Constraints on power law cosmology from cosmic chronometer, standard ruler, and standard candle data
arXiv:2102.08457 · doi:10.1088/1475-7516/2021/08/051
Abstract
In this paper I investigate how well simple power law expansion fits observational data in comparison to the standard CDM model. I analyze a data set consisting of cosmic chronometer, standard ruler, and standard candle measurements, finding that the CDM model provides a better fit to most combinations of these data than the power law ansatz.
arXiv comment18 pages, 2 figures. The previous version of this paper was rejected by Phys. Rev. D; this version has been accepted for publication in JCAP after some minor editorial changes
References in corpus (70)
- emcee: The MCMC Hammer
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- Constraints on the redshift dependence of the dark energy potential
- A 6% measurement of the Hubble parameter at : direct evidence of the epoch of cosmic re-acceleration
- Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
- Information criteria for astrophysical model selection
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers
- Cosmological implications of baryon acoustic oscillation (BAO) measurements
- Planck evidence for a closed Universe and a possible crisis for cosmology
- Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope
- Reconstruction of dark energy and expansion dynamics using Gaussian processes
- Curvature tension: evidence for a closed universe
- Measuring the cosmological parameters with the Ep,i-Eiso correlation of Gamma-Ray Bursts
- Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
- Distance measures in cosmology
- Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
- Extremely energetic Fermi Gamma-Ray Bursts obey spectral energy correlations
- 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
- Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
- Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey
- Observational constraints on Hubble constant and deceleration parameter in power-law cosmology
- Using the tilted flat-CDM and the untilted non-flat 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
- Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data
- The relation for massive bursts of star formation
- Observational constraints on the tilted spatially-flat and the untilted nonflat CDM dynamical dark energy inflation models
- Planck 2015 constraints on the non-flat CDM inflation model
- Fits, and especially linear fits, with errors on both axes, extra variance of the data points and other complications
- Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
- Strong evidence for an accelerating universe
- Constraining the Dark Energy Equation of State with HII Galaxies
- Constraints on cosmological parameters in power-law cosmology
- Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies
- Cosmological Constraints on a Power Law Universe
- Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
- Independent Cosmological Constraints from high-z HII Galaxies
- Planck 2015 constraints on the non-flat CDM inflation model
- Observational Constraints On Power-Law Cosmologies
- Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
- Robust model comparison disfavors power law cosmology
- Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
- Planck 2015 constraints on the non-flat XCDM inflation model
- Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
- Testing power-law cosmology with galaxy clusters
- Planck 2015 constraints on spatially-flat dynamical dark energy models
- Linear Coasting in Cosmology and SNe Ia
- Cosmological Tests for a Linear Coasting Cosmology
- Nucleosynthesis in Power-Law Cosmologies
- Power law cosmology model comparison with CMB scale information
- Power-law cosmology, SN Ia, and BAO
- The angular size - redshift relation in power-law cosmologies
- Observational constraints on phantom power-law cosmology
- Reaffirming the Cosmic Acceleration without Supernova and CMB
- Quintessential power-law cosmology: dark energy equation of state
- Probing dynamics of dark energy with latest observations
- Principal components of dark energy with SNLS supernovae: the effects of systematic errors
- Observational constraints on dark energy cosmological model parameters
- Power law cosmology - a viable alternative
- Constraints on Lepton Asymmetry from Nucleosynthesis in a Linearly Coasting Cosmology
- Scalar field power-law cosmology with spatial curvature and dark energy-dark matter interaction
- Nucleosynthesis in a Simmering Universe
- Tachyonic (phantom) power-law cosmology
- Observational constraints on running vacuum model
- On "Observational Constraints on Power-Law Cosmologies"
- Coulomb screening in linear coasting nucleosynthesis
- Nucleosynhthesis in a Simmering Universe
- The power-law expansion universe and dark energy evolution
- Evidence against Ryskin's model of cosmic acceleration
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- Testing spatial curvature and anisotropic expansion on top of the CDM model
- Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
- Revising the Hubble constant, spatial curvature and dark energy dynamics with the latest observations of quasars
- Testing Linearly Coasting Cosmology by Strong Lensing System and Pantheon+ Data