Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature

Abstract

We compile an updated list of 38 measurements of the Hubble parameter $H(z)$ between redshifts $0.07\le z\le 2.36$ and use them to place constraints on model parameters of constant and time-varying dark energy cosmological models, both spatially flat and curved. We use five models to measure the redshift of the cosmological deceleration-acceleration transition, $z_{\mathrm{da}}$, from these $H(z)$ data. Within the error bars, the measured $z_{\mathrm{da}}$ are insensitive to the model used, depending only on the value assumed for the Hubble constant $H_0$. The weighted mean of our measurements is $z_{\mathrm{da}}=0.72\pm 0.05(0.84\pm 0.03)$ for $H_0=68\pm 2.8(73.24\pm 1.74)$ km s${}^{-1}$ Mpc${}^{-1}$ and should provide a reasonably model-independent estimate of this cosmological parameter. The $H(z)$ data are consistent with the standard spatially-flat $\Lambda$CDM cosmological model but do not rule out non-flat models or dynamical dark energy models.

arXiv comment7 Tables and 4 Figures, ApJ, in press

References in corpus (72)

• Planck 2015 results. XIII. Cosmological parameters
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• 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 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3
• Observational Probes of Cosmic Acceleration
• Constraints on the redshift dependence of the dark energy potential
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
• Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2
• Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers
• The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1
• Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
• Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
• Cosmological implications of baryon acoustic oscillation (BAO) measurements
• Baryon Acoustic Oscillations in the Ly-α forest of BOSS quasars
• Quasar-Lyman $\alpha$ Forest Cross-Correlation from BOSS DR11 : Baryon Acoustic Oscillations
• Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant
• Dark Energy vs. Modified Gravity
• Hubble parameter measurement constraints on the cosmological deceleration-acceleration transition redshift
• The Atacama Cosmology Telescope: Cosmological parameters from three seasons of data
• Modeling the Anisotropic Two-Point Galaxy Correlation Function on Small Scales and Improved Measurements of H(z), D_A(z), and f(z)sigma_8(z) from the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
• H0 Revisited
• Cosmographic analysis of the equation of state of the universe through Padé approximations
• Median Statistics, H_0, and the Accelerating Universe
• Quantifying discordance in the 2015 Planck CMB spectrum
• Cosmographic bounds on the cosmological deceleration-acceleration transition redshift in $f(\mathcal{R})$ gravity
• Cosmological Constraints from Hubble Parameter versus Redshift Data
• Median statistics and the Hubble constant
• New observational constraints on f(T) gravity from cosmic chronometers
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• The Beginning and Evolution of the Universe
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• Binned Cosmic Microwave Background Anisotropy Power Spectra: Peak Location
• Binned Hubble parameter measurements and the cosmological deceleration-acceleration transition
• Probing kinematics and fate of the Universe with linearly time-varying deceleration parameter
• New Model-independent Method to Test the Curvature of the Universe
• Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations
• Test of the cosmic evolution using Gaussian processes
• Hubble parameter data constraints on dark energy
• Nonflat time-variable dark energy cosmology
• Constraining dark energy with gamma-ray bursts
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• A parametric reconstruction of the cosmological jerk from diverse observational data sets
• Constraints on Scalar-Field Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift
• Median Statistics and the Mass Density of the Universe
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• Forecasting cosmological parameter constraints from near-future space-based galaxy surveys
• On the luminosity distance and the epoch of acceleration
• Redshift drift test of exotic singularity universes
• Reconstructing thawing quintessence with multiple datasets

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