cosmic X-ray Background and constraints on undetected populations
• Dehnen halo effect on a black hole in an ultra-faint dwarf galaxy
• Detection of the Gravitational Lens Magnifying a Type Ia Supernova
• A $w-M$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension
• TDCOSMO. XII. Improved Hubble constant measurement from lensing time delays using spatially resolved stellar kinematics of the lens galaxy
• Interacting radiation after Planck and its implications for the Hubble Tension
• Cosmological Constraints on Dark Matter Interactions with Ordinary Matter
• The PHLEK Survey: A New Determination of the Primordial Helium Abundance
• The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX): Description and Early Pilot Survey Results
• DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest
• Negative cosmological constant in the dark sector?
• The brightness of the Red Giant Branch tip: Theoretical framework, a set of reference models, and predicted observables
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• Dark matter effect on the weak deflection angle by black holes at the center of Milky Way and M87 galaxies
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-Point Calibration
• Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data
• Higgsed Chromo-Natural Inflation
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• Improving Helium Abundance Determinations with Leo P as a Case Study
• CMB bispectrum from primordial magnetic fields on large angular scales
• Galaxy Build-up in the first 1.5 Gyr of Cosmic History: Insights from the Stellar Mass Function at $z\sim 4-9$ from JWST NIRCam Observations
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Primordial Deuterium after LUNA: concordances and error budget
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• Observational bounds on the cosmic radiation density
• SN2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova
• Shadow and weak deflection angle of extended uncertainty principle black hole surrounded with dark matter
• On Larger $H_0$ Values in the CMB Dipole Direction
• Dark energy in light of the early JWST observations: case for a negative cosmological constant?
• Dark matters on the scale of galaxies
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• The X-ray fundamental plane of the Platinum Sample, the Kilonovae and the SNe Ib/c associated with GRBs
• Using Galaxy Two-point Correlation Functions to Determine the Redshift Distributions of Galaxies Binned by Photometric Redshift
• Gamma-ray induced cascades and magnetic fields in intergalactic medium
• New Constraints on Warm Dark Matter from the Lyman-$\alpha$ Forest Power Spectrum
• Has JWST already falsified dark-matter-driven galaxy formation?
• The cosmic microwave background temperature bispectrum from scalar perturbations induced by primordial magnetic fields
• An independent determination of the local Hubble constant
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• Baryonic Tully-Fisher Relation for Extremely Low Mass Galaxies
• A Subaru Weak Lensing Survey I: Cluster Candidates and Spectroscopic Verification
• Disformal couplings and the dark sector of the universe
• Can late-time extensions solve the $H_0$ and ${\sigma }_8$ tensions?
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of $z>12$ Galaxies
• Testing Screened Modified Gravity
• Strong lensing time-delay cosmography in the 2020s
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Matching current observational constraints with nonminimally coupled dark energy
• Slow-roll inflation in $f(Q)$ non-metric gravity
• Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
• Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
• Evidence for suppression of structure growth in the concordance cosmological model
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Standard rulers, candles, and clocks from the low-redshift Universe
• The Big-Bang Singularity in the framework of a Generalized Uncertainty Principle
• Search for Dark Matter Axions with CAST-CAPP
• A new perspective on Dark Energy modeling via Genetic Algorithms
• Relieving the $H_0$ tension with a new interacting dark energy model
• Unification of inflation and dark energy {\it à la} quintessential inflation
• Constraints on Cosmological Parameters from the 500 deg${}^2$ SPTpol Lensing Power Spectrum
• Detection of a Supervoid Aligned with the Cold Spot of the Cosmic Microwave Background
• Running vacuum in quantum field theory in curved spacetime: renormalizing ${\rho }_{vac}$ without $\sim m^4$ terms
• Constraints on $\Lambda$CDM Extensions from the SPT-3G 2018 $EE$ and $TE$ Power Spectra
• Tracing The Sound Horizon Scale With Photometric Redshift Surveys
• The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
• Quintom cosmology and modified gravity after DESI 2024
• Toward a New Distance to the Active Galaxy NGC 4258: II. Centripetal Accelerations and Investigation of Spiral Structure
• Implication of the Hubble tension for the primordial Universe in light of recent cosmological data
• A class of quintessential inflation models with parameter space consistent with BICEP2
• Light Neutralino Dark Matter: Direct/Indirect Detection and Collider Searches
• Non-extensive Statistics Solution to the Cosmological Lithium Problem
• The Impact of New d(p,γ)He3 Rates on Big Bang Nucleosynthesis
• Radiative Production of Non-thermal Dark Matter
• Inflation meets neutrinos
• A designer approach to $f(Q)$ gravity and cosmological implications
• Cosmology Intertwined IV: The Age of the Universe and its Curvature
• On the baryonic, stellar, and luminous scaling relations of disk galaxies
• Observational constraints on successful model of quintessential Inflation
• Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study
• New Early Dark Energy is compatible with current LSS data
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• A detection of the integrated Sachs-Wolfe imprint of cosmic superstructures using a matched-filter approach
• Templates for Fitting Photometry of Ultra-High-Redshift Galaxies
• Sharpening the Tip of the Red Giant Branch
• Dark sector interaction and the supernova absolute magnitude tension
• TDCOSMO V: strategies for precise and accurate measurements of the Hubble constant with strong lensing
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model
• Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
• Anisotropic non-Gaussianity from vector field perturbations
• The high mass end of the Tully-Fisher relation
• Large-Scale Clustering of Cosmic Voids
• The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey
• Inhomogeneous vacuum energy
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• A massive blow for $\Lambda$CDM $-$ the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology
• A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey
• Testing Late Time Cosmic Acceleration with uncorrelated Baryon Acoustic Oscillations dataset
• Galaxy Bias and its Effects on the Baryon Acoustic Oscillations Measurements
• Arc sensitivity to cluster ellipticity, asymmetries and substructures
• A Model of Universe Anisotropization
• Assessing tension metrics with Dark Energy Survey and Planck data
• Spatially Resolved Properties of High Redshift Galaxies in the SMACS0723 JWST ERO Field
• The Megamaser Cosmology Project. VI. Observations of NGC 6323
• Cosmology Intertwined I: Perspectives for the Next Decade
• The FAST all sky HI survey (FASHI): The first release of catalog
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• Fast cosmological parameter estimation using neural networks
• Dark Matter Halos with Cores from Hierarchical Structure Formation
• Dark Energy Survey Year 3 Results: Clustering Redshifts -- Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS
• Evidence of a decreasing trend for the Hubble constant
• Vacuum models with a linear and a quadratic term in H: structure formation and number counts analysis
• Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Direct detection of dark energy: the XENON1T excess and future prospects
• 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
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• Dark Matter Halos of Disk Galaxies: Constraints from the Tully-Fisher Relation
• Ultra-light dark matter in disk galaxies
• CEERS Key Paper IV: Galaxies at $4<z<9$ are Bluer than They Appear -- Characterizing Galaxy Stellar Populations from Rest-Frame $\sim 1$ micron Imaging
• Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
• Distance estimates for AGB stars from parallax measurements
• Black holes in galactic centers: quasinormal ringing, grey-body factors and Unruh temperature
• Dark Radiation Emerging After Big Bang Nucleosynthesis?
• Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest
• Early results from GLASS-JWST. XI: Stellar masses and mass-to-light ratio of z>7 galaxies
• High-Redshift Galaxies from Early JWST Observations: Constraints on Dark Energy Models
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from counts and stacked weak-lensing
• Scattering of Dark Matter and Dark Energy
• Do cosmological observations allow a negative $\Lambda$?
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology
• Bianchi Model CMB Polarization and its Implications for CMB Anomalies
• Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2 - I. Binarity from proper motion anomaly
• The state of the dark energy equation of state circa 2023
• The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure
• Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
• High-precision limit on variation in the fine-structure constant from a single quasar absorption system
• Numerical evolution of squeezed and non-Gaussian states in loop quantum cosmology
• zeus: A Python implementation of Ensemble Slice Sampling for efficient Bayesian parameter inference
• Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Validation of the accuracy and precision of Gaia EDR3 parallaxes with globular clusters
• Omnipotent dark energy: A phenomenological answer to the Hubble tension
• Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Observable-to-Mass-and-Redshift Relations of Galaxy Clusters and Groups with Weak-Lensing Mass Calibration from the Hyper Suprime-Cam Subaru Strategic Program Survey
• Robustness of dark energy phenomenology across different parameterizations
• Relativistic N-body simulations with massive neutrinos
• A new measurement of the expansion history of the Universe at z=1.26 with cosmic chronometers in VANDELS
• A 5% measurement of the Hubble constant from Type II supernovae
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology
• Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data
• The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
• Towards early dark energy and $n_s$=1 with Planck, ACT and SPT
• DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons
• Consistency of effective field theory analyses of the BOSS power spectrum
• Primordial power spectrum in light of JWST observations of high redshift galaxies
• Resolving the Hubble tension with Early Dark Energy
• Did JWST observe imprints of axion miniclusters or primordial black holes?
• New period-luminosity and period-color relations of classical Cepheids: III. Cepheids in SMC
• How to use GP: Effects of the mean function and hyperparameter selection on Gaussian Process regression
• The Cosmic Microwave Background and the Ionization History of the Universe
• Calibrating Dark Energy
• Cosmological Bound on the QCD Axion Mass, Redux
• Constraining the Dark Energy Equation of State with HII Galaxies
• Observational constraints on the deceleration parameter in a tilted universe
• Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the ${\sigma }_8$ and $H_0$ tensions
• The UTMOST: A hybrid digital signal processor transforms the MOST
• The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• Tidal Deformability of Dark Matter Admixed Neutron Stars
• Addressing $H_0$ tension by means of VCDM
• Revisit of the interacting holographic dark energy model after Planck 2015
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Lorentz-covariant deformed algebra with minimal length
• Accelerating astronomical and cosmological inference with Preconditioned Monte Carlo
• Cosmological constraints on multi-interacting dark matter
• Cosmology and modified gravitational wave propagation from binary black hole population models
• Quasar standardization: Overcoming Selection Biases and Redshift Evolution
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• Homogeneous and isotropic cosmologies with nonlinear electromagnetic radiation
• The lensing and temperature imprints of voids on the Cosmic Microwave Background
• The halo model for cosmology: a pedagogical review
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• $f(R)$ gravity in the Jordan Frame as a Paradigm for the Hubble Tension
• Neutrino Self-Interactions and Double Beta Decay
• Infrared Tip of the Red Giant Branch and Distances to the Maffei/IC 342 Group
• Early galaxy formation in warm dark matter cosmologies
• Additional Light Sterile Neutrinos and Cosmology
• Late time interacting cosmologies and the Hubble constant tension
• Constraints on Primordial Magnetic Fields from Planck combined with the South Pole Telescope CMB B-mode polarization measurements
• Black hole in quantum wave dark matter
• A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• The Radial Tully-Fisher relation for spiral galaxies I
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
• HICOSMO - Cosmology with a complete sample of galaxy clusters: I. Data analysis, sample selection and luminosity-mass scaling-relation
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• Constraining the physical properties of the first lensed $z\sim 10-16$ galaxy candidates with JWST
• $T_0$ censorship of early dark energy and AdS vacua
• KiDS-1000: cosmic shear with enhanced redshift calibration
• Model-agnostic assessment of dark energy after DESI DR1 BAO
• STRIDES: Automated uniform models for 30 quadruply imaged quasars
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium
• Cosmological equivalence principle and the weak-field limit
• Long Range Interactions in Cosmology: Implications for Neutrinos
• Determination of the primordial helium abundance based on NGC 346 an HII region of the Small Magellanic Cloud
• Can Gravitational Instantons Really Constrain Axion Inflation?
• Hybrid cosmological attractors
• Exploring the high-redshift PBH-$\Lambda$CDM Universe: early black hole seeding, the first stars and cosmic radiation backgrounds
• Non-Gaussian estimates of tensions in cosmological parameters
• Imprint of the seesaw mechanism on feebly interacting dark matter and the baryon asymmetry
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae
• A new cosmological distance measure using AGN X-ray variability
• Constraints on the Evolution of the Primordial Magnetic Field from the Small-Scale Cosmic Microwave Background Angular Anisotropy
• The stacked ISW signal of rare superstructures in ΛCDM
• Can a supervoid explain the Cold Spot?
• COMAP Early Science: I. Overview
• Reconstruction of the Dark Energy equation of state
• The Early Dark Sector, the Hubble Tension, and the Swampland
• Relaxing the ${\sigma }_8$-tension through running vacuum in the Universe
• An Improved Calibration of the Wavelength Dependence of Metallicity on the Cepheid Leavitt law
• Model-independent reconstruction of $f(T)$ teleparallel cosmology
• The Megamaser Cosmology Project.IX. Black hole masses for three maser galaxies
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Primordial Magnetic Field Limits from Cosmic Microwave Background Bispectrum of Magnetic Passive Scalar Modes
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Addressing the cosmological $H_0$ tension by the Heisenberg uncertainty
• Independent Cosmological Constraints from high-z HII Galaxies
• Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
• Concordance cosmology without dark energy
• Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model
• Cosmology under the fractional calculus approach
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Gaussian processes and effective field theory of $f(T)$ gravity under the $H_0$ tension
• Cosmological Constraints from Gas Mass Fractions of Massive, Relaxed Galaxy Clusters
• CMB anisotropies due to cosmological magnetosonic waves
• The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Multipole decomposition of the general luminosity distance 'Hubble law' -- a new framework for observational cosmology
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Neutrino-Assisted Early Dark Energy: Theory and Cosmology
• Direct detection of dark matter: a critical review
• Testing the Cosmological Principle with CatWISE Quasars: A Bayesian Analysis of the Number-Count Dipole
• Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
• Forecasting constraints on deviations from general relativity in $f(Q)$ gravity with standard sirens
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• Viability of the matter bounce scenario in Loop Quantum Cosmology for general potentials
• Do we Live in a "Small Universe"?
• Parametric and nonparametric methods hint dark energy evolution
• Isotropic cosmic birefringence from early dark energy
• Quantifying the Effects of Known Unknowns on Inferred High-redshift Galaxy Properties: Burstiness, the IMF, and Nebular Physics
• Hot New Early Dark Energy
• Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
• New NIR light-curve templates for classical Cepheids
• The Parallax Zero-Point of Gaia Early Data Release 3 from LAMOST Primary Red Clump Stars
• Gravitoelectromagnetism, Solar System Test and Weak-Field Solutions in $f(T,B)$ Gravity with Observational Constraints
• Gravitational Waves from Light Cosmic Strings: Backgrounds and Bursts with Large Loops
• A double take on early and interacting dark energy from JWST
• Cosmic viscosity as a remedy for tension between PLANCK and LSS data
• Euclid: Cosmological forecasts from the void size function
• A tale of two (or more) $h$'s
• Resolving Cosmic Gamma Ray Anomalies with Dark Matter Decaying Now
• Observable primordial vector modes
• Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
• Cosmic variance of the galaxy cluster weak lensing signal
• Model-independent cosmological inference post DESI DR1 BAO measurements
• Alleviating the need for exponential evolution of JWST galaxies in 10${}^{10}{M}_{\odot }$ haloes at $z>10$ by a modified $\Lambda$CDM power spectrum
• Luminous superclusters: remnants from inflation
• Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
• Gaia EDR3 Parallax Zero-point Offset based on W Ursae Majoris-type Eclipsing Binaries
• 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
• A 0.9% Calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids
• Dark matter spike around Bumblebee black holes
• Probing elastic interactions in the dark sector and the role of $S_8$
• Towards hybrid inflation with $n_s=1$ in light of Hubble tension and primordial gravitational waves
• Testing the Quasar Hubble Diagram with LISA Standard Sirens
• New Constraints on the Mass of Fermionic Dark Matter from Dwarf Spheroidal Galaxies
• Novel null tests for the spatial curvature and homogeneity of the Universe and their machine learning reconstructions
• The impact of an evolving stellar initial mass function on early galaxies and reionisation
• Stringy-Running-Vacuum-Model Inflation: from primordial Gravitational Waves and stiff Axion Matter to Dynamical Dark Energy
• Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS
• A Step in Understanding the $S_8$ Tension
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• JAX-COSMO: An End-to-End Differentiable and GPU Accelerated Cosmology Library
• Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey
• Big Bang Nucleosynthesis constraints on higher-order modified gravities
• Comparing inclination dependent analyses of kilonova transients
• Anisotropy of the Universe via the Pantheon supernovae sample revisited
• Novel cosmological bounds on thermally-produced axion-like particles
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Finsler-Randers Cosmology: dynamical analysis and growth of matter perturbations
• Black hole surrounded by the pseudo-isothermal dark matter halo
• A new way to test the Cosmological Principle: measuring our peculiar velocity and the large scale anisotropy independently
• Realistic simulations of galaxy formation in f(R) modified gravity
• Improved Treatment of Dark Matter Capture in White Dwarfs
• Constraints on Scalar and Tensor spectra from $N_{eff}$
• The resilience of the Etherington-Hubble relation
• Improved constraints on the dark energy equation of state using Gaussian processes
• Kinematic constraints beyond $z\simeq 0$ using calibrated GRB correlations
• Non-parametric reconstruction of the cosmological \textit{jerk} parameter
• Equation of state of the running vacuum
• Evolution of gravitational orbits in the expanding universe
• Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
• Imprint of DES super-structures on the Cosmic Microwave Background
• Rates and delay times of type Ia supernovae in the Dark Energy Survey
• Towards a precision calculation of $N_{\mathrm{eff}}$ in the Standard Model III: Improved estimate of NLO contributions to the collision integral
• Markov chain Monte Carlo analysis of Bianchi VII_h models
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Search for GeV-scale Dark Matter Annihilation in the Sun with IceCube DeepCore
• Rotating black holes in three-dimensional Hořava gravity
• Gravitino thermal production revisited
• Uncovering a population of gravitational lens galaxies with magnified standard candle SN Zwicky
• Earth as a transducer for dark-photon dark-matter detection
• White Paper and Roadmap for Quantum Gravity Phenomenology in the Multi-Messenger Era
• A new determination of the primordial helium abundance using the analyses of HII region spectra from SDSS
• New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood
• Using Surface Brightness Fluctuations to Study Nearby Satellite Galaxy Systems: Calibration and Methodology
• Simple-graduated dark energy and spatial curvature
• Hints for a gravitational constant transition in Tully-Fisher data
• Taiji Data Challenge for Exploring Gravitational Wave Universe
• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• A type of Born-Infeld regular gravity and its cosmological consequences
• Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the ${\Omega }_m$-${\sigma }_8$ plane
• Neural Network Reconstruction of Late-Time Cosmology and Null Tests
• Optical selection bias and projection effects in stacked galaxy cluster weak lensing
• Directional Variations of Cosmological Parameters from the Planck CMB Data
• Lensed Type Ia Supernova "Encore" at z=2: The First Instance of Two Multiply-Imaged Supernovae in the Same Host Galaxy
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• High-redshift JWST Observations and Primordial Non-Gaussianity
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• The Mira-Titan Universe IV. High Precision Power Spectrum Emulation
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach
• Strong gravitational lensing and microlensing of supernovae
• The ArDM Liquid Argon Time Projection Chamber at the Canfranc Underground Laboratory: a ton-scale detector for Dark Matter Searches
• Translation and Rotation Equivariant Normalizing Flow (TRENF) for Optimal Cosmological Analysis
• Automated galaxy-galaxy strong lens modelling: no lens left behind
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Inferring $S_8(z)$ and $\gamma (z)$ with cosmic growth rate measurements using machine learning
• Phantom matter: a challenging solution to the cosmological tensions
• Joint Analysis of near-infrared properties and surface brightness fluctuations of LMC star clusters
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Constraints on the Faint End of the Galaxy Stellar Mass Function at z ~ 4-8 from Deep JWST Data
• CONNECT: A neural network based framework for emulating cosmological observables and cosmological parameter inference
• Cosmography by orthogonalized logarithmic polynomials
• The Dark Energy Spectroscopic Instrument: One-dimensional power spectrum from first Lyman-$\alpha$ forest samples with Fast Fourier Transform
• Modelling and testing the equation of state for (Early) dark energy
• The First Billion Years of a Warm Dark Matter Universe
• Aspects of the Dark Dimension in Cosmology
• Modified big bang nucleosynthesis with non-standard neutron sources
• The Dark Energy Survey Year 3 and eBOSS: constraining galaxy intrinsic alignments across luminosity and colour space
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
• Assessment of the cosmic distance duality relation using Gaussian Process
• Probing nuclear rates with Planck and BICEP2
• Large Magellanic Cloud Near-Infrared Synoptic Survey. V. Period-Luminosity Relations of Miras
• Inference of the cosmic rest-frame from supernovae Ia
• Updated constraints on decaying cold dark matter
• Cosmic voids: a novel probe to shed light on our Universe
• Modified Gravity Constraints from the Full Shape Modeling of Clustering Measurements from DESI 2024
• A Bayesian direct method implementation to fit emission line spectra: Application to the primordial He abundance determination
• A sub-2% Distance to M31 from Photometrically Homogeneous Near-Infrared Cepheid Period-Luminosity Relations Measured with the Hubble Space Telescope
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Cross-correlating the gamma-ray sky with catalogs of galaxy clusters
• Optical Identification of Cepheids in 19 Host Galaxies of Type Ia Supernovae and NGC 4258 with the Hubble Space Telescope
• Big-bounce and future time singularity resolution in Bianchi I: the projective invariant Nieh-Yan case
• Late-Time constraints on Interacting Dark Energy: Analysis independent of $H_0$, $r_d$ and $M_B$
• Crossing Statistic: Reconstructing the Expansion History of the Universe
• WALLABY Pilot Survey: Public release of HI data for almost 600 galaxies from phase 1 of ASKAP pilot observations
• Investigating effects of dark matter on photon orbits and black hole shadows
• Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB
• CP violating scalar Dark Matter
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• Importance nested sampling with normalising flows
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Quasinormal modes of Schwarzschild black holes in projective invariant Chern-Simons modified gravity
• Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios
• Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments
• Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
• The Hubble constant from strongly lensed supernovae with standardizable magnifications
• Evaluating bulk flow estimators for CosmicFlows-4 measurements
• A Bayesian comparison between $\Lambda$CDM and phenomenologically emergent dark energy models
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Toward a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift
• Integral $F(R)$ Gravity and Saddle Point Condition as a Remedy for the $H_0$-tension
• Interacting dark energy: clarifying the cosmological implications and viability conditions
• Dark energy, the colored anti-de Sitter vacuum, and LHC phenomenology
• New constraints on ${\sigma }_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters
• Astrophysical Distance Scale The JAGB Method: I. Calibration and a First Application
• QUBIC I: Overview and ScienceProgram
• Early dark energy in $k$-essence
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
• A Giant Arc on the Sky
• One spectrum to cure them all: Signature from early Universe solves major anomalies and tensions in cosmology
• What it takes to solve the Hubble tension through modifications of cosmological recombination
• Black holes surrounded by Einstein clusters as models of dark matter fluid
• LISA Definition Study Report
• The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters
• Rapidly growing primordial black holes as seeds of the massive high-redshift JWST Galaxies
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Composite Dark Energy and the Cosmological Tensions
• Clues on void evolution III: Structure and dynamics in void shells
• Model-independent constraints on cosmic curvature: implication from updated Hubble diagram of high-redshift standard candles
• An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). IV. Discovery of High-Redshift AGB Analogs
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
• Chemical abundances in 7 metal-poor HII regions and a determination of the primordial helium abundance
• Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
• Shock cooling of a red-supergiant supernova at redshift 3 in lensed images
• An updated metal-dependent theoretical scenario for Classical Cepheids
• Towards a model-independent reconstruction approach for late-time Hubble data
• The fifth data release of the Kilo Degree Survey: Multi-epoch optical/NIR imaging covering wide and legacy-calibration fields
• Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence
• Quintessential inflation: A tale of emergent and broken symmetries
• How to relax the cosmological neutrino mass bound
• Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation -- II. KODIAQ, SQUAD & XQ-100
• Is the dark energy equation of state parameter singular?
• Hot New Early Dark Energy: Towards a Unified Dark Sector of Neutrinos, Dark Energy and Dark Matter
• Black Hole Shadows in Verlinde's Emergent Gravity
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• KiDS-1000: Cosmology with improved cosmic shear measurements
• Early Structure Formation from Cosmic String Loops in Light of Early JWST Observations
• Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: I. HARPS-N@TNG spectroscopy of 47 Classical Cepheid and 1 BL Her variables
• Is there a need and another way to measure the Cosmic Microwave Background temperature more accurately?
• Baryogenesis in Nonminimally Coupled $f(R)$ Theories
• Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\mathrm{eff}}$=0.85 from the final dataset
• Baryon Asymmetry from the Generalized Uncertainty Principle
• Solving the Hubble tension without spoiling Big Bang Nucleosynthesis
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• Ruling Out New Physics at Low Redshift as a solution to the $H_0$ Tension
• Calibrating Gamma-Ray Bursts by Using a Gaussian Process with Type Ia Supernovae
• Cosmology beyond BAO from the 3D distribution of the Lyman-$\alpha$ forest
• Massive neutrino self-interactions and inflation
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• The integrated 3-point correlation function of cosmic shear
• Dark matter in ghost-free bigravity theory: From a galaxy scale to the universe
• A simultaneous solution to the Hubble tension and observed bulk flow within 250 $h^{-1}$ Mpc
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• Reconstruction of the neutrino mass as a function of redshift
• Reconnaissance with JWST of the J-region Asymptotic Giant Branch in Distance Ladder Galaxies: From Irregular Luminosity Functions to Approximation of the Hubble Constant
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Metric $f(R)$ gravity with dynamical dark energy as a scenario for the Hubble tension
• The Mira Distance to M101 and a 4% Measurement of H0
• Carbon stars as standard candles: I. The luminosity function of carbon stars in the Magellanic Clouds
• Cosmological gravitational particle production of massive spin-2 particles
• The GALAH Survey: A new constraint on cosmological lithium and Galactic lithium evolution from warm dwarf stars
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• Sloan Great Wall as a complex of superclusters with collapsing cores
• Target Selection for the DESI Peculiar Velocity Survey
• A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters
• Cosmic microwave background bispectrum of tensor passive modes induced from primordial magnetic fields
• BAO signatures in the 2-point angular correlations and the Hubble tension
• The cosmic radio dipole: Bayesian estimators on new and old radio surveys
• Higgs inflation and teleparallel gravity
• Early and late time cosmology: the $f(R)$ gravity perspective
• Evolution of the fine-structure constant in runaway dilaton models
• An Infrared Census Of Dust In Nearby Galaxies With Spitzer (DUSTiNGS): V. The Period-luminosity Relation For Dusty Metal-Poor AGB Stars
• Bayesian forward modelling of cosmic shear data
• Noether Symmetries and Quantum Cosmology in Extended Teleparallel Gravity
• Resolving conclusions about the early Universe requires accurate nuclear measurements
• Parque Astronómico de Atacama: An ideal site for millimeter, submillimeter, and mid-infrared astronomy
• The contribution of discrete sources to the sky temperature at 144 MHz
• Self-Interacting Neutrinos in Light of Large-Scale Structure Data
• Planck-scale-modified dispersion relations in homogeneous and isotropic spacetimes
• Projected Cosmological Constraints from Strongly Lensed Supernovae with the Roman Space Telescope
• Snowmass2021 CMB-HD White Paper
• Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee
• Dynamics in Varying vacuum Finsler-Randers Cosmology
• Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
• Running vacuum in QFT in FLRW spacetime: The dynamics of ${\rho }_{\mathrm{vac}}(H)$ from the quantized matter fields
• Modelling Long-Period Variables -- II. Fundamental mode pulsation in the nonlinear regime
• Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements
• Model selection applied to reconstructions of the Dark Energy
• Principal reconstructed modes of dark energy and gravity
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Spectral modeling of type II supernovae II. A machine learning approach to quantitative spectroscopic analysis
• 6Li/7Li estimates for metal-poor stars
• Six Puzzles for LCDM Cosmology
• Mathematical foundations for field theories on Finsler spacetimes
• Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Slow-rolling scalar dynamics and as solution for the Hubble tension
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Testing dark matter interactions with CMB spectral distortions
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• Simple inflationary quintessential model II: Power law potentials
• Optical appearance of black holes surrounded by a dark matter halo
• Quantum Gravity Corrections and Entropy at the Planck time
• Cosmological constraints on ${\Lambda }_{\mathrm{s}}$CDM scenario in a type II minimally modified gravity
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• JWST high-z galaxy constraints on warm and cold dark matter models
• Updated Constraints on Primordial Black Hole Evaporation
• JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78
• Bianchi I meets the Hubble diagram
• Axionic dark energy and a composite QCD axion
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Thermalizing sterile neutrino dark matter
• Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension
• Dwarf galaxies imply dark matter is heavier than $2.2\times 10^{-21}\mathbf{eV}$
• The DES view of the Eridanus supervoid and the CMB Cold Spot
• The future search for low-frequency axions and new physics with the FLASH resonant cavity experiment at Frascati National Laboratories
• Multi-field dark energy: cosmic acceleration on a steep potential
• Hubble tension vs two flows
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at $z\sim 3$
• CMB anisotropies in the presence of a stochastic magnetic field
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• Do supernovae indicate an accelerating universe?
• Towards a reliable calculation of relic radiation from primordial gravitational waves
• FLIMFLAM DR1: The First Constraints on the Cosmic Baryon Distribution from 8 FRB sightlines
• Relativistic kinetic gases as direct sources of gravity
• Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
• The Hubble Tension, The $M$ Crisis of Late Time $H(z)$ Deformation Models and the Reconstruction of Quintessence Lagrangians
• Small-scale clumping at recombination and the Hubble tension
• Observational constraints on early dark energy
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• The two-mode puzzle: Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum
• Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars
• Hubble tension bounds the GUP and EUP parameters
• Generalized Uncertainty Principle Impact on Nonextensive Black Hole Thermodynamics
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck II: Cross-correlation measurements and cosmological constraints
• First measurement of the Hubble parameter from bright binary black hole GW190521
• Dynamical dark energy confronted with multiple CMB missions
• Machine Learning improved fits of the sound horizon at the baryon drag epoch
• Tensions with the flat $\mathbf{\Lambda }$CDM model from high-redshift cosmography
• Further evidence that galaxy age drives observed type Ia supernova luminosity differences
• Gravitational ringing and superradiant instabilities of the Kerr-like black holes in a dark matter halo
• The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample
• An Effective Sign Switching Dark Energy: Lotka-Volterra Model of Two Interacting Fluids
• Tsallis and Kaniadakis statistics from the viewpoint of entropic gravity formalism
• Cold New Early Dark Energy pulls the trigger on the $H_0$ and $S_8$ tensions: a simultaneous solution to both tensions without new ingredients
• Constraining the curvature density parameter in cosmology
• Science with the Murchison Widefield Array: Phase I Results and Phase II Opportunities
• Landau damping for gravitational waves in parity-violating theories
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Confronting interacting dark radiation scenarios with cosmological data
• CosmoPower-JAX: high-dimensional Bayesian inference with differentiable cosmological emulators
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Redshift-space effects in voids and their impact on cosmological tests. Part II: the void-galaxy cross-correlation function
• Astrophysical Distance Scale II. Application of the JAGB Method: A Nearby Galaxy Sample
• Measuring the sound horizon and absolute magnitude of SNIa by maximizing the consistency between low-redshift data sets
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey
• Model marginalized constraints on neutrino properties from cosmology
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Euclid: Forecasts from the void-lensing cross-correlation
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Gamma-ray burst supernovae as standardizable candles
• An updated measurement of the Hubble constant from near-infrared observations of Type Ia supernovae
• The Local Hole: a galaxy under-density covering 90% of sky to ~200 Mpc
• Fourier-series expansion of the dark-energy equation of state
• Fuzzy Dark Matter as a Solution to Reconcile the Stellar Mass Density of High-z Massive Galaxies and Reionization History
• Time variation of proton-electron mass ratio and fine structure constant with runaway dilaton
• Cosmological singularities in Born-Infeld determinantal gravity
• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Machine Learning for Observational Cosmology
• Gravitational Lensing of Schwarzschild and Charged Black Holes Immersed in Perfect Fluid Dark Matter Halo
• Cosmic microwave background bispectrum of vector modes induced from primordial magnetic fields
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Influence of the Bounds of the Hyperparameters on the Reconstruction of Hubble Constant with Gaussian Process
• Primordial Magnetic Helicity Constraints from WMAP Nine-Year Data
• Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters
• The Copernican principle in light of the latest cosmological data
• Measuring the reionization optical depth without large-scale CMB polarization
• Dark radiation and small-scale structure problems with decaying particles
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest
• The IA Guide: A Breakdown of Intrinsic Alignment Formalisms
• Cosmography with next-generation gravitational wave detectors
• An effective description of Laniakea: impact on cosmology and the local determination of the Hubble constant
• Capse.jl: efficient and auto-differentiable CMB power spectra emulation
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• $S_8$ Tension in the Context of Dark Matter-Baryon Scattering
• Cosmographic view on the $H_0$ and ${\sigma }_8$ tensions
• Neural network reconstructions for the Hubble parameter, growth rate and distance modulus
• Dipole Cosmology: The Copernican Paradigm Beyond FLRW
• Exploiting the Einstein Telescope to solve the Hubble tension
• Testing cosmic anisotropy with Pantheon sample and quasars at high redshifts
• Cosmic backgrounds due to the formation of the first generation of supermassive black holes
• Constant roll inflation in multifield models
• Stellar prospects for FRB gravitational lensing
• Evolution of Dark Energy Perturbations in Scalar-Tensor Cosmologies
• Cosmological Avatars of the Landscape II: CMB and LSS Signatures
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Observational constraints on Tsallis modified gravity
• An exploration of an early gravity transition in light of cosmological tensions
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Large-Scale Gravitational Lens Modeling with Bayesian Neural Networks for Accurate and Precise Inference of the Hubble Constant
• Metastable dark energy
• Direct and indirect probes of Goldstone dark matter
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• Cosmology from weak lensing peaks and minima with Subaru Hyper Suprime-Cam survey first-year data
• TDCOSMO X. Automated Modeling of 9 Strongly Lensed Quasars and Comparison Between Lens Modeling Software
• Inflation via Gravitino Condensation in Dynamically Broken Supergravity
• Model independent bounds on Type Ia supernova absolute peak magnitude
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• Theoretical systematics in testing the Cosmological Principle with the kinematic quasar dipole
• Microlensing of the X-ray, UV and optical emission regions of quasars: Simulations of the time-scales and amplitude variations of microlensing events
• Cosmic voids detection without density measurements
• A new life for sterile neutrino dark matter after the pandemic
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• Tomographic Alcock-Paczynski Test with Redshift-Space Correlation Function: Evidence for the Dark Energy Equation of State Parameter w>-1
• Constraints on Yukawa gravity parameters from observations of bright stars
• The Gravitational Lensing Signatures of BOSS Voids in the Cosmic Microwave Background
• Early Dark Energy in Type IIB String Theory
• Stasis in an Expanding Universe: A Recipe for Stable Mixed-Component Cosmological Eras
• KiDS-1000 cosmology: Combined second- and third-order shear statistics
• From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension
• Cosmicflows-3: Cold Spot Repeller?
• Properties of M31. II: A Cepheid disk sample derived from the first year of PS1 PAndromeda data
• Bounding the mass of ultralight bosonic Dark Matter particles with the motion of the S2 star around Sgr A*
• Torsional birefringence in metric-affine Chern-Simons gravity: gravitational waves in late-time cosmology
• The Second Radio Synchrotron Background Workshop: Conference Summary and Report
• Non-parametric reconstruction of interaction in the cosmic dark sector
• Theoretical Aspects of Quintom Models
• Constraints on Tsallis Cosmology from Big Bang Nucleosynthesis and the Relic Abundance of Cold Dark Matter Particles
• Gravitationally induced particle production in scalar-tensor $f(R,T)$ gravity
• Cosmicflows-4: The Baryonic Tully-Fisher Relation Providing ~10,000 Distances
• Profiling Cold New Early Dark Energy
• Equivalence of non-minimally coupled cosmologies by Noether symmetries
• A model-independent reconstruction of dark sector interactions
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Recent advances in cosmological singularities
• Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• The multipole expansion of the local expansion rate
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• Observational constraints on bimetric gravity
• The Araucaria Project. Distances to Nine Galaxies Based on a Statistical Analysis of their Carbon Stars (JAGB Method)
• Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation
• Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
• Evidence for galaxy dynamics tracing background cosmology below the de Sitter scale of acceleration
• J-PAS: Forecasts for dark matter - dark energy elastic couplings
• Connecting Infrared Surface Brightness Fluctuation Distances to Type Ia Supernova Hosts: Testing the Top Rung of the Distance Ladder
• Quasars as high-redshift standard candles
• The TRGB-SBF Project. III. Refining the HST Surface Brightness Fluctuation Distance Scale Calibration with JWST
• Exploring the Hubble tension with a late time Modified Gravity scenario
• GroundBIRD : A CMB polarization experiment with MKID arrays
• Teleparallel axions and cosmology
• Effect of evolutionary physical constants on type-1a supernova luminosity
• Euclid preparation. XXXII. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
• The perspective of voids on rising cosmology tensions
• Why Cosmic Voids Matter: Nonlinear Structure & Linear Dynamics
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• Discordances in cosmology and the violation of slow-roll inflationary dynamics
• Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations
• Revisiting the Hubble constant, spatial curvature and cosmography with time-delay and cosmic chronometer observations
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• Cosmic Birefringence: Cross-Spectra and Cross-Bispectra with CMB Anisotropies
• A comparison of template vs. direct model fitting for redshift-space distortions in BOSS
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• ${\Lambda }_{\mathrm{s}}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties
• Hot thermal universe endowed with massive dark vector fields and the Hubble tension
• Promise of Future Searches for Cosmic Topology
• Noncommutative minisuperspace, gravity-driven acceleration and kinetic inflation
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Observational cosmology with Artificial Neural Networks
• Gaussian Processes Reconstruction of the Dark Energy Potential
• Quantifying the tension between cosmological and terrestrial constraints on neutrino masses
• Big-Bounce cosmology in the presence of Immirzi field
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Non-fiducial cosmological test from geometrical and dynamical distortions around voids
• Neural Network Reconstruction of $H^{\prime }(z)$ and its application in Teleparallel Gravity
• Cosmological parameter estimation with Genetic Algorithms
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Fundamental constants and cosmic vacuum: the micro and macro connection
• Phantom scalar-tensor models and cosmological tensions
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• Searching for the Evidence of Dynamical Dark Energy
• A comparison of optimisation algorithms for high-dimensional particle and astrophysics applications
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Gravitational transitions via the explicitly broken symmetron screening mechanism
• Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology
• Carbon stars as standard candles: II. The median J magnitude as a distance indicator
• Evolution of superclusters in the cosmic web
• Cosmological Constraints from the eBOSS Lyman-$\alpha$ Forest using the PRIYA Simulations
• Towards a possible solution to the Hubble tension with Horndeski gravity
• The formation and survival of the Milky Way's oldest stellar disk
• MCR-TRGB: A Multiwavelength-Covariant, Robust Tip of the Red Giant Branch Measurement Method
• Axiology
• Diffusion in unimodular gravity: Analytical solutions, late-time acceleration, and cosmological constraints
• ETHOS -- An effective parametrization and classification for structure formation: the non-linear regime at $z\gtrsim 5$
• The metallicity and distance of NGC 2403 from blue supergiants
• Rapidly Descending Dark Energy and the End of Cosmic Expansion
• Model-independent determination of the cosmic expansion rate. I. Application to type-Ia supernovae
• Impact of the Hubble tension on the $r$-$n_s$ contour
• A possible common explanation for several cosmic microwave background (CMB) anomalies: A strong impact of nearby galaxies on observed large-scale CMB fluctuations
• Testing $\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter
• Decaying dark matter, the $H_0$ tension, and the lithium problem
• C${}^3$-Cluster Clustering Cosmology I. New constraints on the cosmic growth rate at z~0.3 from redshift-space clustering anisotropies
• Quantum Genetic Algorithm with Individuals in Multiple Registers
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• Revised constraints on the photon mass from well-localized fast radio bursts
• Quasars: standard candles up to z=7.5 with the precision of Supernovae Ia
• Alleviating $H_0$ Tension with New Gravitational Scalar Tensor Theories
• A three-dimensional map of the Milky Way using 66,000 Mira variable stars
• Backreaction of axion-SU(2) dynamics during inflation
• New late-time constraints on $f(R)$ gravity
• Exact Solutions in Higher-Dimensional Lovelock and $Ad{S}_5$ Chern-Simons Gravity
• Tracing high redshift cosmic web with quasar systems
• The Corona Borealis supercluster: connectivity, collapse, and evolution
• candl: Cosmic Microwave Background Analysis with a Differentiable Likelihood
• ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors
• Non-Local Curvature and Gauss-Bonnet Cosmologies by Noether Symmetries
• Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection
• Gaussian Process Approach for Model-Independent Reconstruction of $f(Q)$ Gravity with Direct Hubble Measurements
• Quintessential Cosmological Tensions
• Fractional Holographic Dark Energy
• A roadmap to cosmological parameter analysis with third-order shear statistics I: Modelling and validation
• Observational test for $f(Q)$ gravity with weak gravitational lensing
• Probing correlations of early magnetic fields using mu-distortion
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Constraints via the Event Horizon Telescope for Black Hole Solutions with Dark Matter under the Generalized Uncertainty Principle Minimal Length Scale Effect
• H_0 tension: clue to common nature of dark sector?
• Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling
• ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn
• An improved Tully-Fisher estimate of $H_0$
• Starlet l1-norm for weak lensing cosmology
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
• Dark Matter Candidates of a Very Low Mass
• New integrable models and analytical solutions in $f(R)$~cosmology with an ideal gas
• The quest for new correlations in the realm of the Gamma-Ray Burst -- Supernova connection
• Model-independently calibrating the luminosity correlations of gamma-ray bursts using deep learning
• Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy
• Clusters of galaxies up to z=1.5 identified from photometric data of the Dark Energy Survey and unWISE
• Properties of self-excited pulsations in 3D simulations of AGB stars and red supergiants
• Testing an oscillatory behavior of dark energy
• Toward a concordance teleparallel Cosmology II: Linear perturbation
• No-go guide for the Hubble tension: late-time or local-scale new physics
• A short review on clustering dark energy
• Alleviating $H_0$ tension in Horndeski gravity
• Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
• Modeling Intrinsic Galaxy Alignment in the MICE Simulation
• Searching for dark energy with the Sun
• Progress on the calibration of surface brightness-color relations for early- and late-type stars
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Do we need soft cosmology?
• 4D Gauss-Bonnet gravity: cosmological constraints, $H_0$ tension and large scale structure
• A Maximum Likelihood Calibration of the Tip of the Red Giant Branch Luminosity from High Latitude Field Giants using Gaia Early Data Release 3 Parallaxes
• Compressing the cosmological information in one-dimensional correlations of the Lyman-$\alpha$ forest
• Strong lensing selection effects
• A Stochastic Approach To Reconstruct Gamma Ray Burst Lightcurves
• Impact of inhomogeneous reionization on the Lyman-α forest
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Analysis of Unified Galaxy Power Spectrum Multipole Measurements
• Dark Radiation from Neutrino Mixing after Big Bang Nucleosynthesis
• The Cosmic Dipole in the Quaia Sample of Quasars: A Bayesian Analysis
• Scalar perturbations from inflation in the presence of gauge fields
• Apparent and emergent dark matter around a Schwarzschild black hole
• Gamma-ray Bursts as Distance Indicators by a Statistical Learning Approach
• LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
• The 3D Lyman-$\alpha$ Forest Power Spectrum from eBOSS DR16
• Supernovae evidence for foundational change to cosmological models
• Large extra dimensions from higher-dimensional inflation
• Solving the $H_0$ tension in $f(T)$ Gravity through Bayesian Machine Learning
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• Constraining interacting dark energy models with the halo concentration-mass relation
• Exploring new physics in the late Universe's expansion through non-parametric inference
• A BayeSN Distance Ladder: $H_0$ from a consistent modelling of Type Ia supernovae from the optical to the near infrared
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Extracting cosmological parameters from N-body simulations using machine learning techniques
• Bayesian reconstruction of the inflaton's speed of sound using CMB data
• Big-Bang nucleosynthyesis: constraints on nuclear reaction rates, neutrino degeneracy, inhomogeneous and Brans-Dicke models
• Strong constraints on a simple self-interacting neutrino cosmology
• Testing f(R) gravity models with quasar X-ray and UV fluxes
• Quintessential Inflation from Lorentzian Slow Roll
• Constraining a late time transition of $G_{\mathrm{eff}}$ using low-z galaxy survey data
• Large-scale motions and growth rate from forward-modelling Tully-Fisher peculiar velocities
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• Mapping the ${\Lambda }_{\mathrm{s}}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate
• The expected kinematic matter dipole is robust against source evolution
• Coupled Multi Scalar Field Dark Energy
• The El Gordo galaxy cluster challenges ΛCDM for any plausible collision velocity
• Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data
• Local Hole revisited: evidence for bulk motions and self-consistent outflow
• Artificial intelligence and quasar absorption system modelling; application to fundamental constants at high redshift
• Gaussian Approximation of Peak Values in the Integrated Sachs-Wolfe Effect
• Cosmological Avatars of the Landscape I: Bracketing the SUSY Breaking Scale
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Hubble tension and absolute constraints on the local Hubble parameter
• The universal multiplicity function: counting halos and voids
• Sensitivity forecasts for the cosmological recombination radiation in the presence of foregrounds
• Cascading Dark Energy
• Scalar field dark matter and dark energy: a hybrid model for the dark sector
• The deceleration parameter in `tilted' universes: generalising the Friedmann background
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• On chromonatural inflation in string theory
• The Peebles -- Vilenkin quintessential inflation model revisited
• Two sides of the same coin: sterile neutrinos and dark radiation. Status and perspectives
• Constraining f(R) models with cosmic chronometers and the HII galaxy Hubble diagram
• Model-independent constraints on cosmic curvature: implication from the future gravitational wave observation DECIGO
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• Bounce Models within Teleparallel modified gravity
• Neural Networks Optimized by Genetic Algorithms in Cosmology
• Rescuing constraints on modified gravity using gravitational redshift in large-scale structure
• Measuring Hubble constant in an anisotropic extension of $\Lambda$CDM model
• Null test for cosmic curvature using Gaussian process
• LiteBIRD Science Goals and Forecasts: Improving Sensitivity to Inflationary Gravitational Waves with Multitracer Delensing
• Strong Evidence Against a Statistically Isotropic Universe
• Gravitational-wave dark siren cosmology systematics from galaxy weighting
• The redshift dependence of the inferred $H_0$ in a local void solution to the Hubble tension
• Guess the cheese flavour by the size of its holes: A cosmological test using the abundance of Popcorn voids
• The kinetic gas universe
• Neural networks and standard cosmography with newly calibrated high redshift GRB observations
• High Eddington quasars as discovery tools: current state and challenges
• TDCOSMO VIII: Cosmological distance measurements in light of the mass-sheet degeneracy -- forecasts from strong lensing and IFU stellar kinematics
• Gravitational Lensing in Modified Gravity: A case study for Fast Radio Bursts
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Dynamics in interacting scalar-torsion theory
• Bulk Flow Motion Detection in the Local Universe with Pantheon$+$ Type Ia Supernovae
• Impact of symmetron screening on the Hubble tension: new constraints using cosmic distance ladder data
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Comparative Analysis of TRGBs (CATs) from Unsupervised, Multi-Halo-Field Measurements: Contrast is Key
• Non-detection of ${}^6$Li in Spite plateau stars with ESPRESSO
• Alleviating $H_0$ tension in scalar-tensor and bi-scalar-tensor theories
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• Neural network reconstruction of cosmology using the Pantheon compilation
• Enhancing cosmic shear with the multi-scale lensing PDF
• Joint reconstructions of growth and expansion histories from stage-IV surveys with minimal assumptions. II. Modified gravity and massive neutrinos
• Effects of Baryonic Feedback on the Cosmic Web
• Cosmological foundations revisited with Pantheon+
• Unifying Inflation with early and late Dark Energy in Multi-Fields: Spontaneously broken scale invariant TMT
• Covariant cosmography: the observer-dependence of the Hubble parameter
• HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• The cosmic shallows I: interaction of CMB photons in extended galaxy halos
• Cross-correlation of Planck CMB lensing with DESI galaxy groups
• The evolution of Lithium: implications of a universal Spite plateau
• A Model of Interacting Dark Matter and Dark Radiation for $H_0$ and ${\sigma }_8$ Tensions
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Discordance of dipole asymmetries seen in recent large radio surveys with the Cosmological Principle
• Consistent extinction model for type Ia supernovae in Cepheid-based calibration galaxies and its impact on $H_0$
• Compatibility of JWST results with exotic halos
• A critical discussion on the $H_0$ tension
• Gravitationally induced matter creation in scalar-tensor $f(R,T_{\mu \nu }{T}^{\mu \nu })$ gravity
• Interacting dark sector from the trace-free Einstein equations: cosmological perturbations with no instability
• Testing the isotropy of cosmic acceleration with Pantheon+ and SH0ES: A cosmographic analysis
• Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for Type II Cepheids
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Running Hubble constant: evolutionary Dark Energy
• New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions
• Modified gravity in the presence of matter creation: scenario for the late Universe
• MG-MAMPOSSt: A code to test modifications of gravity with the dynamics of galaxy clusters
• Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
• Accounting for object detection bias in weak gravitational lensing studies
• Dark Stars Powered by Self-Interacting Dark Matter
• Non-comoving Cosmology
• Scalar-Tensor Gravity and DESI 2024 BAO data
• An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. I. HST WFC3/IR F110W and F160W Filters
• CoLFI: Cosmological Likelihood-free Inference with Neural Density Estimators
• The Layzer-Irvine equation in theories with non-minimal coupling between matter and curvature
• Carbon stars as standard candles -- III. Un-binned maximum likelihood fitting and comparison with TRGB estimations
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Dark Matter Line Searches with the Cherenkov Telescope Array
• Gravitational wave birefringence in spatially curved teleparallel cosmology
• Holographic and Gravity-Thermodynamic Approaches in Entropic Cosmology: Bayesian Assessment using late-time Data
• Reconstructing Quintessence
• Cluster cosmology with anisotropic boosts: Validation of a novel forward modeling analysis and application on SDSS redMaPPer clusters
• Dynamic cosmography of the local Universe: Laniakea and five more watershed superclusters
• Constraints on the cosmological parameters with three-parameter correlation of Gamma-ray bursts
• Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes
• Dark Energy from Inspiraling in Field Space
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach
• Jeans Instability in Non-Minimal Matter-Curvature Coupling Gravity
• Differentiating dark interactions with perturbation
• A cosmic glitch in gravity
• The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
• HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Global dynamics in Einstein-Gauss-Bonnet scalar field cosmology with matter
• Constraints on the axial-vector and pseudo-scalar mediated WIMP-nucleus interactions from PandaX-4T experiment
• Constraining $\Lambda$CDM cosmological parameters with Einstein Telescope mock data
• Hubble tension in a nonminimally coupled curvature-matter gravity model
• Getting the model right; an information criterion for spectroscopy
• Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Can accreting primordial black holes explain the excess radio background?
• Observational bounds on extended minimal theories of massive gravity: New limits on the graviton mass
• Baryon acoustic oscillations in thin redshift shells from BOSS DR12 and eBOSS DR16 galaxies
• Deviation from $\Lambda$CDM: Pressure Parametrization
• Cosmological constraints from weak lensing scattering transform using HSC Y1 data
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• NIR Tully-Fisher in the Zone of Avoidance. -- III. Deep NIR catalogue of the HIZOA galaxies
• The future of cosmological likelihood-based inference: accelerated high-dimensional parameter estimation and model comparison
• A Stimulating Explanation of the Extragalactic Radio Background
• Measuring anisotropic stress with relativistic effects
• A simple parametrisation for coupled dark energy
• D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models
• Can decaying dark matter scenarios alleviate both $H_0$ and ${\sigma }_8$ tensions?
• Probing modified gravitational-wave propagation with extreme mass-ratio inspirals
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Testing the $\Lambda$CDM paradigm with growth rate data and machine learning
• Future Constraints on Dark Matter with Gravitationally Lensed Fast Radio Bursts Detected by BURSTT
• A Gaia Data Release 3 View on the Tip of the Red Giant Branch Luminosity
• Hamilton's Object -- a clumpy galaxy straddling the gravitational caustic of a galaxy cluster : Constraints on dark matter clumping
• A comparison between axion-like and power law potentials in cosmological background
• Geometrical origins of the Universe dark sector: string-inspired torsion and anomalies as seeds for inflation and dark matter
• Velocity Dispersions of Clusters in the Dark Energy Survey Y3 redMaPPer Catalog
• Sunyaev-Zel'dovich effect and X-ray scaling relations of galaxies, groups and clusters in the IllustrisTNG simulations
• A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA
• LADDER: Revisiting the Cosmic Distance Ladder with Deep Learning Approaches and Exploring its Applications
• Cosmic Growth in $f(T)$ Teleparallel Gravity
• Calibration of Surface Brightness Fluctuations for Dwarf Galaxies in the Hyper Suprime-Cam $gi$ Filter System
• Dynamical consistency conditions for rapid turn inflation
• The eROSITA Final Equatorial-Depth Survey (eFEDS): A complete census of X-ray properties of Subaru Hyper Suprime-Cam weak lensing shear-selected clusters in the eFEDS footprint
• Probing the two-body decaying dark matter scenario with weak lensing and the cosmic microwave background
• Impact of the damping tail on neutrino mass constraints
• Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?
• Analysis of the apparent lack of power in the cosmic microwave background anisotropy at large angular scales
• Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
• The Atacama Cosmology Telescope: limits on dark matter-baryon interactions from DR4 power spectra
• Family dispute: do Type IIP supernova siblings agree on their distance?
• Finding origins of CMB anomalies in the inflationary quantum fluctuations
• Pantheon+ constraints on dark energy and modified gravity: An evidence of dynamical dark energy
• Refined modelling of the radio SZ signal: kinematic terms, relativistic temperature corrections and anisotropies in the radio background
• Consistency of Pantheon+ supernovae with a large-scale isotropic universe
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Structure Formation Paradigm and Axion Quark Nugget dark matter model
• Bayesian analysis of a Unified Dark Matter model with transition: can it alleviate the $H_0$ tension?
• A roadmap to cosmological parameter analysis with third-order shear statistics III: Efficient estimation of third-order shear correlation functions and an application to the KiDS-1000 data
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Cosmology in the Lorentz gauge theory
• Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS II. Deciphering Gaia parallax systematics using red clump stars
• Field-level inference of cosmic shear with intrinsic alignments and baryons
• On the interacting dark energy scenarios $-$ the case for Hubble constant tension
• Stochastic star formation and the abundance of $z>10$ UV-bright galaxies
• Cosmological Implications of the String Theory Landscape
• Viability of the Matter Bounce Scenario
• Cosmological constraints using Minkowski functionals from the first year data of the Hyper Suprime-Cam
• Inflation Driven by Non-Linear Electrodynamics
• Measuring the distortion of time with relativistic effects in large-scale structure
• Role of the Hubble Scale in the Weak Lensing vs. CMB Tension
• Spatial Curvature and Thermodynamics
• BAO cosmology in non-spatially flat background geometry from BOSS+eBOSS and lessons for future surveys
• Fast Radio Bursts as probes of the late-time universe: a new insight on the Hubble tension
• Disentangling Doppler modulation, aberration and the temperature dipole in the CMB
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Constraining Self-interacting Scalar Field Dark Matter From the Black Hole Shadow of the Event Horizon Telescope
• The evolution of high-density cores of the BOSS Great Wall superclusters
• Reeling in the Whirlpool: the distance to M 51 clarified by Cepheids and the Type IIP SN 2005cs
• Testing anisotropic Hubble expansion
• The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
• Gravitational Wave from Axion-SU(2) Gauge Fields: Effective Field Theory for Kinetically Driven Inflation
• Discrepancy between cosmological and electroweak observables in Higgs Inflation
• Observational Evidence for Negative-Energy Dust in Late-Times Cosmology
• Photometric redshifts and intrinsic alignments: degeneracies and biases in 3$\times$2pt analysis
• Possible evidence for a large-scale enhancement in the Lyman-$\alpha$ forest power spectrum at redshift $\text{z}\ge 4$
• An empirical approach to model selection: weak lensing and intrinsic alignments
• The CMB Cold Spot as predicted by foregrounds around nearby galaxies
• Non-oscillating Early Dark Energy and Quintessence from Alpha-Attractors
• Thin-wall vacuum decay in the presence of a compact dimension meets the $H_0$ and $S_8$ tensions
• Quantifying the tension between cosmological models and JWST red candidate massive galaxies
• A generalized mass-to-horizon relation: a new global approach to entropic cosmologies and its connection to $\Lambda$CDM
• Fast Radio Bursts and Artificial Neural Networks: a cosmological-model-independent estimation of the Hubble Constant
• Optical interferometry and Gaia measurement uncertainties reveal the physics of asymptotic giant branch stars
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• A Framework for Obtaining Accurate Posteriors of Strong Gravitational Lensing Parameters with Flexible Priors and Implicit Likelihoods using Density Estimation
• Big bang nucleosynthesis and early dark energy in light of the EMPRESS $Y_p$ results and the $H_0$ tension
• Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology
• Quantum kinetic theory of Jeans instability in non-minimal matter-curvature coupling gravity
• Cosmology in a reduced Born-Infeld--$f(T)$ theory of gravity
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Quark stars with isotropic matter in Hořava gravity and Einstein-æther theory
• $f(T)$ cosmology in the regime of quasar observations
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Tachyon inflation in an AdS braneworld with back-reaction
• Integrated photometry of multiple stellar populations in Globular Clusters
• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• Interacting Scalar fields: Dark matter and early dark energy
• Search for the $f(R,T)$ gravity functional form via gaussian processes
• Paths to gravitation via the gauging of parameterized field theories
• On How to Extend the NIR Tully-Fisher Relation to be Truly All-Sky
• Apercal -- The Apertif Calibration Pipeline
• Unveiling the largest structures in the nearby Universe: Discovery of the Quipu superstructure
• A MeerKAT, e-MERLIN, H.E.S.S. and Swift search for persistent and transient emission associated with three localised FRBs
• A theoretical estimate of intrinsic ellipticity bispectra induced by angular momenta alignments
• Dissecting a miniature universe: A multi-wavelength view of galaxy quenching in the Shapley supercluster
• Deep Neural Networks for Estimation of Gamma-Ray Burst Redshifts
• Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
• Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from MgII and CIV reverberation-mapped quasar data
• DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
• $f(T)$ Cosmology with Nonzero Curvature
• Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems using Recurrent Inference Machines
• Neutrino astronomy as a probe of physics beyond the Standard Model: decay of sub-MeV $B$-$L$ gauge boson dark matter
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Tsallis holographic dark energy with power law ansatz approach
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term
• Axion gravitodynamics, Lense-Thirring effect, and gravitational waves
• Structure Formation in Various Dynamical Dark Energy Scenarios
• The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey II: Unveiling a pancake structure with a 100 Mpc radius in the local Universe
• Reassessment of the dipole in the distribution of quasars on the sky
• Consistent Constraints on the Equivalence Principle from localised Fast Radio Bursts
• Clustering of CODEX clusters
• The Wide-field Spectroscopic Telescope (WST) Science White Paper
• Axial Ratio of Edge-On Spiral Galaxies as a Test For Extended Bright Radio Halos
• First constraints on non-minimally coupled Natural and Coleman-Weinberg inflation and massive neutrino self-interactions with Planck+BICEP/Keck
• LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
• Reconstructing the growth index $\gamma$ with Gaussian Processes
• Irreversible Geometrothermodynamics of Open Systems in Modified Gravity
• New insights on $\nu$-DM Interactions
• Period-Luminosity Relations for Galactic classical Cepheids in the Sloan bands
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• Cosmological Distances And Hubble Tension In Einstein-Cartan Theory
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• A Cosmological Unicorn Solution to Finsler Gravity
• Continuous gravitational wave detection to understand the generation mechanism of fast radio bursts
• Standardized Luminosity of the Tip of the Red Giant Branch utilizing Multiple Fields in NGC 4258 and the CATs Algorithm
• Fast and effortless computation of profile likelihoods using CONNECT
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Checking the second law at cosmic scales
• Complementary Probes of Two-component Dark Matter
• Detection of ${}^7$Be II in the Small Magellanic Cloud
• JWST high redshift galaxy observations have a strong tension with Planck CMB measurements
• Can the Local Bubble explain the radio background?
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• Warm inflation with non-comoving scalar field and radiation fluid
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Constraints on the speed of sound in the k-essence model of dark energy
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Viewing angle observations and effects of evolution with redshift, black hole mass, and Eddington ratio in quasar based cosmology
• Fundamental Physics with ESPRESSO, Constraining a simple parametrisation for varying $\alpha$
• Robust constraints on tensor perturbations from cosmological data: a comparative analysis from Bayesian and frequentist perspectives
• A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
• Solar chameleons: Novel channels
• A possible late-time transition of $M_B$ inferred via neural networks
• Tomographic redshift dipole: Testing the cosmological principle
• New calibrated models for the TRGB luminosity and a thorough analysis of theoretical uncertainties
• Weak-Lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: II. Cosmological Constraints from the Cluster Abundance
• Dark Energy Survey Year 3: Blue Shear
• Testing $\alpha$-attractor quintessential inflation against CMB and low-redshift data
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
• Explanation of high redshift luminous galaxies from JWST by early dark energy model
• A generalized uncertainty-inspired quantum black hole
• Is cosmological data suggesting a nonminimal coupling between matter and gravity?
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• Runaway dilaton models: improved constraints from the full cosmological evolution
• Generalised model-independent characterisation of strong gravitational lenses VIII. automated multi-band feature detection to constrain local lens properties
• What if Newton's Gravitational Constant was negative?
• Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
• Probing the anisotropic distribution of baryon matter in the Universe using fast radio bursts
• Particle creation and reheating in a braneworld inflationary scenario
• Exploiting the diversity of modeling methods to probe systematic biases in strong lensing analyses
• Data-driven and Almost Model-independent Reconstruction of Modified Gravity
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Revisiting dark energy models using differential ages of galaxies
• The interacting vacuum and tensions: a comparison of theoretical models
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Searching for TeV Dark Matter in Irregular dwarf galaxies with HAWC Observatory
• Scaling solutions as Early Dark Energy resolutions to the Hubble tension
• A closer look at dark photon explanations of the excess radio background
• PROBES-I: A Compendium of Deep Rotation Curves and Matched multiband Photometry
• Constraints on extended Bekenstein models from cosmological, astrophysical, and local data
• The low multipoles in the Pantheon+SH0ES data
• Searching for local features in primordial power spectrum using genetic algorithms
• Chameleon Mechanism in Scalar Nonmetricity Cosmology
• Towards early-type eclipsing binaries as extragalactic milestones: II. NLTE spectral analysis and stellar parameters of the detached O-type system OGLE-LMC-ECL-06782 in the LMC
• Can Early Dark Energy be Probed by the High-Redshift Galaxy Abundance?
• Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys
• Model selection and parameter estimation using the iterative smoothing method
• Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
• Gravitational particle production and the Hubble tension
• Calibration of the Tully-Fisher relation in the WISE W1 ($3.4\mu \mathrm{m}$) and W2 ($4.6\mu \mathrm{m}$) Bands
• Hubble constant by natural selection: Evolution chips in the Hubble tension
• Determining the Hubble Constant with AGN-assisted Black Hole Mergers
• Cosmic voids and the kinetic analysis. III. Hubble tension and structure formation in the late Universe
• Relic neutrino decay solution to the excess radio background
• A study of Dipolar Signal in distant Quasars with various observables
• A Non-parametric Reconstruction of the Hubble Parameter $H(z)$ Based on Radial Basis Function Neural Networks
• Modelling the emergence of cosmic anisotropy from non-linear structures
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
• Hamiltonian formulation of gravity as a spontaneously-broken gauge theory of the Lorentz group
• Oscillations of sterile neutrinos from dark matter decay eliminates the IceCube-Fermi tension
• Einstein-aether theory in Weyl integrable geometry
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• A search for the fine-structure constant evolution from fast radio bursts and type Ia supernovae data
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