Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially Flat ΛCDM Model, the Deceleration–Acceleration Transition Redshift, and Spatial Curvature
Abstract
We construct a complete collection of reliable Hubble parameter H(z) data to redshift z ≤ 2.36 and use them with the Gaussian Process approach to determine continuous H(z) functions for various data subsets. From these continuous H(z)'s, summarizing across the data subsets considered, we find H 0 ~ 67 ± 4 km s–1 Mpc–1, more consistent with the recent lower values observed using a variety of techniques. In most data subsets, we see a cosmological deceleration–acceleration transition at 2σ significance, with the data subsets transition redshifts varying over $$0.33\lt {z}_{\mathrm{da}}\lt 1.0$$ at 1σ significance. We discover that the flat-ΛCDM model is consistent with the H(z) data to a z of 1.5 to 2.0, depending on data subset considered, with 2σ deviations from flat-ΛCDM above this redshift range. Using the continuous H(z) with baryon acoustic oscillation distance-redshift observations, we constrain the current spatial curvature density parameter to be $${{\rm{\Omega }}}_{K0}=-0.03\pm 0.21$$, consistent with a flat universe, but the large error bar does not rule out small values of spatial curvature that are now under debate.
- Authors:
-
- Nanjing Univ. (China); Kansas State Univ., Manhattan, KS (United States)
- Kansas State Univ., Manhattan, KS (United States)
- Nanjing Univ. (China)
- Publication Date:
- Research Org.:
- Kansas State Univ., Manhattan, KS (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Basic Research Program of China; National Natural Science Foundation of China (NSFC); China Scholarship Council
- OSTI Identifier:
- 1542020
- Grant/Contract Number:
- SC0011840
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 856; Journal Issue: 1; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; cosmological parameters; cosmology: observations; large-scale structure of universe
Citation Formats
Yu, Hai, Ratra, Bharat, and Wang, Fa-Yin. Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially Flat ΛCDM Model, the Deceleration–Acceleration Transition Redshift, and Spatial Curvature. United States: N. p., 2018.
Web. doi:10.3847/1538-4357/aab0a2.
Yu, Hai, Ratra, Bharat, & Wang, Fa-Yin. Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially Flat ΛCDM Model, the Deceleration–Acceleration Transition Redshift, and Spatial Curvature. United States. https://doi.org/10.3847/1538-4357/aab0a2
Yu, Hai, Ratra, Bharat, and Wang, Fa-Yin. Tue .
"Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially Flat ΛCDM Model, the Deceleration–Acceleration Transition Redshift, and Spatial Curvature". United States. https://doi.org/10.3847/1538-4357/aab0a2. https://www.osti.gov/servlets/purl/1542020.
@article{osti_1542020,
title = {Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially Flat ΛCDM Model, the Deceleration–Acceleration Transition Redshift, and Spatial Curvature},
author = {Yu, Hai and Ratra, Bharat and Wang, Fa-Yin},
abstractNote = {We construct a complete collection of reliable Hubble parameter H(z) data to redshift z ≤ 2.36 and use them with the Gaussian Process approach to determine continuous H(z) functions for various data subsets. From these continuous H(z)'s, summarizing across the data subsets considered, we find H 0 ~ 67 ± 4 km s–1 Mpc–1, more consistent with the recent lower values observed using a variety of techniques. In most data subsets, we see a cosmological deceleration–acceleration transition at 2σ significance, with the data subsets transition redshifts varying over $0.33\lt {z}_{\mathrm{da}}\lt 1.0$ at 1σ significance. We discover that the flat-ΛCDM model is consistent with the H(z) data to a z of 1.5 to 2.0, depending on data subset considered, with 2σ deviations from flat-ΛCDM above this redshift range. Using the continuous H(z) with baryon acoustic oscillation distance-redshift observations, we constrain the current spatial curvature density parameter to be ${{\rm{\Omega }}}_{K0}=-0.03\pm 0.21$, consistent with a flat universe, but the large error bar does not rule out small values of spatial curvature that are now under debate.},
doi = {10.3847/1538-4357/aab0a2},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 856,
place = {United States},
year = {Tue Mar 20 00:00:00 EDT 2018},
month = {Tue Mar 20 00:00:00 EDT 2018}
}
Web of Science
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An improved model-independent assessment of the late-time cosmic expansion
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Model-independent reconstruction of the linear anisotropic stress η
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Holographic dark energy through Tsallis entropy
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Dark energy and dark matter unification from dynamical space time: observational constraints and cosmological implications
journal, June 2019
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Most Frequent Value Statistics and the Hubble Constant
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
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Possible signals of vacuum dynamics in the Universe
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Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data
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Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
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General cosmography model with spatial curvature
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Observational constraints on sign-changeable interaction models and alleviation of the tension
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Consistency of the expansion of the Universe with density perturbations
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Current constraints on anisotropic and isotropic dark energy models
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Planck 2015 Constraints on the Non-flat ΛCDM Inflation Model
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Planck 2015 Constraints on the Nonflat ϕ CDM Inflation Model
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The H 0 Tension in Non-flat QCDM Cosmology
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Model-independent Curvature Determination from Gravitational-wave Standard Sirens and Cosmic Chronometers
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Planck 2015 Constraints on the Non-flat XCDM Inflation Model
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Are H 0 and σ 8 Tensions Generic to Present Cosmological Data?
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Flatness without CMB: The Entanglement of Spatial Curvature and Dark Energy Equation of State
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Using the Tilted flat-ΛCDM and the Untilted Non-flat ΛCDM Inflation Models to Measure Cosmological Parameters from a Compilation of Observational Data
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Model-independent Distance Calibration and Curvature Measurement Using Quasars and Cosmic Chronometers
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Reconstructing Functions and Estimating Parameters with Artificial Neural Networks: A Test with a Hubble Parameter and SNe Ia
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Planck 2015 constraints on spatially-flat dynamical dark energy models
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Magnetogenesis in cyclical Universe
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First study of reionization in the Planck 2015 normalized closed ΛCDM inflation model
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First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
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Modified cosmology from extended entropy with varying exponent
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CMB Tensions with Low-Redshift H0 and S8 Measurements: Impact of a Redshift-Dependent Type-Ia Supernovae Intrinsic Luminosity
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Possible signals of vacuum dynamics in the Universe
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Planck 2015 constraints on the non-flat XCDM inflation model
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$H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
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- arXiv
Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
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Modified cosmology from extended entropy with varying exponent
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CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
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Reconstructing Functions and Estimating Parameters with Artificial Neural Networks: A Test with the Hubble Parameter and SNe Ia
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Observational constraints on Myrzakulov gravity
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Decaying Dark Energy in Light of the Latest Cosmological Dataset
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A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters Over Time
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Role of a periodic varying deceleration parameter in Particle creation with higher dimensional FLRW Universe
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