Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys

Abstract

Two sources of geometric information are encoded in the galaxy power spectrum: the sound horizon at recombination and the horizon at matter-radiation equality. Analyzing the BOSS DR12 galaxy power spectra using perturbation theory with ${\Omega }_m$ priors from Pantheon supernovae but no priors on ${\Omega }_b$, we obtain constraints on $H_0$ from the second scale, finding $H_0=65.1_{-5.4}^{+3.0}\mathrm{km}{\mathrm{s}}^{-1}{\mathrm{Mpc}}^{-1}$; this differs from the best-fit of SH0ES at 95\% confidence. Similar results are obtained if ${\Omega }_m$ is constrained from uncalibrated BAO: $H_0=65.6_{-5.5}^{+3.4}\mathrm{km}{\mathrm{s}}^{-1}{\mathrm{Mpc}}^{-1}$. Adding the analogous lensing results from Baxter \& Sherwin 2020, the posterior shifts to $70.6_{-5.0}^{+3.7}\mathrm{km}{\mathrm{s}}^{-1}{\mathrm{Mpc}}^{-1}$. Using mock data, Fisher analyses, and scale-cuts, we demonstrate that our constraints do not receive significant information from the sound horizon scale. Since many models resolve the $H_0$ controversy by adding new physics to alter the sound horizon, our measurements are a consistency test for standard cosmology before recombination. A simple forecast indicates that such constraints could reach ${\sigma }_{H_0}\simeq 1.6\mathrm{km}{\mathrm{s}}^{-1}{\mathrm{Mpc}}^{-1}$ in the era of Euclid.

arXiv comment8 pages, 4 figures, accepted by Phys. Rev. D

References in corpus (46)

• 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
• Baryonic Features in the Matter Transfer Function
• SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
• The Baryon Oscillation Spectroscopic Survey of SDSS-III
• 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
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• A gravitational-wave standard siren measurement of the Hubble constant
• 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
• Planck 2018 results. V. CMB power spectra and likelihoods
• Massive neutrinos and cosmology
• The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Cosmological implications of baryon acoustic oscillation (BAO) measurements
• The Expansion of the Universe is Faster than Expected
• 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
• Measuring cosmological parameters with galaxy surveys
• TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
• Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
• Constraining Early Dark Energy with Large-Scale Structure
• Baryon acoustic oscillations from the cross-correlation of Ly$\alpha$ absorption and quasars in eBOSS DR14
• 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
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• Non-linear perturbation theory extension of the Boltzmann code CLASS
• Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Modeling the clustering and halo occupation distribution of BOSS-CMASS galaxies in the Final Data Release
• The BAO+BBN take on the Hubble tension
• Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data
• Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
• Using The Baryonic Tully-Fisher Relation to Measure $H_o$
• Analytic marginalization over CMB calibration and beam uncertainty
• A Lockdown Perspective on the Hubble Tension (with comments from the SH0ES team)
• Integral constraints in spectroscopic surveys
• Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Analytic Methods for Cosmological Likelihoods
• Peculiar velocities in the local Universe: comparison of different models and the implications for $H_0$ and dark matter
• The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure

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• A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond
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• Lifshitz cosmology: quantum vacuum and Hubble tension
• Observing relativistic features in large-scale structure surveys -- I: Multipoles of the power spectrum
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• Can the sound horizon-free measurement of $H_0$ constrain early new physics?
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