Constraints on dark energy from the lookback time versus redshift test

Abstract

We use lookback time versus redshift data from galaxy clusters (Capozziello et al., 2004) and passively evolving galaxies (Simon et al., 2005), and apply a bayesian prior on the total age of the Universe based on WMAP measurements, to constrain dark energy cosmological model parameters. Current lookback time data provide interesting and moderately restrictive constraints on cosmological parameters. When used jointly with current baryon acoustic peak and Type Ia supernovae apparent magnitude versus redshift data, lookback time data tighten the constraints on parameters and favor slightly smaller values of the nonrelativistic matter energy density.

Physics Letters B in press. 15 pages, 6 figures, 1 table. Minor typos fixed

References in corpus (32)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
• Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder
• The cluster gas mass fraction as a cosmological probe: a revised study
• Thermodynamics in $F(R)$ gravity with phantom crossing
• Age Problem in the Holographic Dark Energy Model
• Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
• The Beginning and Evolution of the Universe
• Model-Independent Distance Measurements from Gamma-Ray Bursts and Constraints on Dark Energy
• Lookback time as a test for brane cosmology
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• Constraining dark energy with gamma-ray bursts
• Reconstructing the Cosmic Expansion History up to Redshift z=6.29 with the Calibrated Gamma-Ray Bursts
• Bayesian Analysis and Constraints on Kinematic Models from Union SNIa
• Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy
• Non-minimally coupled scalar field cosmology on the phase plane
• Age constraints on the cosmic equation of state
• Constraints on $w_0$ and $w_a$ of Dark Energy from High Redshift Gamma Ray Bursts
• Clustering, Angular Size and Dark Energy
• Cosmological Studies with Radio Galaxies and Supernovae
• Cosmology-Independent Distance Moduli of 42 Gamma-Ray Bursts between Redshift of 1.44 and 6.60
• Clarifying Forecasts of Dark Energy Constraints from Baryon Acoustic Oscillations
• Gamma-ray burst contributions to constraining the evolution of dark energy
• Galaxy Cluster Gas Mass Fraction and Hubble Parameter versus Redshift Constraints on Dark Energy
• Constraints on dark energy from baryon acoustic peak and galaxy cluster gas mass measurements
• Cosmological constraints on unifying Dark Fluid models
• Power law cosmology - a viable alternative
• Current lookback time-redshift bounds on dark energy
• Prospects in Constraining the Dark Energy Potential

Cited by in corpus (34)

• Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
• Median statistics and the Hubble constant
• CDM Accelerating Cosmology as an Alternative to LCDM model
• Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• 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
• 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
• Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data
• Constraining cosmic curvature by using age of galaxies and gravitational lenses
• Dark Energy in Practice
• Hubble parameter data constraints on dark energy
• Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
• Inflation in a closed universe
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Constraints on dark energy from H II starburst galaxy apparent magnitude versus redshift data
• Transition Redshift: New constraints from parametric and nonparametric methods
• Galaxy cluster number count data constraints on cosmological parameters
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
• Luminous Red Galaxies in Simulations: Cosmic Chronometers?
• Observational Constraints on Dynamical Dark Energy Models
• Galaxy cluster angular size data constraints on dark energy
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• On the use of galaxies as clocks and the universal expansion
• Constraints on dark energy from the Lyα forest baryon acoustic oscillations measurement of the redshift 2.3 Hubble parameter
• Time and distance constraints on accelerating cosmological models
• Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample
• Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
• Constraining scalar field dark energy with cosmological observations
• Lookback time and Chandra constrains on cosmological parameters