Equality scale-based and sound horizon-based analysis of the Hubble tension

Abstract

The Hubble horizon at matter-radiation equality ($k_{\mathrm{eq}}^{-1}$) and the sound horizon at the last scattering surface ($r_s(z_{\ast })$) provides interesting consistency check for the $\Lambda$CDM model and its extensions. It is well known that the reduction of $r_s$ can be compensated by the increase of $H_0$, while the same is true for the standard rulers $k_{\mathrm{eq}}$. Adding extra radiational component to the early universe can reduce $k_{\mathrm{eq}}$. The addition of early dark energy (EDE), however, tends to increase $k_{\mathrm{eq}}$. We perform $k_{\mathrm{eq}}$- and $r_s$-based analyses in both the EDE model and the Wess-Zumino Dark Radiation (WZDR) model. In the latter case we find $\Delta H_0=0.4$ between the $r_s$- and $k_{\mathrm{eq}}$-based datasets, while in the former case we find $\Delta H_0=1.2$. This result suggests that the dark radiation scenario is more consistent in the fit of the two standard rulers ($k_{\mathrm{eq}}$ and $r_s$). As a forecast analyses, we fit the two models with a mock $k_{\mathrm{eq}}$ prior derived from \emph{Planck} best-fit $\Lambda$CDM model. Compared with the best-fit $H_0$ in baseline $\Lambda$CDM model, we find $\Delta H_0=1.1$ for WZDR model and $\Delta H_0=-2.4$ for EDE model.

arXiv comment12 pages, 7 figures

References in corpus (84)

• 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 Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
• 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
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• The Baryon Oscillation Spectroscopic Survey of SDSS-III
• 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 Pantheon+ Analysis: Cosmological Constraints
• Dark Energy Survey Year 1 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
• Planck 2018 results. V. CMB power spectra and likelihoods
• Early Dark Energy Can Resolve The Hubble Tension
• Challenges for $\Lambda$CDM: An update
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• The trouble with $H_0$
• Measurements of the Hubble Constant: Tensions in Perspective
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
• New physics in light of the $H_0$ tension: an alternative view
• The non-gravitational interactions of dark matter in colliding galaxy clusters
• The $H_0$ Olympics: A fair ranking of proposed models
• Cosmological Parameters from the BOSS Galaxy Power Spectrum
• An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
• Measurement of BAO correlations at $z=2.3$ with SDSS DR12 \lya-Forests
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
• Early Dark Energy Does Not Restore Cosmological Concordance
• Cosmological implications of ultra-light axion-like fields
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• 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?
• KiDS+GAMA: Cosmology constraints from a joint analysis of cosmic shear, galaxy-galaxy lensing and angular clustering
• Non-linear perturbation theory extension of the Boltzmann code CLASS
• Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
• Distance Priors from Planck Final Release
• A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
• On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• Can Late Dark Energy Transitions Raise the Hubble constant?
• Interacting Dark Sector and Precision Cosmology
• Running Hubble Tension and a H0 Diagnostic
• Is there an early Universe solution to Hubble tension?
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range $0.8<z<2.2$
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies
• A rapid transition of $G_{\mathrm{eff}}$ at $z_t\simeq 0.01$ as a solution of the Hubble and growth tensions
• Thermal Friction as a Solution to the Hubble Tension
• Alleviating the $H_0$ and ${\sigma }_8$ anomalies with a decaying dark matter model
• Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles
• Neutrinos help reconcile Planck measurements with both Early and Local Universe
• A $w-M$ phantom transition at $z_t<0.1$ as a resolution of the Hubble tension
• A late-time transition in the cosmic dark energy?
• Implications of a transition in the dark energy equation of state for the $H_0$ and ${\sigma }_8$ tensions
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• A Step in Understanding the Hubble Tension
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
• Determining the Hubble Constant without the Sound Horizon: Measurements from Galaxy Surveys
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• Sensitivity of the Hubble Constant Determination to Cepheid Calibration
• Equivalent Neutrinos, Light WIMPs, and the Chimera of Dark Radiation
• Early mass varying neutrino dark energy: Nugget formation and Hubble anomaly
• Cosmological constraints on multi-interacting dark matter
• Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing
• Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
• A fresh look into the interacting dark matter scenario
• Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae
• Hints for a gravitational constant transition in Tully-Fisher data
• Can Early Dark Energy Explain EDGES?
• Did the Universe Experienced a Pressure non-Crushing Type Cosmological Singularity in the Recent Past?
• Is the $H_0$ tension suggesting a 4th neutrino's generation?
• Integral $F(R)$ Gravity and Saddle Point Condition as a Remedy for the $H_0$-tension
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
• No-go guide for late-time solutions to the Hubble tension: Matter perturbations
• Dissimilar Donuts in the Sky? Effects of a Pressure Singularity on the Circular Photon Orbits and Shadow of a Cosmological Black Hole
• Wandering in the Lyman-alpha Forest: A Study of Dark Matter-Dark Radiation Interactions
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• Analyzing the Hubble tension through hidden sector dynamics in the early universe
• Cosmological search for sterile neutrinos after Planck 2018
• Searching for Signatures of Dark matter-Dark Radiation Interaction in Observations of Large-scale Structure
• Early-time thermalization of cosmic components? A hint for solving cosmic tensions

Cited by in corpus (2)

• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Particle physics and cosmology intertwined