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.

arXiv comment15+12 pages, 7 figures. v2: Minor corrections, references added. v3: Extended appendices

References in corpus (91)

• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• 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
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Tensions between the Early and the Late Universe
• H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
• Early Dark Energy Can Resolve The Hubble Tension
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• The Hubble Hunter's Guide
• Cosmological Non-Linearities as an Effective Fluid
• The Effective Field Theory of Cosmological Large Scale Structures
• A classification of scalar field potentials with cosmological scaling solutions
• The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• Cosmological Parameters from the BOSS Galaxy Power Spectrum
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra
• The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions
• 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
• Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
• Early dark energy from massive neutrinos -- a natural resolution of the Hubble tension
• Acoustic Dark Energy: Potential Conversion of the Hubble Tension
• The IR-resummed Effective Field Theory of Large Scale Structures
• Baryon acoustic oscillations from the cross-correlation of Ly$\alpha$ absorption and quasars in eBOSS DR14
• Resolving the Hubble Tension with New Early Dark Energy
• Elucidating $\Lambda$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
• Baryon acoustic oscillations at z = 2.34 from the correlations of Ly$\alpha$ absorption in eBOSS DR14
• New Early Dark Energy
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Equivalence Principle and the Baryon Acoustic Peak
• Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
• Bias in the Effective Field Theory of Large Scale Structures
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
• Biased Tracers and Time Evolution
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogs for Cosmological Analysis
• The Effective Field Theory of Large Scale Structures at Two Loops
• On the Renormalization of the Effective Field Theory of Large Scale Structures
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• 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
• The Effective Field Theory of Large Scale Structure at Two Loops: the apparent scale dependence of the speed of sound
• Axion-Dilaton Destabilization and the Hubble Tension
• A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations
• Galaxy Bias and Primordial Non-Gaussianity
• Cosmological Perturbation Theory Using the FFTLog: Formalism and Connection to QFT Loop Integrals
• The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures
• Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
• The 2-loop matter power spectrum and the IR-safe integrand
• Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations
• On the Velocity in the Effective Field Theory of Large Scale Structures
• On the EFT of Large Scale Structures in Redshift Space
• Over-constrained Gravitational Lens Models and the Hubble Constant
• Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
• On the IR-Resummation in the EFTofLSS
• Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure
• Cosmological perturbation theory in 1+1 dimensions
• On the reach of perturbative descriptions for dark matter displacement fields
• Systematic Renormalization of the Effective Theory of Large Scale Structure
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• The Trispectrum in the Effective Field Theory of Large Scale Structure
• $\Lambda$CDM or self-interacting neutrinos? - how CMB data can tell the two models apart
• Dark Energy and Modified Gravity in the Effective Field Theory of Large-Scale Structure
• An analytic implementation of the IR-resummation for the BAO peak
• CMB-slow, or How to Estimate Cosmological Parameters by Hand
• Dark Energy, $H_0$ and Weak Gravity Conjecture
• Towards Precision Constraints on Gravity with the Effective Field Theory of Large-Scale Structure
• Very Massive Tracers and Higher Derivative Biases
• The EFT of Large Scale Structures at All Redshifts: Analytical Predictions for Lensing
• The Effective Field Theory of Large Scale Structure at Three Loops
• IR-safe and UV-safe integrands in the EFTofLSS with exact time dependence
• Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos
• On the reach of perturbative methods for dark matter density fields
• An effective description of dark matter and dark energy in the mildly non-linear regime
• Efficient exploration of cosmology dependence in the EFT of LSS
• On the Bispectra of Very Massive Tracers in the Effective Field Theory of Large-Scale Structure
• Inflation Wars: A New Hope
• Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure
• Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum

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• Neutrino-Assisted Early Dark Energy: Theory and Cosmology
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• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
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• 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
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• Addressing the Hubble and $S_8$ Tensions with a Kinetically Mixed Dark Sector
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• Predictive uncertainty on improved astrophysics recovery from multifield cosmology
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