The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data

Abstract

The disagreement between direct late-time measurements of the Hubble constant from the SH0ES collaboration, and early-universe measurements based on the $\Lambda$CDM model from the Planck collaboration might, at least in principle, be explained by new physics in the early universe. Recently, the application of the Effective Field Theory of Large-Scale Structure to the full shape of the power spectrum of the SDSS/BOSS data has revealed a new, rather powerful, way to measure the Hubble constant and the other cosmological parameters from Large-Scale Structure surveys. In light of this, we analyze two models for early universe physics, Early Dark Energy and Rock 'n' Roll, that were designed to significantly ameliorate the Hubble tension. Upon including the information from the full shape to the Planck, BAO, and Supernovae measurements, we find that the degeneracies in the cosmological parameters that were introduced by these models are well broken by the data, so that these two models do not significantly ameliorate the tension.

15+12 pages, 7 figures. v2: Minor corrections, references added. v3: Extended appendices

References in corpus (21)

• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• The Effective Field Theory of Cosmological Large Scale Structures
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• Early Dark Energy Does Not Restore Cosmological Concordance
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0
• The IR-resummed Effective Field Theory of Large Scale Structures
• Resolving the Hubble Tension with New Early Dark Energy
• Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogs for Cosmological Analysis
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• Limits on $w$CDM from the EFTofLSS with the PyBird code
• Is there an early Universe solution to Hubble tension?
• The Bispectrum in the Effective Field Theory of Large Scale Structure
• Dark energy from the string axiverse
• Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
• Over-constrained Gravitational Lens Models and the Hubble Constant
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• Inflation Wars: A New Hope
• Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure

Cited by in corpus (96)

• Challenges for $\Lambda$CDM: An update
• The $H_0$ Olympics: A fair ranking of proposed models
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• New Horizons for Fundamental Physics with LISA
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• Is Local $H_0$ At Odds With Dark Energy EFT?
• The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy
• New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• Restoring cosmological concordance with early dark energy and massive neutrinos?
• Hints of FLRW Breakdown from Supernovae
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
• Precision analysis of the redshift-space galaxy bispectrum
• Dark sector interaction and the supernova absolute magnitude tension
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Neutrino Self-Interactions: A White Paper
• A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology
• Dark Sector to Restore Cosmological Concordance
• The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure
• Early-Universe-Physics Insensitive and Uncalibrated Cosmic Standards: Constraints on ${\Omega }_{\mathrm{m}}$ and Implications for the Hubble Tension
• Resolving the Hubble tension with Early Dark Energy
• Updated constraints from the effective field theory analysis of BOSS power spectrum on Early Dark Energy
• No-go guide for the Hubble tension : Late-time solutions
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• The Early Dark Sector, the Hubble Tension, and the Swampland
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Neutrino-Assisted Early Dark Energy: Theory and Cosmology
• Isotropic cosmic birefringence from early dark energy
• Testing AdS early dark energy with Planck, SPTpol and LSS data
• Hot New Early Dark Energy
• Towards hybrid inflation with $n_s=1$ in light of Hubble tension and primordial gravitational waves
• Constraints on modified gravity from the BOSS galaxy survey
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
• Hot New Early Dark Energy: Towards a Unified Dark Sector of Neutrinos, Dark Energy and Dark Matter
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Cosmological constraints from the power spectrum of eBOSS quasars
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Observational constraints on early dark energy
• Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Microphysics of Early Dark Energy
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Multiple transitions in vacuum dark energy and $H_0$ tension
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• Early Dark Energy in Type IIB String Theory
• Profiling Cold New Early Dark Energy
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• Limits on Clustering and Smooth Quintessence from the EFTofLSS
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Addressing the Hubble and $S_8$ Tensions with a Kinetically Mixed Dark Sector
• Taming redshift-space distortion effects in the EFTofLSS and its application to data
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
• Detecting the power spectrum turnover with HI intensity mapping
• BOSS full-shape analysis from the EFTofLSS with exact time dependence
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• Cosmology from weak lensing alone and implications for the Hubble tension
• Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag
• Neutrino masses from large-scale structures: future sensitivity and theory dependence
• Early dark energy by dark Higgs, and axion-induced non-thermal trapping
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• Does the fraction of dark matter diminish with early dark energy?
• Explanation of high redshift luminous galaxies from JWST by early dark energy model
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Coupled Dark Sector Models and Cosmological Tensions
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Incompatibility of fine-structure constant variations at recombination with local observations
• Chameleon Early Dark Energy and the Hubble Tension
• Cosmology at high redshift -- a probe of fundamental physics
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• Predictive uncertainty on improved astrophysics recovery from multifield cosmology
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Early dark energy in the pre- and post-recombination epochs
• $\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum
• Sound Horizon Independent Constraints on Early Dark Energy: The Role of Supernova Data
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order