Future supernovae data and quintessence models
arXiv:astro-ph/0207332 · doi:10.1046/j.1365-8711.2003.06508.x
Abstract
The possibility to unambiguously determine the equation-of-state of the cosmic dark energy with existing and future supernovae data is investigated. We consider four evolution laws for this equation-of-state corresponding to four quintessential models, i.e. i) a cosmological constant, ii) a general barotropic fluid, iii) a perfect fluid with a linear equation-of-state and iv) a more physical model based on a pseudo-Nambu-Goldstone boson field. We explicitly show the degeneracies present not only within each model but also between the different models : they are caused by the multi-integral relation between the equation-of-state of dark energy and the luminosity distance. Present supernova observations are analysed using a standard method and the minimal values obtained for each model are compared. We confirm the difficulty to discriminate between these models using present SNeIa data only. By means of simulations, we then show that future SNAP observations will not remove all the degeneracies. For example, wrong estimations of with a good value of could be found if the right cosmological model is not used to fit the data. We finally give some probabilities to obtain unambiguous results, free from degeneracies. In particular, the probability to confuse a cosmological constant with a true barotropic fluid with an equation-of-state different from -1 is shown to be 95% at a level.
12 pages. This improved version has been accepted for publication in M.N.R.A.S
References in corpus (8)
- Cosmology and the Fate of Dilatation Symmetry
- Probing the dark energy: methods and strategies
- Future Supernovae observations as a probe of dark energy
- Measuring the Equation-of-state of the Universe: Pitfalls and Prospects
- Probing quintessence: reconstruction and parameter estimation from supernovae
- Supernovae and the Nature of the Dark Energy
- Current constraints on the dark energy equation of state
- Future supernova probes of quintessence
Cited by in corpus (143)
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Dark Energy
- Comparison of the Legacy and Gold SnIa Dataset Constraints on Dark Energy Models
- A comparison of cosmological models using recent supernova data
- Constraints on linear-negative potentials in quintessence and phantom models from recent supernova data
- Cosmographic analysis of the equation of state of the universe through Padé approximations
- Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
- Cosmological Constraints on New Agegraphic Dark Energy
- General Cosmography Model with Spatial Curvature
- Exploring Cosmological Expansion Parametrizations with the Gold SnIa Dataset
- Observational Constraints on Cosmological Models with the Updated Long Gamma-Ray Bursts
- Constraints on cosmological models from strong gravitational lensing systems
- Noether Symmetry in Theory
- Modified gravity a la Galileon: Late time cosmic acceleration and observational constraints
- Probing for dynamics of dark energy and curvature of universe with latest cosmological observations
- Observing Dark Energy Dynamics with Supernova, Microwave Background and Galaxy Clustering
- Observational constraints on holographic dark energy with varying gravitational constant
- Constraint on Coupled Dark Energy Models from Observations
- Constraints on the Sound Speed of Dynamical Dark Energy
- High-Redshift Cosmography
- Constraints on kinematic models from the latest observational data
- Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
- Cosmological Constraints on the Sign-Changeable Interactions
- Cosmological Applications of Pade Approximant
- The growth of matter perturbations in some scalar-tensor DE models
- Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
- Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum
- Theoretical Limits on the Equation-of-State Parameter of Phantom Cosmology
- Pilgrim Dark Energy
- Gamma-ray bursts as dark energy-matter probes in the context of the generalized Chaplygin gas model
- Cosmography: Supernovae Union2, Baryon Acoustic Oscillation, Observational Hubble Data and Gamma Ray Bursts
- Constraints on Primordial Non-Gaussianity from Large Scale Structure Probes
- Constraining Primordial Non-Gaussianity with High-Redshift Probes
- Testing the phenomenological interacting dark energy with observational data
- Cosmography beyond standard candles and rulers
- Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
- Observational constraint on generalized Chaplygin gas model
- Overcoming the Circular Problem for γ-ray Bursts in Cosmological Global Fitting Analysis
- Cosmological Constraints on the Modified Entropic Force Model
- Observational constraints on the interacting Ricci dark energy model
- The High Redshift Integrated Sachs-Wolfe Effect
- Holographic f(T)-gravity model with power-law entropy correction
- Holographic Dark Energy Model with Hubble Horizon as an IR Cut-off
- Generalized Holographic and Ricci Dark Energy Models
- Accelerating cosmologies tested by distance measures
- Constraining gravity models using type Ia supernovae
- Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach
- Determining Cosmological Parameters with Latest Observational Data
- Cosmological constraints combining H(z), CMB shift and SNIa observational data
- Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
- Late-Time constraints on Interacting Dark Energy: Analysis independent of , and
- Constraints on Kinematic Model from Recent Cosmic Observations: SN Ia, BAO and Observational Hubble Data
- Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
- Early Dark Energy at High Redshifts: Status and Perspectives
- Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?
- Modified Holographic Dark Energy
- Tension in the Recent Type Ia Supernovae Datasets
- Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
- Combined cosmological and solar system constraints on chameleon mechanism
- Constraining dynamical dark energy with a divergence-free parametrization in the presence of spatial curvature and massive neutrinos
- Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of
- Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
- QCD ghost f(T)-gravity model
- Quasi-Rip: A New Type of Rip Model without Cosmic Doomsday
- Constraints on extended quintessence from high-redshift Supernovae
- Dynamics of holographic vacuum energy in the DGP model
- Constraints on Dark Energy Models Including Gamma Ray Bursts
- Cosmic Constraint to DGP Brane Model: Geometrical and Dynamical Perspectives
- Probing the dynamics of dark energy with divergence-free parametrizations: A global fit study
- Multiple kinetic k-essence, phantom barrier crossing and stability
- Constraining DGP Gravity from Observational Data
- New Generalizations of Cosmography Inspired by the Pade Approximant
- Observational constraint on the varying speed of light theory
- Probing Inflation and Dark Energy with Current Cosmological Observations
- Background cosmological dynamics in gravity and observational constraints
- Observational constraint on the interacting dark energy models including the Sandage-Loeb test
- Cosmological Constraints on Variable Warm Dark Matter
- Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
- Dark-Energy Dynamics Required to Solve the Cosmic Coincidence
- Tracing the cosmic history by Gauss-Bonnet gravity
- Observational Constraints on Interacting Dark Matter Model Without Dark Energy
- Cosmological Models and Latest Observational Data
- Galaxy cluster angular size data constraints on dark energy
- Cosmological Constant, Fine Structure Constant and Beyond
- Quintom evolution in power-law potentials
- Reconstructing the History of Energy Condition Violation from Observational Data
- Probing for the Cosmological Parameters with PLANCK Measurement
- Constraining Cosmological Parameters with Observational Data Including Weak Lensing Effects
- Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
- Does accelerating universe indicates Brans-Dicke theory
- Constraints on the cosmic equation of state: age conflict versus phantom energy. Age-redshift relations in an accelerated universe
- Theoretic Limits on the Equation of State Parameter of Quintessence
- Tension between SN and BAO: current status and future forecasts
- Spatial Ricci scalar dark energy model
- Confronting Tracker Field Quintessence with Data
- Constraints on the exponential model from latest Hubble parameter measurements
- Cosmological constraints on the generalized holographic dark energy
- Probing Dark Energy with Supernovae : Bias from the time evolution of the equation of state
- Cosmological constraints on polytropic gas model
- Constraints from the CMB temperature and other common observational data-sets on variable dark energy density models
- Constraints on Dark Energy Parameters from Correlations of CMB with LSS
- Constraints on the generalized tachyon field models from latest observational data
- Cosmological neutrino mass limit and the dynamics of dark energy
- Improving Dark Energy Constraints with High Redshift Type Ia Supernovae from CANDELS and CLASH
- Cosmological constraints on holographic dark energy models under the energy conditions
- Transient acceleration in gravity
- DE models with combined from BAO and CMB dataset and friends
- Observational Constraints on the Generalized Chaplygin Gas
- Probing for variation of neutrino mass with current observations
- Dark Energy Cosmology with the Alternative Cosmic Microwave Background Data
- Consistency of nonlinear interacting ghost dark energy with recent observations
- Constraints on Models with a Break in the Primordial Power Spectrum
- Relaxing the Cosmological Constraints on Unparticle Dark Component
- Decaying dark energy in light of the latest cosmological dataset
- Scale dependence of the primordial spectrum from combining the three-year WMAP, Galaxy Clustering, Supernovae, and Lyman-alpha forests
- First cosmological constraints on the Superfluid Chaplygin gas model
- The interacting generalized Ricci dark energy model in non-flat universe
- Observational constraints on electromagnetic Born-Infeld cosmology
- Observational constraints from SNe Ia and Gamma-Ray Bursts on a clumpy universe
- Observational Constraints on Varying Alpha in CDM Cosmology
- Effect of low anisotropy on cosmological models by using supernova data
- Impact of Cosmology on Lorentz Invariance Violation Constraints from GRB Time-Delays
- Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
- Flat Cosmology with Coupled Matter and Dark Energies
- Unbiased constraints on the clumpiness of universe from standard candles
- Interacting dark energy collapse with matter components separation
- Impacts on Cosmological Constraints from Degeneracies
- Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
- Cosmological Model-independent Gamma-ray Bursts Calibration and its Cosmological Constraint to Dark Energy
- Observational constraints on the unified dark matter and dark energy model based on the quark bag model
- Time Variable Cosmological Constant from Renormalization Group Equations
- Large-scale structure and the Cardassian fluid
- Probing for cosmological parameters with LAMOST measurement
- Cosmic constraint on the unified model of dark sectors with or without a cosmic string fluid in the varying gravitational constant theory
- Cosmological Study in Myrzakulov Quasi-dilaton Massive Gravity
- Testing Dvali-Gabadadze-Porrati Gravity with Planck
- The torsion cosmology in Kaluza-Klein theory
- Testing the Consistence of Gamma Ray Burst Data-set and Supernovae Union2
- Cosmology of fermionic dark energy coupled to curvature
- Probing for Lorentz Invariance Violation in Pantheon Plus Dominated Cosmology
- Cosmology of Quasi-Dilaton Massive Gravity with Non-minimal Kinetic Coupling
- Cosmological aspects of cubic Galileon massive gravity