In the Realm of the Hubble tension $-$ a Review of Solutions

Abstract

The $\Lambda$CDM model provides a good fit to a large span of cosmological data but harbors areas of phenomenology. With the improvement of the number and the accuracy of observations, discrepancies among key cosmological parameters of the model have emerged. The most statistically significant tension is the $4-6\sigma$ disagreement between predictions of the Hubble constant $H_0$ by early time probes with $\Lambda$CDM model, and a number of late time, model-independent determinations of $H_0$ from local measurements of distances and redshifts. The high precision and consistency of the data at both ends present strong challenges to the possible solution space and demand a hypothesis with enough rigor to explain multiple observations--whether these invoke new physics, unexpected large-scale structures or multiple, unrelated errors. We present a thorough review of the problem, including a discussion of recent Hubble constant estimates and a summary of the proposed theoretical solutions. Some of the models presented are formally successful, improving the fit to the data in light of their additional degrees of freedom, restoring agreement within $1-2\sigma$ between {\it Planck} 2018, using CMB power spectra data, BAO, Pantheon SN data, and R20, the latest SH0ES Team measurement of the Hubble constant ($H_0=73.2\pm 1.3\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$ at 68\% confidence level). Reduced tension might not simply come from a change in $H_0$ but also from an increase in its uncertainty due to degeneracy with additional physics, pointing to the need for additional probes. While no specific proposal makes a strong case for being highly likely or far better than all others, solutions involving early or dynamical dark energy, neutrino interactions, interacting cosmologies, primordial magnetic fields, and modified gravity provide the best options until a better alternative comes along.[Abridged]

Invited Review of about 134 pages with many figures and tables. Accepted for publication in CQG. A sample code for producing similar whisker plots (e.g. Figs. 1, 2) associated with this Review for any choice of the data is made publicly available online at: https://github.com/lucavisinelli/H0TensionRealm

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• Early-Universe-Physics Insensitive and Uncalibrated Cosmic Standards: Constraints on ${\Omega }_{\mathrm{m}}$ and Implications for the Hubble Tension
• Updated constraints from the effective field theory analysis of BOSS power spectrum on Early Dark Energy
• Black Holes in $f(T,B)$ Gravity: Exact and Perturbed Solutions
• Observational constraints on the deceleration parameter in a tilted universe
• No-go guide for the Hubble tension : Late-time solutions
• The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation
• Standardized long gamma-ray bursts as a cosmic distance indicator
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
• Reconstruction of $\Lambda$CDM Universe in $f(Q)$ Gravity
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Late time interacting cosmologies and the Hubble constant tension
• BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
• $f(R)$ gravity in the Jordan Frame as a Paradigm for the Hubble Tension
• Revealing the effects of curvature on the cosmological models
• Model-agnostic assessment of dark energy after DESI DR1 BAO
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• STRIDES: Automated uniform models for 30 quadruply imaged quasars
• Non-Gaussian estimates of tensions in cosmological parameters
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Cosmological observational constraints on the power law $f(Q)$ type modified gravity theory
• An Improved Calibration of the Wavelength Dependence of Metallicity on the Cepheid Leavitt law
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Testing spatial curvature and anisotropic expansion on top of the $\Lambda$CDM model
• Cosmology under the fractional calculus approach
• Gaussian processes and effective field theory of $f(T)$ gravity under the $H_0$ tension
• Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• Isotropic cosmic birefringence from early dark energy
• Perturbations in Non-Flat Cosmology for $f(T)$ gravity
• Breakdown of the Newton-Einstein Standard Gravity at Low Acceleration in Internal Dynamics of Wide Binary Stars
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Hot New Early Dark Energy
• A double take on early and interacting dark energy from JWST
• Unveiling dark fifth forces with linear cosmology
• A tale of two (or more) $h$'s
• Health checkup test of the standard cosmological model in view of recent Cosmic Microwave Background Anisotropies experiments
• Model-independent cosmological inference post DESI DR1 BAO measurements
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• Towards hybrid inflation with $n_s=1$ in light of Hubble tension and primordial gravitational waves
• Probing elastic interactions in the dark sector and the role of $S_8$
• Unveiling Hidden Physics at the LHC
• Novel cosmological bounds on thermally-produced axion-like particles
• Magnetic Reconnection and Energy Extraction from a Spinning Black Hole with Broken Lorentz Symmetry
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• The resilience of the Etherington-Hubble relation
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Equation of state of the running vacuum
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Simple-graduated dark energy and spatial curvature
• Mirror Twin Higgs Cosmology: Constraints and a Possible Resolution to the $H_0$ and $S_8$ Tensions
• Hints for a gravitational constant transition in Tully-Fisher data
• Chain Early Dark Energy: Solving the Hubble Tension and Explaining Today's Dark Energy
• Neural Network Reconstruction of Late-Time Cosmology and Null Tests
• $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• Strong gravitational lensing and microlensing of supernovae
• Probing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Revealing the late-time transition of $H_0$: relieve the Hubble crisis
• Multi-interacting dark energy and its cosmological implications
• $S_8$ increases with effective redshift in $\Lambda$CDM cosmology
• Is the Harrison-Zel'dovich spectrum coming back? ACT preference for $n_s\sim 1$ and its discordance with Planck
• Late-Time constraints on Interacting Dark Energy: Analysis independent of $H_0$, $r_d$ and $M_B$
• Homogeneous and isotropic cosmology in general teleparallel gravity
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Very Hairy Inflation
• Mirror QCD phase transition as the origin of the nanohertz Stochastic Gravitational-Wave Background
• Interacting dark energy: clarifying the cosmological implications and viability conditions
• Evaluating bulk flow estimators for CosmicFlows-4 measurements
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data
• What it takes to solve the Hubble tension through modifications of cosmological recombination
• Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Measuring the Hubble constant with black sirens
• Project Dinos I: A joint lensing-dynamics constraint on the deviation from the power law in the mass profile of massive ellipticals
• Towards a model-independent reconstruction approach for late-time Hubble data
• Observational Constraints and Cosmological Implications of Scalar-Tensor $f(R,T)$ Gravity
• Accelerating cosmological models in $f(Q)$ gravity and the phase space analysis
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• Is the dark energy equation of state parameter singular?
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• On the dynamics of a dark sector coupling
• The Mira Distance to M101 and a 4% Measurement of H0
• Metric $f(R)$ gravity with dynamical dark energy as a scenario for the Hubble tension
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Late time acceleration due to generic modification of gravity and Hubble tension
• Constraints on Primordial-black-hole Population and Cosmic Expansion History from GWTC-3
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• Gamma ray burst constraints on cosmological models from the improved Amati correlation
• Quantifying the global "CMB tension" between the Atacama Cosmology Telescope and the Planck satellite in extended models of cosmology
• Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
• Slow-rolling scalar dynamics and as solution for the Hubble tension
• Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Intrinsic tension in the supernova sector of the local Hubble constant measurement and its implications
• The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision
• Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension
• The DES view of the Eridanus supervoid and the CMB Cold Spot
• The Interplay between the Dark Matter Axion and Primordial Black Holes
• Priors on red galaxy stochasticity from hybrid effective field theory
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
• Cosmological constraints on ${\Lambda }_{\mathrm{s}}$CDM scenario in a type II minimally modified gravity
• Cosmic expansion parametrization: Implication for curvature and ${\text{H}}_0$ tension
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
• An Effective Sign Switching Dark Energy: Lotka-Volterra Model of Two Interacting Fluids
• A test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• String Tension between de Sitter vacua and Curvature Corrections
• Model-independent versus model-dependent interpretation of the SDSS-III BOSS power spectrum: Bridging the divide
• Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data
• Reconstruction of the dark sectors' interaction: A model-independent inference and forecast from GW standard sirens
• No H_0 Assistance from Assisted Quintessence
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Testing dark energy after pre-recombination early dark energy
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• Landau damping for gravitational waves in parity-violating theories
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Smoothing the $H_0$ tension with a dynamical dark energy model
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Do you smell something decaying? Updated linear constraints on decaying dark matter scenarios
• The Simplest and Most Predictive Model of Muon $g-2$ and Thermal Dark Matter
• Microphysics of Early Dark Energy
• Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
• Yoga Dark Energy: Natural Relaxation and Other Dark Implications of a Supersymmetric Gravity Sector
• An effective description of Laniakea: impact on cosmology and the local determination of the Hubble constant
• Background evolution and growth of structures in interacting dark energy through dynamical system analysis
• Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters
• Precision CMB constraints on eV-scale bosons coupled to neutrinos
• Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
• Measuring the reionization optical depth without large-scale CMB polarization
• Exploiting the Einstein Telescope to solve the Hubble tension
• Dipole Cosmology: The Copernican Paradigm Beyond FLRW
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• Cosmographic view on the $H_0$ and ${\sigma }_8$ tensions
• Constraints on $f(T)$ Cosmology with Pantheon+
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Thin accretion discs around spherically symmetric configurations with nonlinear scalar fields
• SICRET: Supernova Ia Cosmology with truncated marginal neural Ratio EsTimation
• Model independent bounds on Type Ia supernova absolute peak magnitude
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Observational constraints on the equation of state of viscous fluid in $f(R,T)$ gravity
• Observational Constraints on $f(T)$ Gravity from Model-Independent Data
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• An exploration of an early gravity transition in light of cosmological tensions
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• Revisiting Fractional Cosmology
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension
• $H_0$ Tension in Torsion-based Modified Gravity
• Inevitable manifestation of wiggles in the expansion of the late Universe
• Measuring Hubble constant using localized and unlocalized fast radio bursts
• A comprehensive numerical study on four categories of holographic dark energy models
• Gamma-ray Cosmology and Tests of Fundamental Physics
• RR Lyrae-based Distances for 39 Nearby Dwarf Galaxies Calibrated to Gaia eDR3
• The TRGB-SBF Project. III. Refining the HST Surface Brightness Fluctuation Distance Scale Calibration with JWST
• Probing Early Modification of Gravity with Planck, ACT and SPT
• The period--luminosity relation for Mira variables in the Milky Way using Gaia DR3: a further distance anchor for $H_0$
• Constraining the dark-energy equation of state with cosmological data
• Interacting Dark Sectors in light of DESI DR2
• Physical vs phantom dark energy after DESI: thawing quintessence in a curved background
• Spherically symmetric vacuum solutions in 1-Parameter New General Relativity and their phenomenology
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• Exploring the Hubble tension with a late time Modified Gravity scenario
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Can varying the gravitational constant alleviate the tensions ?
• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• The perspective of voids on rising cosmology tensions
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Euclid: Forecast constraints on consistency tests of the $\Lambda$CDM model
• Axion Homeopathy: Screening Dilaton Interactions
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• CMB Anomalies and the Hubble Tension
• Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• Dynamical systems analysis of $f(Q)$ gravity
• A Cosmological Underdensity Does Not Solve the Hubble Tension
• Phantom scalar-tensor models and cosmological tensions
• ${\Lambda }_{\mathrm{s}}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Implications of an extended dark energy model with massive neutrinos
• Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
• Neural Network Reconstruction of $H^{\prime }(z)$ and its application in Teleparallel Gravity
• Minimal theory of massive gravity in the light of CMB data and the $S_8$ tension
• Do reverberation-measured H$\beta$ quasars provide a useful test of cosmology?
• Consistency study of high- and low-accreting Mg ii quasars: No significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity relation dispersion
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Exact solutions and cosmological constraints in fractional cosmology
• How the Big Bang Ends up Inside a Black Hole
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• New cosmological constraints on $f(T)$ gravity in light of full Planck-CMB and type Ia supernovae data
• Addressing the Hubble and $S_8$ Tensions with a Kinetically Mixed Dark Sector
• Dark energy in conformal Killing gravity
• Towards a possible solution to the Hubble tension with Horndeski gravity
• Low-redshift estimates of the absolute scale of baryon acoustic oscillations
• Gravitational transitions via the explicitly broken symmetron screening mechanism
• The distribution of galaxy rotation in JWST Advanced Deep Extragalactic Survey
• Linear stability of black holes with static scalar hair in full Horndeski theories: generic instabilities and surviving models
• Novel constraints on fifth forces and ultralight dark sector with asteroidal data
• Observational Constraints on Dynamical Dark Energy Models
• Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
• Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
• Cosmological constraints on dark energy models using DESI BAO 2024
• Probing neutrino interactions and dark radiation with gravitational waves
• Torsion in string-inspired cosmologies and the universe dark sector
• Alleviating $H_0$ Tension with New Gravitational Scalar Tensor Theories
• Quintessential Cosmological Tensions
• Toward a concordance teleparallel Cosmology II: Linear perturbation
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• The HETDEX Survey: Emission Line Exploration and Source Classification
• Testing an oscillatory behavior of dark energy
• Phantom braneworld and the Hubble tension
• Non-Gaussianity constraints from Planck spectral distortion cross-correlations
• Galaxy-Scale Test of General Relativity with Strong Gravitational Lensing
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Searching for Heavy Leptophilic $Z^{\prime }$: from Lepton Colliders to Gravitational Waves
• A short review on clustering dark energy
• Cosmological dynamical systems in modified gravity
• On Zero Point Calibration of the Red Giant Branch Tip in the Magellanic Clouds
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Alleviating $H_0$ tension in Horndeski gravity
• Supernovae evidence for foundational change to cosmological models
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• No-go guide for the Hubble tension: late-time or local-scale new physics
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Constraining a late time transition of $G_{\mathrm{eff}}$ using low-z galaxy survey data
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• Solving the $H_0$ tension in $f(T)$ Gravity through Bayesian Machine Learning
• Primordial Black Holes and Gravitational Waves in Multi-Axion-Chern-Simons Inflation
• Dynamical Stability in presence of non-minimal derivative dependent coupling of $k$-essence field with a relativistic fluid
• Mapping the ${\Lambda }_{\mathrm{s}}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate
• Exploring new physics in the late Universe's expansion through non-parametric inference
• A search for sterile neutrinos in interacting dark energy models using DESI baryon acoustic oscillations and DES supernovae data
• Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature
• The effect of outflows on CMB bounds from Primordial Black Hole accretion
• Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data
• Constraints on $f(Q)$ logarithmic model using gravitational wave standard sirens
• Dark matter produced from right-handed neutrinos
• Analyzing the Hubble tension through hidden sector dynamics in the early universe
• Redshift drift cosmography for model-independent cosmological inference
• Running vacuum in Brans-Dicke theory: a possible cure for the ${\sigma }_8$ and $H_0$ tensions
• Two sides of the same coin: sterile neutrinos and dark radiation. Status and perspectives
• Modified recombination and the Hubble tension
• Evolving Dark Energy or Evolving Dark Matter?
• Quasi-local masses and cosmological coupling of black holes and mimickers
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Well-Tempered Minkowski Solutions in Teleparallel Horndeski Theory
• Coupled Multi Scalar Field Dark Energy
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• A note on interacting holographic dark energy with a Hubble-scale cutoff
• Hubble tension and absolute constraints on the local Hubble parameter
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Consistency tests between SDSS and DESI BAO measurements
• jetsimpy: A Highly Efficient Hydrodynamic Code for Gamma-ray Burst Afterglow
• The Unsettled Number: Hubble's Tension
• Running vacuum versus Holographic dark energy: a cosmographic comparison
• $U(1{)}_{L_{\mu }-L_{\tau }}$ for Light Dark Matter, $g_{\mu }-2$, the $511$ keV excess and the Hubble Tension
• Dark Energy within the Generalized Uncertainty Principle in Light of DESI DR2
• A framework for the next generation of stationary cosmological models
• Measuring Hubble constant in an anisotropic extension of $\Lambda$CDM model
• Gravitational-wave dark siren cosmology systematics from galaxy weighting
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• Measuring the Hubble Constant with cosmic chronometers: a machine learning approach
• Supernova Limits on Muonic Dark Forces
• TDCOSMO VIII: Cosmological distance measurements in light of the mass-sheet degeneracy -- forecasts from strong lensing and IFU stellar kinematics
• Neural network reconstruction of cosmology using the Pantheon compilation
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• Shedding Light on Dark Matter and Neutrino Interactions from Cosmology
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Cosmological Perturbation Theory in Metric-Affine Gravity
• Cosmological foundations revisited with Pantheon+
• The Heisenberg limit at cosmological scales
• Decay of multiple dark matter particles to dark radiation in different epochs does not alleviate the Hubble tension
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
• Does DESI DR2 challenge $\Lambda$CDM paradigm ?
• Dynamics in interacting scalar-torsion theory
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Unifying Inflation with early and late Dark Energy in Multi-Fields: Spontaneously broken scale invariant TMT
• Alleviating $H_0$ tension in scalar-tensor and bi-scalar-tensor theories
• A critical discussion on the $H_0$ tension
• Barrow and Tsallis entropies after the DESI DR2 BAO data
• Improved null tests of $\Lambda$CDM and FLRW in light of DESI DR2
• Modified gravity in the presence of matter creation: scenario for the late Universe
• Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2
• The $S_8$ Tension in Light of Updated Redshift-Space Distortion Data and PAge Approximation
• Nonsingular Cosmology from an Interacting Vacuum
• Can the Hubble tension be resolved by bulk viscosity?
• Unbiased likelihood-free inference of the Hubble constant from light standard sirens
• Cosmological models in scale-independent energy-momentum squared gravity
• Towards a Realistic Model of Dark Atoms to Resolve the Hubble Tension
• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• General Effective Field Theory of Teleparallel Gravity
• A New Test of Dynamical Dark Energy Models and Cosmic Tensions in Hořava Gravity
• Cosmology from weak lensing alone and implications for the Hubble tension
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• Resonant neutrino self-interactions and the $H_0$ tension
• The first variation of the matter energy-momentum tensor with respect to the metric, and its implications on modified gravity theories
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• Interacting dark sector from the trace-free Einstein equations: cosmological perturbations with no instability
• Reassessing the Constraints from SH0ES Extragalactic Cepheid Amplitudes on Systematic Blending Bias
• Cosmological constraints on dynamical dark energy model in $F(Q)$ gravity
• Consistent extinction model for type Ia supernovae in Cepheid-based calibration galaxies and its impact on $H_0$
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Probing Cosmology with 92 Localized Fast Radio Bursts and DESI BAO
• Machine learning cosmic backreaction and its effects on observations
• Cosmic backreaction and the mean redshift drift from symbolic regression
• Tracking the Multifield Dynamics with Cosmological Data: A Monte Carlo approach
• Foundations of ghost stability
• Ghost and Laplacian Instabilities in the Teleparallel Horndeski Gravity
• Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
• Phenomenological Gravitational Phase Transition: Early and Late Modifications
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• Scalar-Tensor Gravity and DESI 2024 BAO data
• Cosmological implications of Rastall-$f(R)$ theory
• Relativistic corrections for measuring Hubble's constant to 1% using stellar standard candles
• Unified $f(R)$ gravity at local scales
• Noether Symmetry Approach in Scalar-Torsion $f(T,\varphi )$ Gravity
• The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
• Baryon acoustic oscillations in thin redshift shells from BOSS DR12 and eBOSS DR16 galaxies
• Addressing Cosmological Tensions by Non-Local Gravity
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Unexplored regions in teleparallel $f(T)$ gravity: Sign-changing dark energy density
• Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs
• Observational constraints on soft dark energy and soft dark matter: challenging $\Lambda$CDM
• f(T) cosmology against the cosmographic method: A new study using mock and observational data
• Stability of $f(Q,B)$ Gravity via Dynamical System Approach: a Comprehensive Bayesian Statistical Analysis
• Observational bounds on extended minimal theories of massive gravity: New limits on the graviton mass
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• Constraining $\Lambda$CDM cosmological parameters with Einstein Telescope mock data
• Updating constraints on phantom crossing $f(T)$ gravity
• A quantum state for the late Universe
• A null test of the Cosmological Principle with BAO measurements
• Tip of the Red Giant Branch Distances with JWST. II. I-band Measurements in a Sample of Hosts of 10 SN Ia Match HST Cepheids
• A Model-independent Method to Determine $H_0$ Using Time-Delay Lensing, Quasars and Type Ia Supernovae
• Testing a varying-$\Lambda$ model for dark energy within Co-varying Physical Couplings framework
• D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models
• Hubble tension in a nonminimally coupled curvature-matter gravity model
• Stability of symmetric teleparallel scalar-tensor cosmologies with alternative connections
• Reconciling early dark energy with a Harrison-Zeldovich spectrum
• A novel model-marginalized cosmological bound on the QCD axion mass
• Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag
• Cosmography of the Local Universe by Multipole Analysis of the Expansion Rate Fluctuation Field
• Hubble tension as a window on the gravitation of the dark matter sector
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Type Ia supernovae data with scalar-tensor gravity
• Geometrical origins of the Universe dark sector: string-inspired torsion and anomalies as seeds for inflation and dark matter
• Mori-Zwanzig formalism for general relativity: a new approach to the averaging problem
• Can decaying dark matter scenarios alleviate both $H_0$ and ${\sigma }_8$ tensions?
• Testing the $\Lambda$CDM paradigm with growth rate data and machine learning
• Neutrino mass tension or suppressed growth rate of matter perturbations?
• New cosmological constraints on the evolution of dark matter energy density
• A test of the standard dark matter density evolution law using galaxy clusters and cosmic chronometers
• Testing Quintessence Axion Dark Energy with Recent Cosmological Results
• Positive neutrino masses with DESI DR2 via matter conversion to dark energy
• Measuring the cosmic expansion rate using 21-cm velocity acoustic oscillations
• A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data
• Phase-space analysis of dark energy models in non-minimally coupled theories of gravity
• Testing the Cosmic Distance Duality Relation Using Strong Gravitational Lensing Time Delays and Type Ia Supernovae
• The variance of the CMB temperature gradient: a new signature of a multiply connected Universe
• Cuscuta-Galileon cosmology: Dynamics, gravitational "constant"s and the Hubble Constant
• Exploring the Growth Index ${\gamma }_L$: Insights from Different CMB Dataset Combinations and Approaches
• A comparison between axion-like and power law potentials in cosmological background
• LADDER: Revisiting the Cosmic Distance Ladder with Deep Learning Approaches and Exploring its Applications
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals
• A peek outside our Universe
• Cosmology with viscous generalized Chaplygin gas in $f(Q)$ gravity
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• Testing scale-invariant inflation against cosmological data
• Finding origins of CMB anomalies in the inflationary quantum fluctuations
• Cosmology in the Lorentz gauge theory
• Past-directed scalar field gradients and scalar-tensor thermodynamics
• Superhorizon perturbations: A possible explanation of the Hubble--Lemaître Tension and the Large Scale Anisotropy of the Universe
• A short survey of matter-antimatter evolution in the primordial universe
• Environment Dependent Electron Mass and the H${}_0$-Tension
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• On the interacting dark energy scenarios $-$ the case for Hubble constant tension
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Axion Dark Radiation: Hubble Tension and Hyper-kamiokande Neutrino Experiment
• Early Dark Energy from a Higher-dimensional Gauge Theory
• Constraints on Cosmological Models from Quasars Calibrated with Type Ia Supernova by a Gaussian Process
• Was Entropy Conserved between BBN and Recombination?
• Can dark matter-dark energy interaction alleviate the Cosmic Coincidence Problem?
• In search of an interaction in the dark sector through Gaussian Process and ANN approaches
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• On dataset tensions and signatures of new cosmological physics
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• Multi-component DHOST analysis in galaxy clusters
• Fast Radio Bursts and Artificial Neural Networks: a cosmological-model-independent estimation of the Hubble Constant
• Torsion at different scales: from materials to the Universe
• Using machine learning to compress the matter transfer function $T(k)$
• Tracing cosmic evolution through Weyl-Type f(Q,T) gravity model: theoretical analysis and observational validation
• Noether Symmetries in $f(T,T_G)$ Cosmology
• Hubble distancing: Focusing on distance measurements in cosmology
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• Neutron Stars in Modified Teleparallel Gravity
• Fast Radio Bursts as probes of the late-time universe: a new insight on the Hubble tension
• A single parameterization for dark energy and modified gravity models
• $H_0$ tension without CMB data: beyond the $\Lambda$CDM
• Cosmology of an Axion-Like Majoron
• Lifshitz cosmology: quantum vacuum and Hubble tension
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• Constraints on Dark Energy Models Using Late Universe Probes
• Thin-wall vacuum decay in the presence of a compact dimension meets the $H_0$ and $S_8$ tensions
• TDCOSMO XV: Population Analysis of Lines of Sight of 25 Strong Galaxy-Galaxy Lenses with Extreme Value Statistics
• On finite time singularities in scalar field dark energy models based in the RS-II Braneworld
• A unified TDiff invariant field theory for the dark sector
• Geodesic deviation in Saez--Ballester theory
• Tachyonic cosmology with cubic contractions of the Riemann tensor
• Accelerating cosmology from $\Lambda <0$ gravitational effective field theory
• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• Project Dinos II: Redshift evolution of dark and luminous matter density profiles in strong-lensing elliptical galaxies across 0.1 < z < 0.9
• Dynamical analysis of logarithmic energy-momentum squared gravity
• Minisuperspace Quantization of $f\left(T,B\right)$ Cosmology
• Big bang nucleosynthesis and early dark energy in light of the EMPRESS $Y_p$ results and the $H_0$ tension
• Non-unitary three-neutrino mixing in the early Universe
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Cosmological implications of the Weyl geometric gravity theory
• Dark matter from torsion in Friedmann cosmology
• Investigating The Hubble Tension Through Hubble Parameter Data
• Cosmological Parameter Estimation Using Current and Future Observations of Strong Gravitational Lensing
• Does the fraction of dark matter diminish with early dark energy?
• f(R) Gravity in an Ellipsoidal Universe
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• Early dark energy constraints with late-time expansion marginalization
• Cosmology with supernova Encore in the strong lensing cluster MACS J0138-2155: Lens model comparison and H0 measurement
• Structure formation in an anisotropic universe: Eulerian perturbation theory
• Cosmic voids and the kinetic analysis
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Primordial power spectra from $k$-inflation with curvature
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Unveiling the Hubble Constant through Galaxy Cluster Gas Mass Fractions
• Cuspy dark matter density profiles in massive dwarf galaxies
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Linear matter density perturbations in the ${\Lambda }_{\mathrm{s}}$CDM model: Examining growth dynamics and addressing the $S_8$ tension
• Conformal and Non-Minimal Couplings in Fractional Cosmology
• Spatial curvature sensitivity to local $H_0$ from the Cepheid distance ladder
• Gravitational metamaterials from optical properties of spacetime media
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Early dark energy and the screening mechanism
• $f(T,B)$ Gravity in the late Universe in the context of local measurements
• Towards a Solution to the H0 Tension: the Price to Pay
• $f(T)$ Cosmology with Nonzero Curvature
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Measuring neutrino masses with joint JWST and DESI DR2 data
• Rotating Kerr-Newman space-times in Metric-Affine Gravity
• Gravitational waves in higher-order $R^2$ gravity
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• Observational constraints on varying fundamental constants in a minimal CPC model
• Narrowing down the Hubble tension to the first two rungs of distance ladders
• Two per cent measurement of $H_0$ from Cepheids alone
• Cosmological Tests of Gravity: A Future Perspective
• Length-preserving biconnection gravity and its cosmological implications
• Testing $\alpha$-attractor quintessential inflation against CMB and low-redshift data
• A study of interacting scalar field model from the perspective of the dynamical systems theory
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• Probing Dark Sectors with Neutron Stars
• $f(T,B)$ gravity in a Friedmann-Lema\^ıtre-Robertson-Walker universe with nonzero spatial curvature
• Cosmographic analysis of sign-switching dark energy
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• New conservation laws and exact cosmological solutions in Brans-Dicke cosmology with an extra scalar field
• Variation of the fine structure constant in the light of recent helium abundance measurement
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• Shan--Chen interacting vacuum cosmology
• One-parameter dynamical dark-energy from the generalized Chaplygin gas
• Possible Resolution of the Hubble Tension with Weyl Invariant Gravity
• The Hubble tension in the non-flat Super-$\Lambda \mathrm{CDM}$ model
• The H0 trouble: Confronting Non-thermal Dark Matter and Phantom Cosmology with the CMB, BAO, and Type Ia Supernovae data
• Cosmological Distances And Hubble Tension In Einstein-Cartan Theory
• Is cosmological data suggesting a nonminimal coupling between matter and gravity?
• Interacting phantom dark energy: new accelerating scaling attractors
• Mitigating the binary viewing angle bias for standard sirens
• Can the Universe decelerate in the future?
• Do we need wavelets in the late Universe?
• Reconstructing the growth index $\gamma$ with Gaussian Processes
• Cosmological effects of the Galileon term in Scalar-Tensor Theories
• A possible late-time transition of $M_B$ inferred via neural networks
• Imprints of screened dark energy on nonlocal quantum correlations
• Bound on photon circular orbits in general relativity and beyond
• Constraining cosmological parameters from strong lensing with DECIGO and B-DECIGO sources
• Testing the Homogeneity of Type Ia Supernovae in the Near-Infrared for Accurate Distance Estimations
• Neutrino at different epochs of the Friedmann Universe
• Testing screened modified gravity with SDSS-IV-MaNGA
• Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity
• Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
• Constraining deviations from $\Lambda$CDM in the Hubble expansion rate
• The Muon Magnetic Moment and Physics Beyond the Standard Model
• The effective running Hubble constant in SNe Ia as a marker for the dark energy nature
• Forecasts for interacting dark energy with time-dependent momentum exchange
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• ${\Lambda }_{\mathrm{s}}$CDM cosmology from a type-II minimally modified gravity
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Can Early Dark Energy be Probed by the High-Redshift Galaxy Abundance?
• Quadratic energy-momentum squared gravity: constraints from big bang nucleosynthesis
• Constraints on sterile neutrinos and the cosmological tensions
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect
• A representation learning approach to probe for dynamical dark energy in matter power spectra
• Dissipative quintessence, and its cosmological implications
• Cosmological Fisher forecasts for next-generation spectroscopic surveys
• Weak field and slow motion limits in energy-momentum powered gravity
• Neutrino non-radiative decay and the diffuse supernova neutrino background
• Gravitational waves from inspiraling black holes in quadratic gravity
• No evidence for EDE from Planck data in extended scenarios
• Using peculiar velocity surveys to constrain neutrino masses
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• Determination of the Kinematic Parameters from SNe Ia and Cosmic Chronometers
• Imprint of Early Dark Energy in Stochastic Gravitational Wave Background
• The effect of screening mechanisms on black hole binary inspiral waveforms
• Probing ultra-light dark photon from inverse Compton-like scattering
• Probing the dark matter density evolution law with large scale structures
• SIDE-real: Supernova Ia Dust Extinction with truncated marginal neural ratio estimation applied to real data
• Cosmological fluids with boundary term couplings
• Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
• Cosmological singularities in $f(T,\varphi )$ gravity
• Shadows of black holes at cosmological distances in the co-varying physical couplings framework
• Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
• Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
• Non-parametric modeling of the cosmological data, base on the ${\chi }^2$ distribution
• Is there a dynamical tendency in H0 with late time measurements?
• Domain Wall Network: A Dual Solution for Gravitational Waves and Hubble Tension?
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• The Hubble Rate Trouble: An Effective Field Theory of Dark Matter
• II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Chameleon Screening in Cosmic Voids
• A Geometric Calibration of the Tip of the Red Giant Branch in the Milky Way using Gaia DR3
• Machine learning unveils the linear matter power spectrum of modified gravity
• Gravitational particle production and the Hubble tension
• Generalized McVittie geometry in Horndeski gravity with matter
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Effects of a local physics change on the SH0ES determination of $H_0$
• Van der Waals Anomaly
• An empirical consistent redshift bias: A possible direct reproducible observation of Zwicky's TL theory
• Extended Uncertainty Principle: A Deeper Insight into the Hubble Tension?
• Addressing the Hubble tension in Yukawa cosmology?
• Modelling the emergence of cosmic anisotropy from non-linear structures
• Assessing the foundation and applicability of some dark energy fluid models in the Dirac-Born-Infeld framework
• Cosmic voids and the kinetic analysis. III. Hubble tension and structure formation in the late Universe
• Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes
• Quantum analysis of the recent cosmological bounce in the comoving Hubble length
• Dirac dark matter, dark radiation, and the type-II seesaw mechanism in alternative $U(1{)}_X$ standard model
• Modified Equations of State for Dark Energy and Observational Limitations
• A Non-parametric Reconstruction of the Hubble Parameter $H(z)$ Based on Radial Basis Function Neural Networks
• Improving Constraints on Models Addressing the Hubble Tension with CMB Delensing
• Consequences of using a smooth cosmic distance in a lumpy universe: I
• Phantom cosmologies from QCD ghost dark energy
• Measuring the matter fluctuations in the Local Universe with the ALFALFA catalog
• A field-level emulator for modified gravity
• Two Dynamical Scenarios for Binned Master Sample Interpretation
• A generic dynamical system formulation for Bianchi-I cosmology with isotropic fluid in $f(Q)$ gravity
• Modern Cosmology, an Amuse-Gueule
• Coupled Quintessence scalar field model in light of observational datasets
• Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
• Mirror Dark Sector Solution of the Hubble Tension with Time-varying Fine-structure Constant
• Metastability in Emergent Dark Energy: A New Framework Confronting Cosmological Observations
• Casimir cosmology
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Scalar field evolution at background and perturbation levels for a broad class of potentials
• Exploring Alternative Cosmologies with the LSST: Simulated Forecasts and Current Observational Constraints
• Fundamental Physics and Cosmology with TianQin
• Cosmological Constraints using the newest VLT-KMOS HII Galaxies and the full Planck CMB spectrum
• Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
• Inhomogeneous solutions in $f(T,B)$ gravity
• Eliminating the Hubble Tension in the Presence of the Interconnection between Dark Energy and Matter in the Modern Universe
• Testing the cosmic distance duality relation with baryon acoustic oscillations and supernovae data
• Quintessential Implications of the presence of AdS in the Dark Energy sector
• Exploring Modified Gravity: Constraints on the $\mu$ and $\Sigma$ Parametrization with WMAP, ACT, and SPT
• Matter really does matter, or Why $f(R,\mathrm{Matter})$ type theories are significant for gravitational physics and cosmology
• Revisiting CPL with sign-switching density: To cross or not to cross the NECB
• Measuring distances to galaxies with globular cluster velocity dispersions
• Compact star in noninteger power model of $f(R)$ gravity
• Solar System-scale interferometry on fast radio bursts could measure cosmic distances with sub-percent precision
• Phantom crossing or dark interaction?
• Effects of anisotropy in an anisotropic extension of $w$CDM model
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• Synergy Between Hubble Tension Motivated Self-Interacting Neutrino and KeV-Sterile Neutrino Dark Matter
• The Spectre of Underdetermination in Modern Cosmology
• Dynamics of dwarf galaxies in $f(R)$ gravity
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• Is there evidence for CIDER in the Universe?
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Cosmic voids and the kinetic analysis. II. Link to Hubble tension
• Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude
• Constraining cosmological scaling solutions of a Galileon field
• On the Hubble expansion in a Big Bang quantum cosmology
• Unveiling the Universe with Emerging Cosmological Probes
• Axi-Higgs cosmology: Cosmic Microwave Background and cosmological tensions
• Big Bang Nucleosynthesis with $f(R)$ gravity scalarons and astrophysical consequences
• New Anisotropic Exact Solution in Multifield Cosmology
• Thermodynamics of the Weyl Geometric Gravity Black Holes
• Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars
• Chameleon Early Dark Energy and the Hubble Tension
• Inferring Cosmological Parameters with Evidential Physics-Informed Neural Networks
• Examining the validity of the minimal varying speed of light model through cosmological observations: relaxing the null curvature constraint
• Litmus tests of the flat $\Lambda$CDM model and model-independent measurement of $H_0{r}_{\mathrm{d}}$ with LSST and DESI
• Constraining modified gravity scenarios with the 6dFGS and SDSS galaxy peculiar velocity datasets
• Relativistic binary systems in scale-independent energy-momentum squared gravity
• Observational constraints on the growth index parameters in $f(Q)$ gravity
• Late-time dynamics of dark energy EoS in symmetric teleparallel gravity
• Spatially Homogeneous Universes with Late-Time Anisotropy
• Testing $f(T)$ Gravity with Cosmological Observations: Confronting the Hubble Tension and Implications for the Late-Time Universe
• Dynamics of dark energy in a scalar-vector-torsion theory
• Non-parametric reconstructions of cosmic curvature: current constraints and forecasts
• Constraints on Late Time Violations of the Equivalence Principle in the Dark Sector
• Constraining the Hubble constant with scattering in host galaxies of fast radio bursts
• A possible role for the merger of clusters/voids in the cosmological expansion
• Can the sound horizon-free measurement of $H_0$ constrain early new physics?
• HOLISMOKES -- XII. Time-delay Measurements of Strongly Lensed Type Ia Supernovae using a Long Short-Term Memory Network
• Thermal leptogenesis in anisotropic cosmology
• A comprehensive data-driven odyssey to explore the equation of state of dark energy
• Higgs Inflation: constraining the top quark mass and breaking the $H_0$-${\sigma }_8$ correlation
• Effects of particle creation rate in two-fluid interacting cosmologies
• Constraining Fundamental Constants with Fast Radio Bursts: Unveiling the Role of Energy Scale
• Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity
• A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
• Accurate method for ultralight axion CMB and matter power spectra
• Addressing the $r_d$ Tension using Late-Time Observational Measurements in a Novel deceleration Parametrization
• Can Baby Universe Absorption Explain Dark Energy?
• Gravitational wave polarizations in nonminimally coupled gravity
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Impact of Low ell's on Large Scale Structure Anomalies
• Non-parametric reconstruction of the fine structure constant with galaxy clusters
• Climbing out of the shadows: building the distance ladder with black hole images
• Do current observations support transient acceleration of our universe?
• Constraining Cosmology With the CMB $\times$ LIM-Nulling Convergence
• Extended minimal theories of massive gravity
• Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
• Investigating the cosmic distance duality relation with gamma-ray bursts
• Lens Modeling of STRIDES Strongly Lensed Quasars using Neural Posterior Estimation
• Linking the $R_{K^{(\ast )}}$ anomalies to the Hubble tension via a single right-handed neutrino
• New exact and analytic solutions in Weyl Integrable cosmology from Noether symmetry analysis
• Exploring parametrized dark energy models in interacting scenario
• Qualitative analysis for viscous cosmologies in a non linear regime of the Israel-Stewart formalism
• Measuring the speed of light with cosmological observations: current constraints and forecasts
• Resilience and implications of adiabatic CMB cooling
• Loop effect with vector mediator in the coherent neutrino-nucleus scattering
• Gravitational waveforms from the inspiral of compact binaries in the Brans-Dicke theory in an expanding Universe
• Using ${}^{44}$Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors
• Cosmic voids and the kinetic analysis. IV. Hubble tension and the cosmological constant
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Foreground biases in strong gravitational lensing
• A new parametrization of Hubble function and Hubble tension
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• A proposal to improve the accuracy of cosmological observables and address the Hubble tension problem
• Limit on the dark matter mass from its interaction with photons
• Dynamical system analysis in modified Galileon cosmology
• Generalized second law of thermodynamics for the matter creation scenario and emergence of phantom regime
• New simple and accurate quintessence approximations
• A New Parameterized Interacting Holographic Dark Energy
• Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions
• Reconstructing the parameter space of non-analytical cosmological fixed points
• Coupled quintessence inspired by warm inflation
• Fluctuating Dark Energy and the Luminosity Distance
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• Constraining Cosmology with Double-source-plane Strong Gravitational Lenses from the AGEL Survey
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Inflation in non-local hybrid metric-Palatini gravity
• The Hubble constant from galaxy cluster scaling-relation and SNe Ia observations: a consistency test
• Tilted non-spatially-flat inflation
• What Prevents Resolving the Hubble Tension through Late-Time Expansion Modifications?
• The Hubble tension from the standpoint of quantum cosmology
• Dynamical analysis and cosmological evolution in Weyl integrable gravity
• Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation
• Type V singularities with inhomogeneous equations of state
• Survival of black holes through a cosmological bounce
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity
• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
• Fab-Four cosmography to tackle the Hubble tension
• The art of building a smooth cosmic distance ladder in a perturbed universe
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Redshift evolution of the X-ray and UV luminosity relation of quasars: calibrated results from SNe Ia
• GausSN: Bayesian Time-Delay Estimation for Strongly Lensed Supernovae
• Another look on the connections of Hubble tension with the Heisenberg Uncertainty Principle
• Non-linear density-velocity dynamics in $f(R)$ gravity from spherical collapse
• Inverse Seesaw, dark matter and the Hubble tension
• Dynamics of holographic dark energy with apparent-horizon cutoff and non-minimal derivative coupling gravity in non-flat FLRW universe
• Revisiting coupled CDM-massive neutrino perturbations in diverse cosmological backgrounds
• Constraining the quintessential $\alpha$-attractor inflation through dynamical horizon exit method
• Sensitivity of the Global 21-cm Signal to Dark Matter-Baryon Scattering
• Gravitational wave oscillations in bimetric cosmology
• Special Issue on Modified Gravity Approaches to the Tensions of $\Lambda$CDM: Goals and Highlights
• A Hubble Constant Determination Through Quasar Time Delays and Type Ia Supernovae
• Bayesian inference of $W$-boson mass
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Cosmic curvature on large-scale structures with homogeneous dark energy
• Emergent universe revisited through the CSL theory
• Cosmic tangle: Loop quantum cosmology and CMB anomalies
• A test of invariance of dark matter halo surface density using multiwavelength mock galaxy catalogues
• Field transformations and invariant quantities in scalar-teleparallel theories of gravity
• Axion-philic cosmological moduli
• Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff
• STag: Supernova Tagging and Classification
• BBN to Late-Time Acceleration in $f(T,{\mathcal{L}}_m)$ Gravity
• Mass assembly history of dark matter halos in the light of $H_0$ tension
• Glimmers of a post-geometric perspective
• Gravitational waves in a cyclic Universe: resilience through cycles and vacuum state
• Sound Horizon Independent Constraints on Early Dark Energy: The Role of Supernova Data
• Testing General Relativity through the $E_G$ Statistic Using the Weyl Potential and Galaxy Velocities
• Dynamical systems analysis of a cosmological model with interacting Umami Chaplygin fluid in adiabatic particle creation mechanism: Some bouncing features
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Host group degeneracy in gravitational lensing time delay determination of $H_0$
• Theory of interacting vector dark energy and fluid
• Anisotropic power-law inflation for a generalized model of two scalar and two vector fields
• Thermodynamics of a transient phantom scenario
• Local Limit of Nonlocal Gravity: Cosmological Perturbations
• Constrain the linear scalar perturbation theory of Cotton gravity
• A possible solution to the Hubble tension from quantum gravity
• Peculiar velocity effects on the Hubble constant from time-delay cosmography
• Stochastic dark matter: Covariant Brownian motion from Planckian discreteness
• Induced Cosmological Anisotropies and CMB Anomalies by a non-Abelian Gauge-Gravity Interaction
• WIMP dark matter in bulk viscous non-standard cosmologies
• Local Limit of Nonlocal Gravity: A Teleparallel Extension of General Relativity
• Propagating Uncertainties in the SALT3 Model Training Process to Cosmological Constraints
• A flexible parameterization to test early physics solutions to the Hubble tension with future CMB data
• Challenges to a sharp change in $G$ as a solution to the Hubble tension
• Probing General Relativity in galactic scales at z $\sim 0.3$
• Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results
• Bayesian jackknife tests with a small number of subsets: Application to HERA 21cm power spectrum upper limits
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• Role of internal space correlations in the dynamics of a higher-dimensional Bianchi type-I universe: shear scalar and Hubble parameter perspectives
• Cosmological model with Gong-Zong Parametrization in $f(R,L_m)$ gravity
• Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood
• Prospects for measuring neutrino mass with 21-cm forest
• Scale and redshift dependent limits on cosmic neutrino properties
• Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
• Can radial motions in the stellar halo constrain the rate of change of mass in the Galaxy?
• Effective field theory of coupled dark energy and dark matter
• Viability of general relativity and modified gravity cosmologies using high-redshift cosmic probes
• Gravitation with modified fluid Lagrangian: Variational principle and an early dark energy model
• When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior
• Wave correlations and quantum noise in cosmology
• Cosmic Strings as Dynamical Dark Energy: Novel Constraints
• Hearing Higgs with Gravitational Wave Detectors
• Non-Parametric Analysis for the Dark Matter Density Evolution
• Variational symmetries and superintegrability in multifield cosmology
• High-redshift Galaxies from JWST Observations in More Realistic Dark Matter Halo Models
• Modified cosmology through generalized mass-to-horizon entropy: observational constraints from DESI DR2 BAO data
• Solving the Hubble tension à la Ellis & Stoeger 1987
• Lowering the Horizon on Dark Energy: A Late-Time Response to Early Solutions for the Hubble Tension
• Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
• Performance of Non-Parametric Reconstruction Techniques in the Late-Time Universe
• Can Hubble tension be eased by invoking a finite range for gravity?
• $H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
• A test for the redshift dependence of ${\sigma }_8$ using $f{\sigma }_8$ measurements
• Early dark energy in the pre- and post-recombination epochs
• On the Metric $f(R)$ gravity Viability in Accounting for the Binned Supernovae Data
• Clusternets: A deep learning approach to probe clustering dark energy
• Early dark energy and scalarization in a scalar-tensor model
• A Semiblind Reconstruction of the History of Effective Number of Neutrinos Using CMB Data
• Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes
• Revisiting the Hubble constant, sound horizon and cosmography from late-time Universe observations
• Cosmic expansion beyond $\Lambda$CDM: Investigating power-law and logarithmic corrections
• Constraints on Tsallis cosmology using recent low and high redshift measurements
• Testing beyond-Kerr spacetimes with GWTC-3
• Reconciling Cosmological Tensions with Inelastic Dark Matter and Dark Radiation in a $\mathbf{U}(1{)}_{\mathbf{D}}$ Framework
• Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective
• Hubble Tension in Power-Law f(R) Gravity and Generalized Brans-Dicke Theory
• HOLISMOKES -- XIV. Time-delay and differential dust extinction determination with lensed type II supernova color curves
• Kinetic recoupling of dark matter
• Contemplating the fate of modified gravity
• The model of the local Universe in the framework of the second-order perturbation theory
• Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis
• A simple direct empirical observation of systematic bias of the redshift as a distance indicator
• Mimetic Weyl geometric gravity
• Revisiting Cosmic Distance Duality with Megamasers and DESI DR2 Observations: Model Independent Constraints on Early-Late Calibration
• Cosmological singularities in non-canonical models of dark energy
• Remarks on overestimating the effects of inhomogeneities on the Hubble constant
• Can the angular scale of cosmic homogeneity be used as a cosmological test?
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• FBQ 0951+2635: time delay and structure of the main lensing galaxy
• Dark Energy Constraints from Pantheon+ Ia Supernovae Data
• Testing the coupling of dark radiations in light of the Hubble tension
• Pantheon+ tomography and Hubble tension
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• New Constraints on Anisotropic Expansion from Supernovae Type Ia
• Cosmology with Higher-Derivative Gravities
• Principal Components for Model-Agnostic Modified Gravity with 3x2pt
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Probing dark fluids and modified gravity with gravitational lensing
• Unraveling the Hubble tension with warm inflation
• New inflationary exact solution from Lie symmetries
• Consistent cosmological structure formation on all scales in relativistic extensions of MOND
• The subtle statistics of the distance ladder: On the distance prior and selection effects
• Testing neutrino mass hierarchy under type-II seesaw scenario in $U(1{)}_X$ from colliders
• Kernel-, mean- and noise-marginalised Gaussian processes for exoplanet transits and $H_0$ inference
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$
• FIMP Dark Matter in bulk viscous non-standard cosmologies
• Time delay estimation in unresolved lensed quasars
• Thermo-Coupled Early Dark Energy
• Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
• Evidence for possible systematic underestimation of uncertainties in extragalactic distances and its cosmological implications
• Realizing late-time cosmology in the context of Dynamical Stability Approach
• Spatially homogeneous teleparallel spacetimes with four-dimensional groups of motions
• From negative to positive cosmological constant through decreasing temperature of the Universe: connection with string theory and spacetime foliation results
• Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: ${\Lambda }_{\mathrm{s}}$CDM versus $\Lambda$CDM
• Testing Lens Models of PLCK G165.7+67.0 Using Lensed SN H0pe
• Particle Production Scenario in an Algebraically Coupled Quintessence Field with a Dark Matter Fluid
• Biases in velocity reconstruction: investigating the effects on growth rate and expansion measurements in the local universe
• Unimodular Theory of Gravity in Light of the Latest Cosmological Data
• Crosschecking Cosmic Distances from DESI BAO and DES SNe
• A Review on Resolving the Hubble Tension via Late-Universe Physics
• New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
• Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data
• Investigating the Redshift Evolution of Lensing Galaxy Density Slopes via Model-Independent Distance Ratios
• Reheating constraints and the $H_0$ tension in Quintessential Inflation
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Second-order dust perturbations of the non-flat FLRW model with the positive cosmological constant
• Mapping luminous and dark matter in the Universe
• Constraining disformal couplings with Redshift Space Distortion
• Model Independent Dark Matter Properties from Cosmic Growth
• Matter Creation Cosmologies and Accelerated Expansion
• Towards a Composite Framework for Simultaneous Exploration of New Physics in Background and Perturbed Universe
• From oversimplified to overlooked: the case for exploring Rich Dark Sectors
• Fast Generation of Weak Lensing Maps in Modified Gravity with COLA
• Periodic boundary conditions and $G_2$ cosmology
• Line-of-sight effects on double source plane lenses
• Fractal properties of particle paths due to generalised uncertainty relations
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• BBN-simple: How to Bake a Universe-Sized Cake
• Cosmological viability of a double field unified model from warm inflation
• New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
• A test of galaxy cluster fundamental plane for the X-COP sample
• Characterising the Standardisation Properties of Type Ia Supernovae in the z band with Hierarchical Bayesian Modelling
• Quantum Mechanics from General Relativity and the Quantum Friedmann Equation
• Assessing the Robustness of the CPL Parametrization to Basis and Prior Variations: Insights from DESI DR2 BAO Data
• Dark matter fluid constraints from galaxy rotation curves
• Tritium beta decay with modified neutrino dispersion relations: KATRIN in the dark sea
• Zwicky Transient Facility and Globular Clusters: the gr-Band Period-Luminosity Relations for Mira Variables at Maximum Light and Their Applications to Local Galaxies
• On the Earth's tidal perturbations. II. LARES 2 satellite
• New parameter region in sterile neutrino searches: a scenario to alleviate cosmological neutrino mass bound and its testability at oscillation experiments
• Asymmetry in galaxy spin directions: a fully reproducible experiment using HSC data
• Observational tests of the conformal osculating Barthel-Kropina cosmological model
• Degrees of Freedom of New General Relativity I: Type 2, Type 3, Type 5, and Type 8
• The Lambda-CDM-NG cosmological model: A possible resolution of the Hubble tension
• A new consistency test for $\Lambda$CDM cosmology using galaxy surveys
• Gravitational Waves and Electromagnetic Transients
• Multifield theories invariant under transverse diffeomorphisms: The mixed regime case
• Signature of $f\left(R\right)$ gravity via Lemaître-Tolman-Bondi inhomogeneous perturbations
• Alleviating the Hubble tension with Torsion Condensation (TorC)
• Modified cosmology through generalized mass-to-horizon entropy: implications for structure growth and primordial gravitational waves
• A mechanism to generate varying speed of light via Higgs-dilaton coupling: Theory and cosmological applications
• Cosmologies in $f(R,{\mathcal{L}}_m)$ theory with non-minimal coupling between geometry and matter
• Constraining decaying dark matter models with gravitational lensing and cosmic voids
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Evolution of perturbations in a universe with exotic solid-like matter
• Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
• Gaussian discriminators between $\Lambda$CDM and wCDM cosmologies using expansion data
• Scalar-induced gravitational waves in spatially covariant gravity
• Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
• Dynamical Dark Energy Signatures from a New Transition $Om(z)$ Parametrization in Flat FLRW Cosmology
• Generation of effective massive Spin-2 fields through spontaneous symmetry breaking of scalar field
• One-point Statistics in various cosmic environments in the presence of massive neutrinos
• Linear seesaw leptogenesis before/after electroweak symmetry breaking
• ZTF SN Ia DR2: Impact of the galaxy cluster environment on the stretch distribution of Type Ia supernovae
• The Case for Space: Estimating Precise Time Delays from Ground- and Space-Based Observations of Lensed Supernovae with Glimpse
• Comparison of $\Lambda$CDM and $R_h=ct$ with updated galaxy cluster $f_{gas}$ measurements using Bayesian inference
• ${\mathbf{\Omega }}_1{\mathbf{\Omega }}_2$-$\mathbf{\Lambda }$CDM: A promising phenomenological extension of the standard model of cosmology
• Confronting global 21-cm signal with ${\mathbb{Z}}_3$ symmetric dark matter models
• Role of Spatial Curvature in a Dark Energy Interacting Model
• Cosmology in $R^2$-gravity: Effects of a Higher Derivative Scalar Condensate Background
• A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Future of Bianchi I magnetic cosmologies with kinetic matter
• A robust assessment of the local anisotropy of the Hubble constant
• Post-Newtonian limit of generalized scalar-teleparallel theories of gravity
• On rips and cosmological singularities in a universe merging with baby universes
• Refitting cosmological data with neutrino mass and degeneracy
• Effects of dynamical friction on perturbations for evolving dark energy
• Interacting tachyon with varying mass dark matter
• Hubble Tension and Gravitational Self-Interaction
• Quarks to Cosmos: Particles and Plasma in Cosmological evolution
• The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles
• Dark sector interactions in light of weak lensing data
• Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope
• The cosmological Mass Varying Neutrino model in the late universe
• A semi-cosmographic approach to study cosmological evolution in phase space
• Thermodynamics of sign-switching dark energy models
• Gravitational Wave Production and Baryogenesis in a Simple Left-Right model
• Understanding Galaxy Rotation Curves with Verlinde's Emergent Gravity
• A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension
• The Luminosity of the Darkness: Schechter function in dark sirens
• Qualitative analysis of a quasi-magnetic universe
• Deflection of light and time delay in hyperbolic Einstein-Straus--de Sitter solution
• Cosmological observational tests in the JWST Era. I: angular size - redshift
• Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx
• Cosmological Frequency Combs
• Stealth black hole solutions in higher-order Maxwell-Einstein theories
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• On energy-momentum conservation in non-minimal geometry-matter coupling theories
• Assessment of Dark Matter Models Using Dark Matter Correlations across Dwarf Spheroidal Galaxies
• Cosmology in warped massive gravity
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Brans-Dicke-like field for co-varying $G$ and $c$: observational constraints
• Observing Double White Dwarfs with the Lunar GW Antenna
• Towards Precision Cosmology With Improved PNLF Distances Using VLT-MUSE. III. Impact of Stellar Populations in Early-Type Galaxy
• Implications of $f(R)$ gravity on late-time cosmic structure growth through a complete description of density perturbations
• A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter
• Stability of spherical thin-shell wormholes in scalar-tensor theories
• Game Theory in Cosmology
• Focus Point on Tensions in Cosmology from Early to Late Universe: Part II: New Directions in the Light of Observations from the Most Modern Astronomical Facilities
• Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Probing Interacting Dark Sectors with upcoming Post-Reionization and Galaxy Surveys
• Nuclear fission reaction simulations in compact stars
• Conformal Killing Gravity: New Constraints from DESI DR2 BAO datasets
• Cosmological constraints on the big bang quantum cosmology model
• Polytropic $f(Q)$ cosmology and its implications for the $H_0$ tension
• Jacobi stability of circular orbits around conformally invariant Weyl gravity black holes
• Towards a Machine Learning Solution for Hubble Tension: Physics-Informed Neural Network (PINN) Analysis of Tsallis Holographic Dark Energy in Presence of Neutrinos
• Probing dynamical embeddings in a five-dimensional spacetime in light of DESI BAO
• Constraining nonminimal f(T) gravity from Primordial Nucleosynthesis to Late-Universe observations
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• Study on Gravitational Waves from Binary Mergers and Constraints on the Hubble Parameter
• Quantum noise in time-dependent media and cosmic expansion
• On the Effects of Non-metricity in an Averaged Universe
• Ricci cosmology in light of astronomical data
• Early dark energy triggered by spacetime dynamics that encodes cosmic radiation-matter transition
• Particle physics and cosmology intertwined
• Smearing of primordial gravitational waves
• Decaying Dark Matter: Simulations and Weak-Lensing Forecast
• Dynamics of Dwarf Galaxies in Scalar-Tensor-Vector-Gravity
• HOLISMOKES -- XVIII. Cosmology with strongly lensed type II supernovae: Effects of instrumental setups on $H_0$
• Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
• Semiresolved Stellar Populations as Distance Indicators
• Effective chemical potential and its phenomenological implications for the Hubble parameter
• Preliminary cosmological results using extreme accretors Quasar formalism
• Luminosity-Temperature Relation as a Probe for Modified Gravity
• Cosmological "constant" in a universe born in the metastable false vacuum state
• Constraining Spatial Curvature with Priors from Swampland Conjectures
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Explaining lepton-flavor non-universality and self-interacting dark matter with $L_{\mu }-L_{\tau }$
• Revisiting the quasi-molecular mechanism of recombination
• Accelerating scaling solutions from dark matter particle creation
• The BAO scale -- how standard is the standard ruler?
• $G_3$ -- interacting scalar tensor dark energy
• Theoretical and observational constraints on early dark energy in $F(R)$ gravity
• Dynamical Henneaux-Teitelboim Gravity
• Revisiting observational constraints on coupled exponential quintessence with energy and momentum transfers: degeneracy with massive neutrinos
• Quantum measurement systems and applications to particle physics and cosmology
• Crunching, Bouncing, and Cyclical Cosmologies from Dark Sector Interactions
• On the True Significance of the Hubble Tension: A Bayesian Error Decomposition Accounting for Information Loss
• Statistical consistency of sign-switching vacuum energy with cosmological observations
• Encyclopedia of Astrophysics: The Expanding Universe
• Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families
• Probing dark energy using anisotropies in the clustering of post-EoR HI distribution
• Cluster gravitational redshifts: uncertainties and survey requirements
• $O(d,d)$ symmetry in teleparallel dark energy
• Background dynamics and observational constraints of flat and non-flat $\Lambda (t)$CDM models from $H(z)$ and DESI DR2 BAO measurements
• Finite time pseudo-rip singularity in cosmology
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Future Dark Energy Constraints from Atomic Clocks
• Controlled Tension Forecasting: Quantifying Cross-Probe Biases in ${\omega }_0{\omega }_a$CDM
• $f(T,B)$ cosmography for high redshifts
• Golden and Silver Dark Sirens for precise H0 measurement with HETDEX
• Cosmological and lunar laser ranging constraints on evolving dark energy in a nonminimally coupled curvature-matter gravity model
• The Galactic Pizza: Flat Rotation Curves in the Context of Cosmological Time-Energy Coupling
• Insights for Early Dark Energy with Big Bang Nucleosynthesis
• Spectral distortions in the decaying QCD dark matter scenario
• Extended datasamples under the lens of Brane World Theory
• A model-independent test of speed of light variability with cosmological observations
• A New Approach to Flatness, Horizon and Late-time Accelerating Expansion Problems on the basis of Mach Principle
• Bayesian and Machine-Learning Analyses of Nonminimal $f(Q)$ Gravity and $H_0$ Tension
• Primordial Perturbations Including Second-Order Derivatives of the Inflationary Potential
• Dynamical friction shear and rotation in Chaplygin cosmology
• Fluctuations in the Ginzburg-Landau Theory of Dark Energy: internal (in-)consistencies in PLANCK data set
• Fully Relativistic Derivation of the Thermal Sunyaev-Zel'dovich Effect
• Running Hubble Constant with the Redshift as a Marker of Evolutionary Dark Energy
• Freeze-in Dark Matter via Lepton Portal: Hubble Tension and Stellar Cooling
• Geodesics in Quantum Gravity
• Superhorizon isocurvature fluctuations relax tensions
• Cosmological Implications of Thermodynamic Split Conjecture
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra
• Comments on the mass sheet degeneracy in cosmography analyses
• Confirming the uniformity of the Hubble flow with Pantheon+ Supernovae
• Testing the cosmic distance duality relation using model-independent approach
• The variational slope of quasar light curves is not a distance indicator
• Thermodynamic Split Conjecture and an Observational Test for Cosmological Entropy
• Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS
• Gravitational waves in Palatini gravity for a non-minimal geometry-matter coupling
• Cosmology with a Non-minimally Coupled Dark Matter Fluid I. Background Evolution
• How Holographic is the Dark Energy? A Spline Nodal reconstruction approach
• Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI
• A Breathing Universe is Consistent
• Breaking the Mass-sheet Degeneracy in Time-delay Cosmology with Lensed and Unlensed Type Ia Supernovae
• The Effects of the Gravitational Coupling Variation on the Local $H_0$ Estimation
• A Robust Bayesian Meta-Analysis for Estimating the Hubble Constant via Time Delay Cosmography
• Quasinormal modes of regular black holes surrounded by skewed dark matter distributions
• Time Delay Cosmography: Analysis of Quadruply Lensed QSO SDSSJ1433 from Wendelstein Observatory
• Sign Switching Dark Energy from a Running Barrow Entropy
• Revisiting dynamics of interacting quintessence
• Evolution of superhorizon perturbations in early Universe with anisotropic solid remnant
• Non-Hermitian Gravitational Wave Scattering
• Non-local Interactions are Essential Elements for Dark Matter Halo Stability: A Cross-Model Study
• Kinetic gases in static spherically symmetric modified dispersion relations
• Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking
• Constraints on energy scales from dark matter decay in a gauged $B-L$ model
• FLRW Kinematic-Induced Measurement of the Hubble Constant from Cosmic Chronometer and Redshift Drift Observations
• Quijote PNG: The information content of the halo power spectrum and bispectrum
• The Astrophysical Distance Scale: V. A 2% Distance to the Local Group Spiral M33 via the JAGB Method, Tip of the Red Giant Branch, and Leavitt Law
• Current constraints on the minimally extended varying speed of light model through the cosmic distance duality relation
• Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum
• Constraining Scalar Charge in Neutron Stars through Gravitational Wave Signals from NSBH Mergers
• The $f(Q)$ gravity and affine EoS: Compatibility and observational constraints
• Interacting dark energy from redshift-space galaxy clustering
• Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology
• Sample Variance for Supernovae Distance Measurements and the Hubble tension
• Using Neutrino Oscillations to Measure $H_0$?
• Generalized Eddington--Finkelstein Coordinates and Exact Vaidya-Type Solutions in Weyl Conformal Gravity
• The Effect of Foreground Galaxies on the Estimation of the Hubble Constant from Type Ia Supernovae
• Testing the growth of cosmic structures during the Dark Ages
• Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology
• Void spin distribution as a powerful probe of ${\sigma }_8$
• AutoKnots: Adaptive Knot Allocation for Spline Interpolation
• Gravitational-wave standard sirens and application in cosmology
• Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse
• Precision near-IR spectroscopy for understanding AGN physics and shed light on the H0 tension -- SHARP Science Book
• Testing a nonlinear solution of the Israel-Stewart theory
• Running Einstein Constant and a Possible Vacuum State of the Universe
• Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
• Three-Dimensional Simulations of Type Ia Supernova Remnants I: Effects of a Main-Sequence Companion Star
• Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae
• Systematic Light Propagation Bias from the Heliosphere and Its Impact on the Hubble Tension
• Role of viscous fluid in FLRW model with observational constraints
• Kinematic Probes of Type-II MMG: Padé Cosmographic Analysis of VCDM
• No preference for generalized emergent dark energy from current cosmological data
• Hubble tension problem encompassed by phase-space quantum cosmology
• A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background
• Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime
• A long life of excess: The interacting transient SN 2017hcc
• Constraints on the Modified Emergent Dark Energy Model Using DESI DR2 BAO
• A comparative study of emergent dark energy models