Reconciling Planck with the local value of $H_0$ in extended parameter space

Abstract

The recent determination of the local value of the Hubble constant by Riess et al, 2016 (hereafter R16) is now 3.3 sigma higher than the value derived from the most recent CMB anisotropy data provided by the Planck satellite in a LCDM model. Here we perform a combined analysis of the Planck and R16 results in an extended parameter space, varying simultaneously 12 cosmological parameters instead of the usual 6. We find that a phantom-like dark energy component, with effective equation of state $w=-1.29_{-0.12}^{+0.15}$ at 68 % c.l. can solve the current tension between the Planck dataset and the R16 prior in an extended $\Lambda$CDM scenario. On the other hand, the neutrino effective number is fully compatible with standard expectations. This result is confirmed when including cosmic shear data from the CFHTLenS survey and CMB lensing constraints from Planck. However, when BAO measurements are included we find that some of the tension with R16 remains, as also is the case when we include the supernova type Ia luminosity distances from the JLA catalog.

6 pages, 1 figure

References in corpus (5)

• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
• Cosmic Microwave Weak lensing data as a test for the dark universe
• Standard rulers, candles, and clocks from the low-redshift Universe
• On the local variation of the Hubble constant

Cited by in corpus (279)

• In the Realm of the Hubble tension $-$ a Review of Solutions
• Early Dark Energy Can Resolve The Hubble Tension
• Challenges for $\Lambda$CDM: An update
• The trouble with $H_0$
• The Hubble Hunter's Guide
• Cosmology Intertwined II: The Hubble Constant Tension
• New physics in light of the $H_0$ tension: an alternative view
• Dynamical dark energy in light of the latest observations
• H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: $H_0$ to 3.8% precision from strong lensing in a flat $\Lambda$CDM model
• Cosmology Intertwined III: $f{\sigma }_8$ and $S_8$
• Non-minimal dark sector physics and cosmological tensions
• Can interacting dark energy solve the $H_0$ tension?
• Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy
• Early dark energy, the Hubble-parameter tension, and the string axiverse
• Cosmology with the Laser Interferometer Space Antenna
• 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
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Global constraints on absolute neutrino masses and their ordering
• Are merging black holes born from stellar collapse or previous mergers?
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Cosmological implications of ultra-light axion-like fields
• Early dark energy from massive neutrinos -- a natural resolution of the Hubble tension
• Acoustic Dark Energy: Potential Conversion of the Hubble Tension
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Local determination of the Hubble constant and the deceleration parameter
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant
• Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z)\ge -1$ are tighter than those obtained in $\Lambda$CDM
• Data Analysis for Precision 21 cm Cosmology
• Prospects for resolving the Hubble constant tension with standard sirens
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• Sterile neutrinos in cosmology
• New Early Dark Energy
• Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Hubble Sinks In The Low-Redshift Swampland
• The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
• KiDS-450: Testing extensions to the standard cosmological model
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Revisiting a negative cosmological constant from low-redshift data
• Reducing the $H_0$ and ${\sigma }_8$ tensions with Dark Matter-neutrino interactions
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• The $H_0$ tension in light of vacuum dynamics in the Universe
• Running Hubble Tension and a H0 Diagnostic
• Refined Bounds on MeV-scale Thermal Dark Sectors from BBN and the CMB
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• A CMB Search for the Neutrino Mass Mechanism and its Relation to the $H_0$ Tension
• Primordial gravitational waves from NANOGrav: a broken power-law approach
• Structure formation in $f(T)$ gravity and a solution for $H_0$ tension
• A Vacuum Phase Transition Solves $H_0$ Tension
• Status of Light Sterile Neutrino Searches
• Dark Energy with Phantom Crossing and the $H_0$ tension
• Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension
• Investigating Cosmic Discordance
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Concerns regarding the use of black hole shadows as standard rulers
• Early modified gravity in light of the $H_0$ tension and LSS data
• Exploring Cosmic Origins with CORE: Cosmological Parameters
• Unified framework for Early Dark Energy from $\alpha$-attractors
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• Determining the Hubble constant from Hubble parameter measurements
• The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators
• Alleviating the $H_0$ and ${\sigma }_8$ anomalies with a decaying dark matter model
• Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• Pseudoscalar - sterile neutrino interactions: reconciling the cosmos with neutrino oscillations
• Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$
• Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
• Axion Gauge Field Inflation and Gravitational Leptogenesis: A Lower Bound on B Modes from the Matter-Antimatter Asymmetry of the Universe
• A $w-M$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension
• Implications of a transition in the dark energy equation of state for the $H_0$ and ${\sigma }_8$ tensions
• Partially Acoustic Dark Matter, Interacting Dark Radiation, and Large Scale Structure
• Density perturbations for running vacuum: a successful approach to structure formation and to the ${\sigma }_8$-tension
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• de Sitter Swampland, $H_0$ tension & observation
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Dynamical system analysis for accelerating models in non-metricity $f(Q)$ gravity
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• Dark energy in light of the early JWST observations: case for a negative cosmological constant?
• Direct Measurements of Neutrino Mass
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Impact of neutrino properties on the estimation of inflationary parameters from current and future observations
• A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
• Running vacuum in quantum field theory in curved spacetime: renormalizing ${\rho }_{vac}$ without $\sim m^4$ terms
• Detection of isotropic cosmic birefringence and its implications for axion-like particles including dark energy
• Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation
• Evidence for Emergent Dark Energy
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• Effects of neutrino mass hierarchies on dynamical dark energy models
• $H_0$ tension as a hint for a transition in gravitational theory
• Reconciling $H_0$ tension in a six parameter space?
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Neutrino Mass Bounds in the era of Tension Cosmology
• Do cosmological observations allow a negative $\Lambda$?
• Cosmological discordances II: Hubble constant, Planck and large-scale-structure data sets
• Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously
• The state of the dark energy equation of state circa 2023
• On the homogeneity of SnIa absolute magnitude in the Pantheon+ sample
• Cosmology in Extended Parameter Space with DESI Data Release 2 Baryon Acoustic Oscillations: A 2$\sigma$+ Detection of Nonzero Neutrino Masses with an Update on Dynamical Dark Energy and Lensing Anomaly
• Cosmological Constraints on Interacting Light Particles
• Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
• Brans-Dicke cosmology with a $\Lambda$- term: a possible solution to $\Lambda$CDM tensions
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• Towards early dark energy and $n_s$=1 with Planck, ACT and SPT
• Residual Non-Abelian Dark Matter and Dark Radiation
• Cosmological discordances: a new measure, marginalization effects, and application to geometry vs growth current data sets
• Impacts of dark energy on weighing neutrinos: mass hierarchies considered
• Late time transitions in the quintessence field and the $H_0$ tension
• Soundness of Dark Energy properties
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Late time interacting cosmologies and the Hubble constant tension
• Cosmology and the neutrino mass ordering
• $T_0$ censorship of early dark energy and AdS vacua
• Observational Constraints on Oscillating Dark-Energy Parametrizations
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Phase Portraits of general f(T) Cosmology
• The Impact of Peculiar Velocities on the Estimation of the Hubble Constant from Gravitational Wave Standard Sirens
• Dark Neutrino interactions phase out the Hubble tension
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Unbiased Hubble constant estimation from binary neutron star mergers
• Data-driven Reconstruction of the Late-time Cosmic Acceleration with f(T) Gravity
• Neutrino-Assisted Early Dark Energy: Theory and Cosmology
• The Price of Shifting the Hubble Constant
• Changing the prior: absolute neutrino mass constraints in nonlocal gravity
• An evaluation of cosmological models from expansion and growth of structure measurements
• Robust and model-independent cosmological constraints from distance measurements
• Challenging bulk viscous unified scenarios with cosmological observations
• The $H_0$ and ${\sigma }_8$ tensions and the scale invariant spectrum
• Reconciling Large And Small-Scale Structure In Twin Higgs Models
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• The resilience of the Etherington-Hubble relation
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Emergent Dark Energy, neutrinos and cosmological tensions
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Hidden Charged Dark Matter and Chiral Dark Radiation
• Phantom cosmological model with observational constraints in $f(Q)$ gravity
• Bayesian Evidence against Harrison-Zel'dovich spectrum in tension cosmology
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• Revealing the late-time transition of $H_0$: relieve the Hubble crisis
• Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\Lambda$CDM cosmology
• Constraints on quintessence scalar field models using cosmological observations
• Quantifying Tensions between CMB and Distance Datasets in Models with Free Curvature or Lensing Amplitude
• A measurement of the Hubble constant using galaxy redshift surveys
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• What it takes to solve the Hubble tension through modifications of cosmological recombination
• $H_0$ tension and the String Swampland
• Rip cosmological models in extended symmetric teleparallel gravity
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Accelerating cosmological models in $f(Q)$ gravity and the phase space analysis
• On the dynamics of a dark sector coupling
• Late time acceleration due to generic modification of gravity and Hubble tension
• A Bayesian interpretation of inconsistency measures in cosmology
• Cornering the Planck $A_{lens}$ tension with future CMB data
• Do joint CMB and HST data support a scale invariant spectrum?
• Power-law cosmology in Weyl-type $f(Q,T)$ gravity
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• $H_0$ Tension and the Phantom Regime: A Case Study In Terms of an Infrared $f(T)$ Gravity
• Toward a concordance teleparallel Cosmology I: Background Dynamics
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Smoothing the $H_0$ tension with a dynamical dark energy model
• No H_0 Assistance from Assisted Quintessence
• Analyzing the geometrical and dynamical parameters of modified Teleparallel-Gauss-Bonnet model
• A Universe Without Dark Energy: Cosmic Acceleration from Dark Matter-Baryon Interactions
• Testing Predictions of the Quantum Landscape Multiverse 2: The Exponential Inflationary Potential
• Testing Predictions of the Quantum Landscape Multiverse 1: The Starobinsky Inflationary Potential
• Measuring the reionization optical depth without large-scale CMB polarization
• Multiple transitions in vacuum dark energy and $H_0$ tension
• Median statistics estimates of Hubble and Newton's Constant
• Constraining the dark-energy equation of state with cosmological data
• Dynamical system analysis in teleparallel gravity with boundary term
• Strong Bounds on Sum of Neutrino Masses in a 12 Parameter Extended Scenario with Non-Phantom Dynamical Dark Energy ($w(z)\ge -1$)
• Evaporating primordial black holes as varying dark energy
• Weyl type $f(Q,T)$ gravity observational constrained cosmological model
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Implications of an extended dark energy model with massive neutrinos
• Scalar field as a perfect fluid: thermodynamics of minimally coupled scalars and Einstein frame scalar-tensor gravity
• Towards a possible solution to the Hubble tension with Horndeski gravity
• Isotropic vs. Anisotropic components of BAO data: a tool for model selection
• A comment on power-law inflation with a dark radiation component
• New late-time constraints on $f(R)$ gravity
• Impact of the Hubble tension on the $r$-$n_s$ contour
• Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly
• The Hubble-Lemaître constant and sound horizon from low-redshift probes
• Phantom braneworld and the Hubble tension
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• Phenomenological Reconstruction of $f(T)$ Teleparallel Gravity
• New parametrization of the dark-energy equation of state with a single parameter
• Hubble constant and sound horizon from the late-time Universe
• The role of CMB spectral distortions in the Hubble tension: a proof of principle
• Constraints on Newton's Constant from Cosmological Observations
• Cascading Dark Energy
• Cosmological discordances III: more on measure properties, Large-Scale-Structure constraints, the Hubble constant and Planck
• Cosmic variance of $H_0$ in light of forthcoming high-redshift surveys
• Thermal Dark Energy
• Cosmographic Footprints of Dynamical Dark Energy
• Exploring Universe acceleration through observational constraints via Hubble parameter reconstruction
• Gravitino/Axino as Decaying Dark Matter and Cosmological Tensions
• Probing dynamics of dark energy with latest observations
• Vacuum dynamics in the Universe versus a rigid $\Lambda =$const
• Probing spatial variation of the fine-structure constant using the CMB
• Isocurvature Perturbations of Dark Energy and Dark Matter from the Swampland Conjecture
• The BAHAMAS project: Effects of dynamical dark energy on large-scale structure
• Redshift remapping and cosmic acceleration in dark-matter-dominated cosmological models
• Probing $\Lambda$CDM cosmology with the Evolutionary Map of the Universe survey
• Accelerating Cosmological Models in $f(T,B)$ Gravitational Theory
• Cosmological parameter forecasts by a joint 2D tomographic approach to CMB and galaxy clustering
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Differentiating dark interactions with perturbation
• Phantom crossing dark energy in Horndeski's theory
• The fate of bound systems through Sudden Future Singularities
• A novel model-marginalized cosmological bound on the QCD axion mass
• Gravitational Wave Opacity from Gauge Field Dark Energy
• Testing averaged cosmology with type Ia supernovae and BAO data
• Thomson scattering: One rate to rule them all
• Early Dark Energy from a Higher-dimensional Gauge Theory
• On the interacting dark energy scenarios $-$ the case for Hubble constant tension
• Hubble distancing: Focusing on distance measurements in cosmology
• Reducing the $H_0$ Tension with Exponential Acoustic Dark Energy
• Cosmological constraints from low-redshift data
• Generalized Brans-Dicke theories in light of evolving dark energy
• Gauged Quintessence
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• Geodesic deviation in Saez--Ballester theory
• Quantum origin of dark energy and the Hubble tension
• How robust are the parameter constraints extending the $\Lambda$CDM model?
• Calibrating Long Period Variables as Standard Candles with Machine Learning
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• A visual tool for assessing tension-resolving models in the $H_0$-${\sigma }_8$ plane
• Do we need wavelets in the late Universe?
• Imprint of baryons and massive neutrinos on velocity statistics
• Cosmological Distances And Hubble Tension In Einstein-Cartan Theory
• Dark energy constraint on equation of state parameter in the Weyl type $f(Q,T)$ gravity
• Possible Resolution of the Hubble Tension with Weyl Invariant Gravity
• Post-reionization HI 21-cm signal: A probe of negative cosmological constant
• Dynamical features of $f(T,B)$ cosmology
• Quantum Discrete Levels of the Universe from the Early Trans-Planckian Vacuum to the Late Dark Energy
• Distant foreground and the Planck-derived Hubble constant
• Observational constraints in Delta Gravity: CMB and supernovas
• Gravitational waves, CMB polarization, and the Hubble tension
• Non-particle dark matter from Hubble parameter
• Revisiting CPL with sign-switching density: To cross or not to cross the NECB
• Geometric Distances of Quasars Measured by Spectroastrometry and Reverberation Mapping:Monte Carlo Simulations
• Unveiling the Universe with Emerging Cosmological Probes
• The impact of 2D and 3D BAO measurements on the Cosmic Distance Duality Relation with HII galaxies
• Phantom Dirac-Born-Infeld Dark Energy
• Climbing out of the shadows: building the distance ladder with black hole images
• Hubble tension and matter inhomogeneities: a theoretical perspective
• Observational constraints on dynamical dark energy with pivoting redshift
• Fluctuating Dark Energy and the Luminosity Distance
• A varying Dark Energy effective speed of sound parameter in the phantom Universe
• Prospects of probing dark energy with eLISA: Standard versus null diagnostics
• The sounds of science a symphony for many instruments and voices part II
• Dynamical System Analysis for Scalar Field Potential in Teleparallel Gravity
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• New measures to test modified gravity cosmologies
• Data Analysis and Phenomenological Cosmology
• Vacuum Energy and Renormalization of the Field-Independent Term
• Cosmological singularities in non-canonical models of dark energy
• Neutrinos in Astrophysics and Cosmology: Theoretical Advanced Study Institute (TASI) 2020 Lectures
• Kinetic recoupling of dark matter
• A Geometric Probe of Cosmology: I. Gravitational Lensing Time Delays and Quasar Reverberation Mapping
• Single-object Imaging and Spectroscopy to Enhance Dark Energy Science from LSST
• Inhomogeneous Cosmology Redux
• Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data
• Reference frame dependence of the local measurement of the Hubble constant
• From Nonparametric Distance Reconstruction to Testing the Etherington Relation and Cosmic Curvature Using 2D and 3D BAO Measurements
• The four-dimensional null energy condition as a swampland conjecture
• Vacuum arbitrariness and the Hubble tension
• Yano-Schrödinger Hyperfluid: Cosmological Implications
• Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse