Direct evidence of acceleration from distance modulus redshift graph
arXiv:astro-ph/0703583 · doi:10.1088/1475-7516/2007/08/018
Abstract
The energy conditions give upper bounds on the luminosity distance. We apply these upper bounds to the 192 essence supernova Ia data to show that the Universe had experienced accelerated expansion. This conclusion is drawn directly from the distance modulus-reshift graph. In addition to be a very simple method, this method is also totally independent of any cosmological model. From the degeneracy of the distance modulus at low redshift, we argue that the choice of for probing the property of dark energy is misleading. One explicit example is used to support this argument.
use revtex,8 figures, JCAP in press, section 2 is re-organized. add more discussions on the dark energy parametrization
References in corpus (60)
- 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
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Cosmological Constant - the Weight of the Vacuum
- The Case for a Positive Cosmological Lambda-term
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
- Reconstructing Dark Energy
- Probing the dark energy: methods and strategies
- Is there Supernova Evidence for Dark Energy Metamorphosis ?
- WMAP constraints on low redshift evolution of dark energy
- The case for dynamical dark energy revisited
- Uncorrelated Estimates of Dark Energy Evolution
- Comparison of the Legacy and Gold SnIa Dataset Constraints on Dark Energy Models
- Crossing the Phantom Divide: Theoretical Implications and Observational Status
- Future Supernovae observations as a probe of dark energy
- Parameterization of Dark-Energy Properties: a Principal-Component Approach
- Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and Three-Year Wilkinson Microwave Anisotropy Probe Observations
- Cosmological parameters from supernova observations: A critical comparison of three data sets
- Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background Anisotropies
- New dark energy constraints from supernovae, microwave background and galaxy clustering
- Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
- Phenomenological parameterization of quintessence
- Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
- A Model-Independent Determination of the Expansion and Acceleration Rates of the Universe as a Function of Redshift and Constraints on Dark Energy
- Reconstruction of the deceleration parameter and the equation of state of dark energy
- Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data
- General Relativistic Energy Conditions: The Hubble expansion in the epoch of galaxy formation
- A model independent approach to the dark energy equation of state
- Opportunities for future supernova studies of cosmic acceleration
- Direct Determination of the Kinematics of the Universe and Properties of the Dark Energy as Functions of Redshift
- What Do We Really Know About Cosmic Acceleration?
- Probing quintessence: reconstruction and parameter estimation from supernovae
- Can luminosity distance measurements probe the equation of state of dark energy
- Energy Conditions and Cosmic Acceleration
- Probing the curvature and dark energy
- Model independent analysis of dark energy I: Supernova fitting result
- Tension and Systematics in the Gold06 SnIa Dataset
- Exploring the Properties of Dark Energy Using Type Ia Supernovae and Other Datasets
- Observational constraints on the acceleration of the Universe
- Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
- Unified dark energy models : a phenomenological approach
- Energy conditions and current acceleration of the universe
- Importance of Supernovae at z>1.5 to Probe Dark Energy
- Energy Conditions and Supernovae Observations
- On the determination of the deceleration parameter from Supernovae data
- Dark Energy Evolution and the Curvature of the Universe from Recent Observations
- Probing the curvature of the Universe from supernova measurement
- Accelerating cosmologies tested by distance measures
- No evidence for Dark Energy Metamorphosis ?
- Dark Energy Parametrizations and the Curvature of the Universe
- Observational constraints on dark energy model
- Toward reconstruction of dynamics of the Universe from distant supernovae type Ia
- Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha
- Particle-Like Description in Quintessential Cosmology
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