Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature

Abstract

In this paper we use all available baryon acoustic oscillation, Hubble parameter, and quasar angular size data to constrain six dark energy cosmological models, both spatially flat and non-flat. Depending on the model and data combination considered, these data mildly favor closed spatial hypersurfaces (by as much as $1.7\sigma$) and dark energy dynamics (up to a little over $2\sigma$) over a cosmological constant $\Lambda$. The data also favor, at $1.8\sigma$ to $3.4\sigma$, depending on the model and data combination, a lower Hubble constant than what is measured from the local expansion rate.

13 pages, 6 figures. This version has been updated to reflect referee comments, and to correct a mistake that was present in an earlier version (results largely unchanged). Accepted for publication in MNRAS

References in corpus (94)

• Planck 2015 results. XIII. Cosmological parameters
• 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
• A 2.4% Determination of the Local Value of the Hubble Constant
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• Information criteria for astrophysical model selection
• Quasar-Lyman $\alpha$ Forest Cross-Correlation from BOSS DR11 : Baryon Acoustic Oscillations
• New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant
• Measurement of BAO correlations at $z=2.3$ with SDSS DR12 \lya-Forests
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2
• Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
• Hubble parameter measurement constraints on the cosmological deceleration-acceleration transition redshift
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Determination of the Cosmic Distance Scale from Sunyaev-Zel'dovich Effect and Chandra X-ray Measurements of High Redshift Galaxy Clusters
• 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
• Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
• Distance measures in cosmology
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Median Statistics, H_0, and the Accelerating Universe
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• Consequences on variable Lambda-models from distant Type Ia supernovae and compact radio sources
• Median statistics and the Hubble constant
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Determining the Hubble constant from Hubble parameter measurements
• Evolution of dark energy reconstructed from the latest observations
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• Using the tilted flat-$\Lambda$CDM and the untilted non-flat $\Lambda$CDM inflation models to measure cosmological parameters from a compilation of observational data
• Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data
• Non-Gaussian Error Distribution of Hubble Constant Measurements
• Cardassian Expansion: Constraints from Compact Radio Source Angular Size versus Redshift Data
• Measuring the speed of light with ultra-compact radio quasars
• An independent determination of the local Hubble constant
• An Improved Method to Measure the Cosmic Curvature
• Observational constraints on the tilted spatially-flat and the untilted nonflat $\varphi$CDM dynamical dark energy inflation models
• Planck 2015 constraints on the non-flat $\Lambda$CDM inflation model
• Dark energy and the angular size - redshift diagram for milliarcsecond radio sources
• Cosmological Constraints from Compact Radio Source Angular Size versus Redshift Data
• Binned Hubble parameter measurements and the cosmological deceleration-acceleration transition
• Cosmological discordances II: Hubble constant, Planck and large-scale-structure data sets
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• New Model-independent Method to Test the Curvature of the Universe
• Constraining cosmic curvature by using age of galaxies and gravitational lenses
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• The distance sum rule from strong lensing systems and quasars - test of cosmic curvature and beyond
• Hubble parameter data constraints on dark energy
• New observational constraints on $f(T)$ cosmology from radio quasars
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• Nonflat time-variable dark energy cosmology
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• Constraining dark energy with gamma-ray bursts
• An evaluation of cosmological models from expansion and growth of structure measurements
• Radio Galaxy Redshift-Angular Size Data Constraints on Dark Energy
• Planck 2015 constraints on the non-flat XCDM inflation model
• Inflation in a closed universe
• Quintessence, Cosmology, and Fanaroff-Riley Type IIB Radio Galaxies
• Observational constraints on non-flat dynamical dark energy cosmological models
• Constraints on quintessence scalar field models using cosmological observations
• A measurement of the Hubble constant using galaxy redshift surveys
• A new test of $f(R)$ gravity with the cosmological standard rulers in radio quasars
• Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
• What is parameterized $Om(z)$ diagnostics telling us in light of recent observations?
• Model independent constraints on transition redshift
• Constraining the dark energy models with H(z) data: an approach independent of $H_0$
• Low redshift observational constraints on tachyon models of dark energy
• Constraints on dark energy from the lookback time versus redshift test
• Constraints on a $\varphi$CDM model from strong gravitational lensing and updated Hubble parameter measurements
• Exploring Parameter Constraints on Quintessential Dark Energy: the Inverse Power Law Model
• Model-independent curvature determination with 21cm intensity mapping experiments
• First study of reionization in the Planck 2015 normalized closed $\Lambda$CDM inflation model
• Constraining the dark energy statefinder hierarchy in a kinematic approach
• Using spatial curvature with HII galaxies and cosmic chronometers to explore the tension in $H_0$
• Galaxy cluster angular size data constraints on dark energy
• Constraints on field flows of quintessence dark energy
• Probing dynamics of dark energy with latest observations
• Galaxy Cluster Gas Mass Fraction and Hubble Parameter versus Redshift Constraints on Dark Energy
• Observational constraints on quintessence models of dark energy
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
• Prospect for cosmological parameter estimation using future Hubble parameter measurements
• First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
• Tight $H_0$ constraint from galaxy redshfit surveys: combining baryon acoustic osillation measurements and Alcock-Paczynski test
• Observational constraints on dark energy cosmological model parameters
• Median Statistics Analysis of Deuterium Abundance Measurements and Spatial Curvature Constraints
• Testing Dark Energy Models through Large Scale Structure
• Signs of Dynamical Dark Energy in Current Observations
• Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations
• A Model-Independent Measurement of the Spatial Curvature using Cosmic Chronometers and the HII Hubble Diagram
• Constraints on $H_0$ from WMAP and baryon acoustic osillation measurements
• Observational constraints on the jerk parameter with the data of the Hubble parameter
• A More Accurate and Competitive Estimative of $H_0$ in Intermediate Redshifts
• Testing and selecting cosmological models with ultra-compact radio quasars

Cited by in corpus (72)

• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• General Cosmography Model with Spatial Curvature
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Using the tilted flat-$\Lambda$CDM and the untilted non-flat $\Lambda$CDM inflation models to measure cosmological parameters from a compilation of observational data
• 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
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
• Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• Standardizing Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\varphi$CDM dark energy inflation cosmologies
• Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?
• Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Observational constraints on Myrzakulov gravity
• Planck 2015 constraints on spatially-flat dynamical dark energy models
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• Model-independent measurement of cosmic curvature with the latest $H(z)$ and SNe Ia data: A comprehensive investigation
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Probing modified gravity theories with multiple measurements of high-redshift quasars
• Ruling Out New Physics at Low Redshift as a solution to the $H_0$ Tension
• CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
• Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
• An 8.0\% Determination of the Baryon Fraction in the Intergalactic Medium from Localized Fast Radio Bursts
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Do reverberation-measured H$\beta$ quasars provide a useful test of cosmology?
• Measurement on the cosmic curvature using the Gaussian process method
• Consistency study of high- and low-accreting Mg ii quasars: No significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity relation dispersion
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• Observational Constraints on Dynamical Dark Energy Models
• Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Questioning the $H_0$ tension via the look-back time
• Cosmological Constraints on Non-flat Exponential $f(R)$ Gravity
• Comparing the scalar-field dark energy models with recent observations
• Hubble constant and sound horizon from the late-time Universe
• Revisiting Chaplygin gas cosmologies with the recent observations of high-redshfit quasars
• A critical discussion on the $H_0$ tension
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• Cosmological Constraints on the Coupling Model from Observational Hubble Parameter and Baryon Acoustic Oscillation Measurements
• The growth factor parametrization versus numerical solutions in flat and non-flat dark energy models
• First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
• Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample
• DECi-hertz Interferometer Gravitational-wave Observatory: Forecast constraints on the cosmic curvature with LSST strong lenses
• Constraints from observational data for a running cosmological constant and warm dark matter with curvature
• The Hubble tension: Change in dark energy or a case for modified gravity?
• Redshift-evolutionary X-ray and UV luminosity relation of quasars from Gaussian copula
• Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from MgII and CIV reverberation-mapped quasar data
• Constraints on power law cosmology from cosmic chronometer, standard ruler, and standard candle data
• Spatial Curvature in Cosmology Revisited
• Does spatial flatness forbid the turnaround epoch of collapsing structures?
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Dynamics of classes of barotropic fluids in spatially curved FRW spacetimes
• Tilted non-spatially-flat inflation
• Emergent universe: tensor perturbations within the CSL framework
• Emergent universe revisited through the CSL theory
• Bayesian analysis of running holographic Ricci dark energy
• Standardizing reverberation-measured Mg II time-lag quasars, by using the radius-luminosity relation, and constraining cosmological model parameters
• Beyond Fisher Forecasting for Cosmology
• Can Hubble tension be eased by invoking a finite range for gravity?
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• ParamANN: A Neural Network to Estimate Cosmological Parameters for $\Lambda$CDM Universe Using Hubble Measurements
• Dynamical analysis approaches in spatially curved FRW spacetimes
• Evidence against Ryskin's model of cosmic acceleration
• Revisiting the Hubble Tension with DESI DR2 Baryon Acoustic Oscillation Observations and Machine Learning Methods
• Yano-Schrödinger Hyperfluid: Cosmological Implications