Expected constraints on the generalized Chaplygin equation of state from future supernova experiments and gravitational lensing statistics
arXiv:astro-ph/0303353 · doi:10.1086/379362
Abstract
This paper aims to study the use of future SNAP data together with the result of searches for strong gravitational lenses in future large quasar surveys to constrain the Generalized Chaplygin Gas (GCG) model. The GCG is considered as a possible unification scheme for dark matter-dark energy. It is found that both experiments should be able to place important constraints on the model, especially when both tests are used together.
Submitted to the Astrophysical Journal, 33 pages, 8 Figures, uses aastex.cls. Changed for publication. Sections where the GCG is used as a dark energy candidate have been eliminated, plus minor changes
References in corpus (54)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- An alternative to quintessence
- A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
- Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
- Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
- Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?
- Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
- Cosmology with a Primordial Scaling Field
- Supernova Limits on the Cosmic Equation of State
- A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
- Scaling solutions in general non-minimal coupling theories
- Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations
- Big-Bang Nucleosynthesis Predictions for Precision Cosmology
- Cosmological scaling solutions of non-minimally coupled scalar fields
- Is There A Cosmological Constant?
- The Most Massive Distant Clusters: Determining Omega and sigma_8
- Nonminimal coupling and quintessence
- Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
- Phenomenology of a realistic accelerating universe using only Planck-scale physics
- Future Supernovae observations as a probe of dark energy
- Generalized Chaplygin gas and CMBR constraints
- Constraints on the generalized Chaplygin gas from supernovae observations
- The CANADA-FRANCE REDSHIFT SURVEY I: Introduction to the Survey, Photometric Catalogs and Surface Brightness Selection Effects
- Cosmic acceleration without quintessence
- Evolution of the Galaxy Population Based on Photometric Redshifts in the Hubble Deep Field
- Cosmological consequences of a Chaplygin gas dark energy
- Models of dynamical supersymmetry breaking and quintessence
- Gravitational Lensing as a Probe of Quintessence
- Limits on Cosmological Models From Radio-Selected Gravitational Lenses
- Cosmological constraints from Archeops
- High-redshift objects and the generalized Chaplygin gas
- Supernovae and the Nature of the Dark Energy
- SUSY QCD and Quintessence
- Cosmological Constraints on an Invisibly Decaying Higgs Boson
- The Redshift Distribution and Luminosity Functions of Galaxies in the Hubble Deep Field
- A Quintessence Scalar Field in Brans-Dicke Theory
- New limits on a cosmological constant from statistics of gravitational lensing
- Alternatives to Quintessence Model Building
- Dark Matter and Energy in the Universe
- The nature of the faint galaxies in the Hubble Deep Field
- The Role of Baryons in Unified Dark Matter Models
- A Two-Field Quintessence Model
- Dissipative Fluid in Brans Dicke theory and late time acceleration
- Cosmology in scalar tensor theory and asymptotically de-Sitter Universe
- Axion and Almost Massless Quark as Ingredients of Quintessence
- Galaxy Mergers and Gravitational Lens Statistics
- Compactification, Vacuum Energy and Quintessence
- Through a Lens Darkly: Evidence for Dusty Gravitational Lenses
- A two-scalar model for a small but nonzero cosmological constant
- A Lower Limit on Omega-Lambda Using Gravitational Lensing in the Hubble Deep Field
- Fitting BOOMERANG and MAXIMA-1 data with a Einstein-Yang-Mills Cosmological Model
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- Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
- A parametric model for dark energy
- A comparison of cosmological models using recent supernova data
- The Revival of the Unified Dark Energy-Dark Matter Model ?
- Latest Supernova data in the framework of Generalized Chaplygin Gas model
- Chaplygin traversable wormholes
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: observational constraints
- Cosmological coincidence problem in interacting dark energy models
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- CDM Accelerating Cosmology as an Alternative to LCDM model
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- Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
- Constraints on Chaplygin quartessence from the CLASS gravitational lens statistics and supernova data
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- Probing the cosmographic parameters to distinguish between dark energy and modified gravity models
- Modified Chaplygin Gas and Constraints on its B parameter from CDM and UDME Cosmological models
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- Observational constraints on cosmology from modified Friedmann equation
- Observational constraints on late-time Lambda(t) cosmology
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- WMAP5 constraints on the unified model of dark energy and dark matter
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- Cosmic Equation of state from Strong Gravitational Lensing Systems
- Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations
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- Latest supernovae constraints on f(R) cosmologies
- Generalized Chaplygin Gas in a modified gravity approach
- Accelerating universe from gravitational leakage into extra dimensions: confrontation with SNeIa
- Chaplygin inspired Inflation
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- Constraints on Scalar-Field Dark Energy from the Cosmic Lens All-Sky Survey Gravitational Lens Statistics
- Large-scale inhomogeneities in modified Chaplygin gas cosmologies
- Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach
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- Constraints on the generalized Chaplygin gas model including gamma-ray bursts via a Markov Chain Monte Carlo approach
- Generalized Chaplygin gas model, supernovae and cosmic topology
- Constraints on Cardassian Scenario from the Expansion Turnaround Redshift and the Sunyaev-Zeldovich/X-ray Data
- Viscous dissipative Chaplygin gas dominated homogenous and isotropic cosmological models
- Cosmological constraints on generalized Chaplygin gas model: Markov Chain Monte Carlo approach
- Observational constraints on a unified dark matter and dark energy model based on generalized Chaplygin gas
- Chemical Potential and the Nature of the Dark Energy: The case of phantom
- Coupled quintessence and vacuum decay
- Measuring the Chaplygin gas equation of state from angular and luminosity distances
- Dynamics of perfect fluid Unified Dark Energy models
- Testing the DGP model with gravitational lensing statistics
- Perturbative approach for mass varying neutrinos coupled to the dark sector in the generalized Chaplygin gas scenario
- Stationary condition in a perturbative approach for mass varying neutrinos
- Bayesian Statistics and Parameter Constraints on the Generalized Chaplygin Gas Model using SNe Ia Data
- The Deformable Universe
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- Remarks on the Generalized Chaplygin Gas
- Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
- Instability of Chaplygin gas trajectories in unified dark matter models
- Constraining the dark energy and smoothness-parameter with supernovae
- A Curvature Principle for the interaction between universes
- Time and distance constraints on accelerating cosmological models
- GCG Parametrization for Growth Function and Current Constraints
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- Observational constraints of the gravitational waves in the Brans-Dicke theory: Einstein frame and Jordan-Brans-Dicke frame
- Accretion of non-minimally coupled generalized Chaplygin gas into black holes
- Observational Constraints on Modified Chaplygin Gas in Horava-Lifshitz Gravity
- Constraints on the generalized tachyon field models from latest observational data
- New parameterization for unified dark matter and dark energy
- Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
- Quintessence as k-essence
- Coupling dark energy with Standard Model states
- A Modified Generalized Chaplygin Gas as the Unified Dark Matter-Dark Energy Revisited
- Observational constraints on the time-dependence of dark energy
- FRW type of cosmology with a Chaplygin gas
- A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
- Perspectives in Fundamental Physics in Space
- Dark Energy, Dark Matter and Gravity
- The Hamiltonian formalism for scalar fields coupled to gravity in a cosmological background
- Mass varying dark matter in effective GCG scenarios
- Cosmic constraint on the unified model of dark sectors with or without a cosmic string fluid in the varying gravitational constant theory
- Constraints on the unified dark energy-dark matter model from latest observational data
- Naturalness and stability of the generalized Chaplygin gas in the seesaw cosmon scenario
- New parameterizations of generalized Chaplygin gas model constrained at background and perturbation levels
- The electromagnetic coupling and the dark side of the Universe
- Dynamical friction shear and rotation in Chaplygin cosmology