Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension

Abstract

We discuss the neutrino mass and Hubble tension solutions and examine their effects on the redshift-space distortion (RSD) observations. An analysis with RSD data indicates smaller amplitude of perturbation. Including RSD data results in a slightly weaker upper limit on the neutrino mass than that derived for data without RSD, which is common in other extended models too. We have evaluated the impacts of RSD observations on some extended models, including the varying electron mass model, a time-dependent dark energy model with two parameter equations of state (EOS), and a model where the number of neutrino species is free. When we estimate the cosmological parameters for data including RSD, we found that the EOS parameter for dark energy is larger than that of the cosmological constant, and the effective number of neutrino species is smaller than the standard value, which infers a smaller present Hubble parameter $H_0$. From the viewpoint of cosmological tensions, the varying electron mass model with nonzero neutrino mass option looks promising to relax the Hubble tension and the $S_8$ tension simultaneously.

arXiv comment26 pages, 7 figures

References in corpus (76)

• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• 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
• Exploring the Expansion History of the Universe
• Accelerating Universes with Scaling Dark Matter
• 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
• DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
• Massive neutrinos and cosmology
• Early Dark Energy Can Resolve The Hubble Tension
• Challenges for $\Lambda$CDM: An update
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Planck 2018 results. VIII. Gravitational lensing
• Measurements of the Hubble Constant: Tensions in Perspective
• New physics in light of the $H_0$ tension: an alternative view
• The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
• An improved upper limit on the neutrino mass from a direct kinematic method by KATRIN
• The $H_0$ Olympics: A fair ranking of proposed models
• Calibration of the Tip of the Red Giant Branch (TRGB)
• Reconstructing the history of structure formation using redshift distortions
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2
• Cosmological implications of ultra-light axion-like fields
• KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering
• Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure
• Acoustic Dark Energy: Potential Conversion of the Hubble Tension
• The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at $z\sim 1.4$
• Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure
• Resolving the Hubble Tension with New Early Dark Energy
• Is the Hubble tension a hint of AdS phase around recombination?
• Tension and constraints on modified gravity parametrizations of $G_{\text{eff}}(z)$ from growth rate and Planck data
• New Early Dark Energy
• Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• Rock 'n' Roll Solutions to the Hubble Tension
• Early modified gravity in light of the $H_0$ tension and LSS data
• Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension
• Joint analysis of 6dFGS and SDSS peculiar velocities for the growth rate of cosmic structure and tests of gravity
• Unified framework for Early Dark Energy from $\alpha$-attractors
• On the most constraining cosmological neutrino mass bounds
• Early recombination as a solution to the $H_0$ tension
• Density perturbations for running vacuum: a successful approach to structure formation and to the ${\sigma }_8$-tension
• New constraints on time-dependent variations of fundamental constants using Planck data
• Quantifying the $S_8$ tension with the Redshift Space Distortion data set
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• Evidence for suppression of structure growth in the concordance cosmological model
• Massive neutrinos and cosmic composition
• KiDS+VIKING-450: Improved cosmological parameter constraints from redshift calibration with self-organising maps
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• Relaxing the ${\sigma }_8$-tension through running vacuum in the Universe
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• Galaxy and Mass Assembly (GAMA): Redshift Space Distortions from the Clipped Galaxy Field
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
• Cosmological Constraints on a Dynamical Electron Mass
• $S_8$ increases with effective redshift in $\Lambda$CDM cosmology
• Constraints on neutrino mass from Cosmic Microwave Background and Large Scale Structure
• The growth rate of cosmic structures in the local Universe with the ALFALFA survey
• How to relax the cosmological neutrino mass bound
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Unbiased clustering estimate with VIPERS slit assignment
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Hubble tension in lepton asymmetric cosmology with an extra radiation
• Testing for dynamical dark energy models with redshift-space distortions
• Cascading Dark Energy
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Environment Dependent Electron Mass and the H${}_0$-Tension
• Constraining Holographic Dark Energy and Analyzing Cosmological Tensions

Cited by in corpus (3)

• Probing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data
• Constraints on the varying electron mass and early dark energy in light of ACT DR6 and DESI DR2 and the implications for inflation
• Testing Lens Models of PLCK G165.7+67.0 Using Lensed SN H0pe