CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity

Abstract

With the recent increase in precision of our cosmological datasets, measurements of $\Lambda$CDM model parameter provided by high- and low-redshift observations started to be in tension, i.e., the obtained values of such parameters were shown to be significantly different in a statistical sense. In~this work we tackle the tension on the value of the Hubble parameter, $H_0$, and the weighted amplitude of matter fluctuations, $S_8$, obtained from local or low-redshift measurements and from cosmic microwave background (CMB) observations. We combine the main approaches previously used in the literature by extending the cosmological model and accounting for extra systematic uncertainties. With such analysis we aim at exploring non standard cosmological models, implying deviation from a cosmological constant driven acceleration of the Universe expansion, in the presence of additional uncertainties in measurements. In more detail, we reconstruct the Dark Energy equation of state as a function of redshift, while we study the impact of type-Ia supernovae (SNIa) redshift-dependent astrophysical systematic effects on these tensions. We consider a SNIa intrinsic luminosity dependence on redshift due to the star formation rate in its environment, or the metallicity of the progenitor. We find that the $H_0$ and $S_8$ tensions can be significantly alleviated, or~even removed, if we account for varying Dark Energy for SNIa and CMB data. However, the tensions remain when we add baryon acoustic oscillations (BAO) data into the analysis, even after the addition of extra SNIa systematic uncertainties. This points towards the need of either new physics beyond late-time Dark Energy, or other unaccounted systematic effects (particulary in BAO measurements), to fully solve the present tensions.

arXiv comment22 pages, 6 figures. New version matching the one accepted by Symmetry

References in corpus (89)

• Galactic Stellar and Substellar Initial Mass Function
• On the variation of the Initial Mass Function
• Cosmic Star Formation History
• 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 2.4% Determination of the Local Value of the Hubble Constant
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• 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
• Galaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation
• Formation of Massive Galaxies at High Redshift: Cold Streams, Clumpy Disks and Compact Spheroids
• Early Dark Energy Can Resolve The Hubble Tension
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
• Cosmological implications of baryon acoustic oscillation (BAO) measurements
• The trouble with $H_0$
• Imperfect Dark Energy from Kinetic Gravity Braiding
• Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
• Efficient sampling of fast and slow cosmological parameters
• The supernova rate per unit mass
• New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant
• Probing the dark energy: methods and strategies
• Prospects for probing the dark energy via supernova distance measurements
• SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes
• Can interacting dark energy solve the $H_0$ tension?
• Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
• H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant
• Reconciling Planck with the local value of $H_0$ in extended parameter space
• The Type Ia Supernova Rate
• On Variations in the Peak Luminosity of Type Ia Supernovae
• Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially-Flat $\Lambda$cdm Model, The Deceleration-Acceleration Transition Redshift, and Spatial Curvature
• Does the Hubble constant tension call for new physics?
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• Acoustic Dark Energy: Potential Conversion of the Hubble Tension
• Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant
• Concordance and Discordance in Cosmology
• Median Statistics, H_0, and the Accelerating Universe
• Evidence of Environmental Dependencies of Type Ia Supernovae from the Nearby Supernova Factory indicated by Local Hα
• Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension
• The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions
• KiDS-450: Testing extensions to the standard cosmological model
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Reducing the $H_0$ and ${\sigma }_8$ tensions with Dark Matter-neutrino interactions
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• A Vacuum Phase Transition Solves $H_0$ Tension
• The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic survey
• Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension
• The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant
• Median statistics and the Hubble constant
• An improved model-independent assessment of the late-time cosmic expansion
• Determining the Hubble constant from Hubble parameter measurements
• Modern yields per stellar generation: the effect of the IMF
• Ages of Type Ia Supernovae Over Cosmic Time
• Should Type Ia Supernova Distances be Corrected for their Local Environments?
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Axion-Dilaton Destabilization and the Hubble Tension
• Can we be tricked into thinking that w is less than -1?
• The value of H_0 in the inhomogeneous Universe
• Galaxy And Mass Assembly (GAMA): Linking Star Formation Histories and Stellar Mass Growth
• GAIA Cepheid parallaxes and 'Local Hole' relieve $H_0$ tension
• Implications of a transition in the dark energy equation of state for the $H_0$ and ${\sigma }_8$ tensions
• Non-Gaussian Error Distribution of Hubble Constant Measurements
• Feasibility of Reconstructing the Quintessential Potential Using SNIa Data
• Metallicity effect in multi-dimensional SNIa nucleosynthesis
• SNe Ia host galaxy properties from Sloan Digital Sky Survey-II spectroscopy
• $H_0$ tension as a hint for a transition in gravitational theory
• Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously
• Is cosmic acceleration proven by local cosmological probes?
• Think Global, Act Local: The Influence of Environment Age and Host Mass on Type Ia Supernova Light Curves
• The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference
• Statistical Inconsistencies in the KiDS-450 Dataset
• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
• Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
• Model-independent cosmic acceleration and type Ia supernovae intrinsic luminosity redshift dependence
• Cosmic distance inference from purely geometric BAO methods: Linear Point standard ruler and Correlation Function Model Fitting
• On the dependence of the type Ia SNe luminosities on the metallicity of their host galaxies
• Impact of theoretical priors in cosmological analyses: the case of single field quintessence
• Dark Energy coupling with electromagnetism as seen from future low-medium redshift probes
• Models for Type Ia supernovae and related astrophysical transients
• Using the local gas-phase oxygen abundances to explore a metallicity-dependence in SNe Ia luminosities
• Model Independent Expansion History from Supernovae: Cosmology versus Systematics
• Does Quartessence Ease Tensions?
• Super-CMB fluctuations and the Hubble tension
• Seven Problems with the Claims Related to the Hubble Tension in arXiv:1810.02595

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• In the Realm of the Hubble tension $-$ a Review of Solutions
• Challenges for $\Lambda$CDM: An update
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• New physics in light of the $H_0$ tension: an alternative view
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Dark Energy with Phantom Crossing and the $H_0$ tension
• Investigating Cosmic Discordance
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• Analyzing the $H_0$ tension in $F(R)$ gravity models
• Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
• Using quasar X-ray and UV flux measurements to constrain cosmological model parameters
• Relieving the $H_0$ tension with a new interacting dark energy model
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Reconciling $H_0$ tension in a six parameter space?
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
• The resilience of the Etherington-Hubble relation
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Exploring the evidence for a large local void with supernovae Ia data
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Sub-Planckian ${\varphi }^2$ Inflation in the Palatini Formulation of Gravity with an $R^2$ term
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Latest evidence for a late time vacuum -- geodesic CDM interaction
• Gaussian Processes Reconstruction of the Dark Energy Potential
• New late-time constraints on $f(R)$ gravity
• Dark matter from torsion in Friedmann cosmology
• Observational constraints on varying fundamental constants in a minimal CPC model
• Can the Universe decelerate in the future?
• Magnification and evolution bias of transient sources: GWs and SNIa
• Dark Gravitational Field on Riemannian and Sasaki Spacetime
• Climbing out of the shadows: building the distance ladder with black hole images
• Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
• Kinematic reconstruction of torsion as dark energy in Friedmann cosmology