Updated constraints from the effective field theory analysis of BOSS power spectrum on Early Dark Energy

Abstract

Analyses of the full shape of BOSS DR12 power spectrum using the one-loop prediction from the Effective Field Theory of Large-Scale Structure (EFTBOSS) have led to new constraints on extensions to the $\Lambda$CDM model, such as Early Dark Energy (EDE) which has been suggested as a resolution to the "Hubble tension". In this paper, we re-assess the constraining power of the EFTBOSS on EDE in light of a correction to the normalization of BOSS window functions. Overall we find that constraints from EFTBOSS on EDE are weakened, and represent a small change compared to constraints from Planck and the conventional BAO/$f{\sigma }_8$ measurements. The combination of Planck data with EFTBOSS provides a bound on the maximal fractional contribution of EDE $f_{\mathrm{EDE}}<0.083$ at 95% C.L. (compared to $<0.054$ with the incorrect normalization, and $<0.088$ without full-shape data) and the Hubble tension is reduced to $2.1\sigma$. However, the more extreme model favored by an analysis with just data from the Atacama Cosmology Telescope is disfavored by the EFTBOSS data. We also show that the updated Pantheon+ Type Ia supernova analysis can slightly increase the constraints on EDE. Yet, the inclusion of the SN1a magnitude calibration by SH0ES strongly increases the preference for EDE to above $5\sigma$, yielding $f_{\mathrm{EDE}}\sim 0.12_{-0.02}^{+0.03}$ around the redshift $z_c=4365_{-1100}^{+3000}$. Our results demonstrate that EFTBOSS data (alone or combined with Planck data) do not exclude the EDE resolution of the Hubble tension.

17 + 13 pages, 11 figures. Comments welcome!

References in corpus (159)

• 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
• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• In the Realm of the Hubble tension $-$ a Review of Solutions
• 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
• The Pantheon+ Analysis: Cosmological Constraints
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• 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
• Power Spectrum Analysis of Three-Dimensional Redshift Surveys
• 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
• KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
• Planck 2018 results. VIII. Gravitational lensing
• The trouble with $H_0$
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey
• The Hubble Hunter's Guide
• Cosmological Non-Linearities as an Effective Fluid
• The Effective Field Theory of Cosmological Large Scale Structures
• Planck evidence for a closed Universe and a possible crisis for cosmology
• Measurements of the Hubble Constant: Tensions in Perspective
• One percent determination of the primordial deuterium abundance
• The $H_0$ Olympics: A fair ranking of proposed models
• 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
• The effects of He I 10830 on helium abundance determinations
• On the Hubble constant tension in the SNe Ia Pantheon sample
• Early dark energy, the Hubble-parameter tension, and the string axiverse
• Curvature tension: evidence for a closed universe
• TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions
• Early Dark Energy Does Not Restore Cosmological Concordance
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
• Cosmological implications of ultra-light axion-like fields
• The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space
• To H0 or not to H0?
• nbodykit: an open-source, massively parallel toolkit for large-scale structure
• Acoustic Dark Energy: Potential Conversion of the Hubble Tension
• The IR-resummed Effective Field Theory of Large Scale Structures
• Constraining Early Dark Energy with Large-Scale Structure
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• Elucidating $\Lambda$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
• Resolving the Hubble Tension with New Early Dark Energy
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• Is the Hubble tension a hint of AdS phase around recombination?
• Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant
• On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030
• Concordance and Discordance in Cosmology
• 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
• Relieving the Hubble tension with primordial magnetic fields
• Non-linear perturbation theory extension of the Boltzmann code CLASS
• Quantifying discordance in the 2015 Planck CMB spectrum
• Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
• Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
• Fast Estimators for Redshift-Space Clustering
• Bias in the Effective Field Theory of Large Scale Structures
• On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference
• Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• The BAO+BBN take on the Hubble tension
• A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey
• Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
• Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
• A non-linear solution to the $S_8$ tension?
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• It's Dust: Solving the Mysteries of the Intrinsic Scatter and Host-Galaxy Dependence of Standardized Type Ia Supernova Brightnesses
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• Early dark energy is not excluded by current large-scale structure data
• 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
• A CMB Search for the Neutrino Mass Mechanism and its Relation to the $H_0$ Tension
• Limits on $w$CDM from the EFTofLSS with the PyBird code
• Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate
• Measuring line-of-sight dependent Fourier-space clustering using FFTs
• Infrared Resummation for Biased Tracers in Redshift Space
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Early modified gravity in light of the $H_0$ tension and LSS data
• Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry
• Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies
• Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension
• The Atacama Cosmology Telescope: Constraints on Pre-Recombination Early Dark Energy
• A local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder
• Unified framework for Early Dark Energy from $\alpha$-attractors
• New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood
• A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
• PArthENoPE reloaded
• A larger value for $H_0$ by an evolving gravitational constant
• Thermal Friction as a Solution to the Hubble Tension
• Should Type Ia Supernova Distances be Corrected for their Local Environments?
• Brans-Dicke gravity with a cosmological constant smoothes out $\Lambda$CDM tensions
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release
• Using The Baryonic Tully-Fisher Relation to Measure $H_o$
• The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant
• Early recombination as a solution to the $H_0$ tension
• Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
• Interacting radiation after Planck and its implications for the Hubble Tension
• Interpreting cosmological tensions from the effective field theory of torsional gravity
• 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
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• On the EFT of Large Scale Structures in Redshift Space
• A Step in Understanding the Hubble Tension
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Reconstructing Gravity on Cosmological Scales
• A complete FFT-based decomposition formalism for the redshift-space bispectrum
• Interpreting measurements of the anisotropic galaxy power spectrum
• New Early Dark Energy is compatible with current LSS data
• Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
• Cosmological Hints of Modified Gravity ?
• Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
• Cosmological constraints on neutrino self-interactions with a light mediator
• Phenomenology of Modified Gravity at Recombination
• A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• Sensitivity of the Hubble Constant Determination to Cepheid Calibration
• Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
• Dark Sector to Restore Cosmological Concordance
• Brans-Dicke cosmology with a $\Lambda$- term: a possible solution to $\Lambda$CDM tensions
• Integral constraints in spectroscopic surveys
• The $H_0$ tension: $\Delta G_N$ vs. $\Delta N_{\mathrm{eff}}$
• Towards early dark energy and $n_s$=1 with Planck, ACT and SPT
• The trouble beyond $H_0$ and the new cosmic triangles
• The Hubble tension and a renormalizable model of gauged neutrino self-interactions
• CMB and BAO constraints for an induced gravity dark energy model with a quartic potential
• The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation
• The Hubble Tension Revisited: Additional Local Distance Ladder Uncertainties
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• Hybrid cosmological attractors
• The Early Dark Sector, the Hubble Tension, and the Swampland
• Cosmological constraints on induced gravity dark energy models
• Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum
• Dark Neutrino interactions phase out the Hubble tension
• An analytic implementation of the IR-resummation for the BAO peak
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• Very Hairy Inflation
• Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data
• Cosmological implications of $n_s\approx 1$ in light of the Hubble tension
• Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Microphysics of Early Dark Energy
• Optimal Weighting Scheme in Redshift-space Power Spectrum Analysis and a Prospect for Measuring the Cosmic Equation of State
• BOSS full-shape analysis from the EFTofLSS with exact time dependence
• Two sides of the same coin: sterile neutrinos and dark radiation. Status and perspectives

Cited by in corpus (32)

• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Rock 'n' Roll Solutions to the Hubble Tension
• Resolving the Hubble tension with Early Dark Energy
• Consistency of effective field theory analyses of the BOSS power spectrum
• A double take on early and interacting dark energy from JWST
• A tale of two (or more) $h$'s
• Return of Harrison-Zeldovich spectrum in light of recent cosmological tensions
• Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Observational constraints on early dark energy
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• A Dark Matter Trigger for Early Dark Energy Coincidence
• A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
• Profiling Cold New Early Dark Energy
• The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
• Testing signatures of phantom crossing through full-shape galaxy clustering analysis
• Dark energy by natural evolution: Constraining dark energy using Approximate Bayesian Computation
• On the consistency of $\Lambda$CDM with CMB measurements in light of the latest Planck, ACT, and SPT data
• Phantom scalar-tensor models and cosmological tensions
• Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
• New late-time constraints on $f(R)$ gravity
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• Testing the $n_s-H_0$ scaling relation with Planck-independent CMB data
• Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag
• Does the fraction of dark matter diminish with early dark energy?
• Early dark energy constraints with late-time expansion marginalization
• Can Early Dark Energy be Probed by the High-Redshift Galaxy Abundance?
• One Extension to Explain Them All, One Scale-Invariant Spectrum to Test Them All, and in One Model Bind Them
• Improving CMB constraints on early Universe physics with LSS: A multi-probe forecast including cross-covariance
• A frequentist view on the two-body decaying dark matter model