Current lookback time-redshift bounds on dark energy
arXiv:0901.2327 · doi:10.1016/j.physletb.2009.08.008
Abstract
We investigate observational constraints on dark energy models from lookback time (LT) estimates of 32 old passive galaxies distributed over the redshift interval . To build up our LT sample we combine the age measurements for these 32 objects with estimates of the total age of the Universe, as obtained from current CMB data. We show that LT data may provide bounds on the cosmological parameters with accuracy competitive with type Ia Supernova methods. In order to break possible degeneracies between models parameters, we also discuss the bounds when our lookback time versus redshift sample is combined with with the recent measurement of the baryonic acoustic oscillation peak and the derived age of the Universe from current CMB measurements.
6 pages, 4 figures, LaTex
References in corpus (68)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Cosmological Imprint of an Energy Component with General Equation of State
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- Cosmological Constant - the Weight of the Vacuum
- The Case for a Positive Cosmological Lambda-term
- The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
- Phantom Energy and Cosmic Doomsday
- Baryonic Features in the Matter Transfer Function
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Constraints on the redshift dependence of the dark energy potential
- Accelerated expansion of the universe driven by tachyonic matter
- Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters
- Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
- Galaxy Cluster Virial Masses and Omega
- Is There A Cosmological Constant?
- Cosmological constraints from the X-ray gas mass fraction in relaxed lensing clusters observed with Chandra
- The Gemini Deep Deep Survey: I. Introduction to the Survey, Catalogs and Composite Spectra
- Cosmological consequences of a Chaplygin gas dark energy
- The Fate of Bound Systems in Phantom and Quintessence Cosmologies
- Evolved Galaxies at z > 1.5 from the Gemini Deep Deep Survey: The Formation Epoch of Massive Stellar Systems
- The evolution of field early-type galaxies to z~0.7
- Chandra measurements of the distribution of mass in the luminous lensing cluster Abell 2390
- Testing dark energy beyond the cosmological constant barrier
- Constraints on Cosmological Parameters from the Analysis of the Cosmic Lens All Sky Survey Radio-Selected Gravitational Lens Statistics
- The Properties of Field Elliptical Galaxies at Intermediate Redshift. I: Empirical Scaling Laws
- The properties of field elliptical galaxies at intermediate redshift. II: photometry and spectroscopy of an HST selected sample
- Constraining the dark energy with galaxy clusters X-ray data
- Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
- Scalar-field-dominated cosmology with a transient accelerating phase
- Cardassian Expansion: Constraints from Compact Radio Source Angular Size versus Redshift Data
- Constraining the cosmic equation of state from old galaxies at high redshift
- Synthetic stellar populations: single stellar populations, stellar interior models and primordial proto-galaxies
- Cosmological constraints on Chaplygin gas dark energy from galaxy clusters X-ray and supernova data
- Some Observational Consequences of Brane World Cosmologies
- Cosmological Constraints from Compact Radio Source Angular Size versus Redshift Data
- Dark energy and the angular size - redshift diagram for milliarcsecond radio sources
- New limits on and from old galaxies at high redshift
- Lookback time as a test for brane cosmology
- An old quasar in a young dark energy-dominated universe?
- Dark Energy and Some Alternatives: a Brief Overview
- Constraining dark energy models using the lookback time to galaxy clusters and the age of the universe
- Constraining Omega_0 With The Angular-Size Redshift Relation Of Double-Lobed Quasars In The FIRST Survey
- Age of High Redshift Objects - a Litmus Test for the Dark Energy Models
- Brane World Cosmologies and Statistical Properties of Gravitational Lenses
- Energy Conditions and Segre Classification of Phantom Fields
- Radio Galaxy Redshift-Angular Size Data Constraints on Dark Energy
- Constraints on Scalar-Field Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift
- Constraints on Scalar-Field Dark Energy from the Cosmic Lens All-Sky Survey Gravitational Lens Statistics
- Cosmological implications of APM 08279+5255, an old quasar at z = 3.91
- Cosmological Constraints from Hubble Parameter on f(R) Cosmologies
- Cosmological constraints from lensing statistics and supernovae on the cosmic equation of state
- Constraints on Dark Energy from Galaxy Cluster Gas Mass Fraction versus Redshift data
- Testing power-law cosmology with galaxy clusters
- The ``angular size - redshift'' relation for compact radio structures in quasars and radio galaxies
- Dark energy and the epoch of galaxy formation
- Age constraints on the cosmic equation of state
- The Sun, stellar-population models, and the age estimation of high-redshift galaxies
- Determining the equation of state of dark energy from angular size of compact radio sources and X-ray gas mass fraction of galaxy clusters
- The angular size - redshift relation in power-law cosmologies
- Baryon Acoustic Oscillations and Dynamical Dark Energy
- Old Galaxies at High Redshift and the Cosmological Constant
- Gravitational lensing constraint on the cosmic equation of state
Cited by in corpus (11)
- Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
- Constraining cosmic curvature by using age of galaxies and gravitational lenses
- Dark Energy in Practice
- Constraints on dark energy from the lookback time versus redshift test
- Comparison of Recent SnIa datasets
- Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
- Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
- Time and distance constraints on accelerating cosmological models
- Testing the cosmic conservation of photon number with type Ia supernovae and ages of old objects
- Constraining scalar field dark energy with cosmological observations
- Analytical considerations about the cosmological constant and dark energy