Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?

Abstract

We wish to investigate whether there is an extension to the base $\Lambda$CDM cosmology that can resolve the tension between the Planck observation of the cosmic microwave background anisotropies and the local measurement of the Hubble constant. We consider various plausible extended models in this work, and we use the Planck 2015 observation, combined with the baryon acoustic oscillation data, the JLA type Ia supernovae data, and the local measurement of the Hubble constant (by Riess et al. in 2016), to make an analysis. We find that the holographic dark energy plus sterile neutrino model can reduce the tension to be at the 1.11$\sigma$ level, but this model is obviously not favored by the current observations. Among these extended models, the $\Lambda$CDM+$N_{\mathrm{eff}}$ model is most favored by the current observations, and this model can reduce the tension to be at the 1.87$\sigma$ level. By a careful test, we conclude that none of these extended models can convincingly resolve the $H_0$ tension.

10 pages, 1 figure

References in corpus (79)

• Planck 2015 results. XIII. Cosmological parameters
• Planck 2013 results. XVI. Cosmological parameters
• Efficient Computation of CMB anisotropies in closed FRW models
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Exploring the Expansion History of the Universe
• Accelerating Universes with Scaling Dark Matter
• A 2.4% Determination of the Local Value of the Hubble Constant
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• A Model of Holographic Dark Energy
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3
• The trouble with $H_0$
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
• Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant
• Can interacting dark energy solve the $H_0$ tension?
• Planck intermediate results. XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth
• Large-scale instability in interacting dark energy and dark matter fluids
• Two accurate time-delay distances from strong lensing: Implications for cosmology
• Reconciling Planck with the local value of $H_0$ in extended parameter space
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• H0 Revisited
• Evidence for massive neutrinos from CMB and lensing observations
• Quantifying discordance in the 2015 Planck CMB spectrum
• The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
• A fresh look at linear cosmological constraints on a decaying dark matter component
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• Hot Axions and the $H_0$ tension
• Interacting Dark Sector and Precision Cosmology
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Tension between the power spectrum of density perturbations measured on large and small scales
• Structure formation in $f(T)$ gravity and a solution for $H_0$ tension
• Testing the Interaction between Dark Energy and Dark Matter with Planck Data
• A Vacuum Phase Transition Solves $H_0$ Tension
• New constraints on Coupled Dark Energy from Planck
• Evidence for dark matter interactions in cosmological precision data?
• Planck Data Reconsidered
• Anthropic Principle Favors the Holographic Dark Energy
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Converting non-relativistic dark matter to radiation
• Planck Constraints on Holographic Dark Energy
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• Determining $H_0$ with Bayesian hyper-parameters
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant
• Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation
• 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
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Testing models of vacuum energy interacting with cold dark matter
• Cosmological Constraints on Interacting Light Particles
• Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2
• Residual Non-Abelian Dark Matter and Dark Radiation
• Impacts of dark energy on weighing neutrinos: mass hierarchies considered
• Constraints on the neutrino mass and mass hierarchy from cosmological observations
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• A search for sterile neutrinos with the latest cosmological observations
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Hidden Charged Dark Matter and Chiral Dark Radiation
• Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• The Mid-Infrared Tully-Fisher Relation: Calibration of the SNIa Scale and Ho
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Do joint CMB and HST data support a scale invariant spectrum?
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Evidence for galaxy dynamics tracing background cosmology below the de Sitter scale of acceleration
• Constraints on inflation revisited: An analysis including the latest local measurement of the Hubble constant
• A comment on power-law inflation with a dark radiation component
• Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
• Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion
• An Accelerating Universe without Lambda: Delta~Gravity Using Monte Carlo

Cited by in corpus (129)

• In the Realm of the Hubble tension $-$ a Review of Solutions
• Challenges for $\Lambda$CDM: An update
• Cosmology Intertwined II: The Hubble Constant Tension
• New physics in light of the $H_0$ tension: an alternative view
• Non-minimal dark sector physics and cosmological tensions
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Local determination of the Hubble constant and the deceleration parameter
• New Early Dark Energy
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• Revisiting a negative cosmological constant from low-redshift data
• Late universe decaying dark matter can relieve the H_0 tension
• Primordial gravitational waves from NANOGrav: a broken power-law approach
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• Restoring cosmological concordance with early dark energy and massive neutrinos?
• The Gravitational-Wave Physics II: Progress
• Interpreting cosmological tensions from the effective field theory of torsional gravity
• Relieving the $H_0$ tension with a new interacting dark energy model
• Evidence for Emergent Dark Energy
• Reconciling $H_0$ tension in a six parameter space?
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Gravitational wave standard sirens and cosmological parameter measurement
• No-go guide for the Hubble tension : Late-time solutions
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Cosmological constraints on late-universe decaying dark matter as a solution to the $H_0$ tension
• Updating constraints on f(T) teleparallel cosmology and the consistency with Big Bang Nucleosynthesis
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Measurements of the Hubble constant and cosmic curvature with quasars: ultra-compact radio structure and strong gravitational lensing
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• Emergent Dark Energy, neutrinos and cosmological tensions
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Neural Network Reconstruction of Late-Time Cosmology and Null Tests
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• 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
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Revealing the late-time transition of $H_0$: relieve the Hubble crisis
• Hints of dark energy anisotropic stress using Machine Learning
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Cosmology with fast radio bursts in the era of SKA
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Dynamical analysis of cosmological models with non-Abelian gauge vector fields
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Possible Hints of Sterile Neutrinos in Recent Measurements of the Hubble Parameter
• Evaporating primordial black holes as varying dark energy
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Anisotropic Einstein Yang-Mills Higgs Dark Energy
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• Galaxy-Scale Test of General Relativity with Strong Gravitational Lensing
• A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short $\gamma$-ray bursts
• Forecast for weighing neutrinos in cosmology with SKA
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Hubble constant and sound horizon from the late-time Universe
• A search for sterile neutrinos in interacting dark energy models using DESI baryon acoustic oscillations and DES supernovae data
• Anisotropic solid dark energy
• Constraining Sterile Neutrino Cosmology with Terrestrial Oscillation Experiments
• Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
• Anisotropic $k$-essence
• Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Strongly lensed type Ia supernovae as a precise late-universe probe of measuring the Hubble constant and cosmic curvature
• Measuring cosmic curvature with non-CMB observations
• Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
• BBN Constraints on $f(Q,T)$ Gravity
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• Arbitrarily coupled $p-$forms in cosmological backgrounds
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• Testing the Cosmic Distance Duality Relation Using Strong Gravitational Lensing Time Delays and Type Ia Supernovae
• The Spin Tensor of Dark Matter and the Hubble Parameter Tension
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• Using machine learning to compress the matter transfer function $T(k)$
• Hubble distancing: Focusing on distance measurements in cosmology
• Kinetically Coupled Scalar Fields Model and Cosmological Tensions
• Cosmological Parameter Estimation Using Current and Future Observations of Strong Gravitational Lensing
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• New evidence and analysis of cosmological-scale asymmetry in galaxy spin directions
• Structure Formation in Various Dynamical Dark Energy Scenarios
• Band-limited Features in the Primordial Power Spectrum Do Not Resolve the Hubble Tension
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• Measuring neutrino masses with joint JWST and DESI DR2 data
• Evidence of dark energy in different cosmological observations
• Observational constraints in Delta Gravity: CMB and supernovas
• Distant foreground and the Planck-derived Hubble constant
• Coupled Dark Sector Models and Cosmological Tensions
• Imprints of screened dark energy on nonlocal quantum correlations
• $\Lambda$CDM as a Noether Symmetry in Cosmology
• Is there a dynamical tendency in H0 with late time measurements?
• Domain Wall Network: A Dual Solution for Gravitational Waves and Hubble Tension?
• Cosmological Constraints on Thermal Friction of Axion Dark Matter
• Testing the cosmic distance duality relation with baryon acoustic oscillations and supernovae data
• Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
• Metastability in Emergent Dark Energy: A New Framework Confronting Cosmological Observations
• Constraining neutrino mass in dynamical dark energy cosmologies with the logarithm parametrization and the oscillating parametrization
• Hubble tension and matter inhomogeneities: a theoretical perspective
• Reconstructing the parameter space of non-analytical cosmological fixed points
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Resilience and implications of adiabatic CMB cooling
• 2D BAO vs 3D BAO: Hints for new physics?
• Performance of Non-Parametric Reconstruction Techniques in the Late-Time Universe
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
• Dark sector interactions in light of weak lensing data
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
• (Pre)-Inflationary Dynamics with Starobinsky Potential in Noncommutative Effective LQC
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra
• Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data