Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models

Abstract

We perform a detailed comparison of the Wilkinson Microwave Anisotropy Probe (WMAP) measurements of the cosmic microwave background (CMB) temperature and polarization anisotropy with the predictions of quintessence cosmological models of dark energy. We consider a wide range of quintessence models, including: a constant equation-of-state; a simply-parametrized, time-evolving equation-of-state; a class of models of early quintessence; scalar fields with an inverse-power law potential. We also provide a joint fit to the CBI and ACBAR CMB data, and the type 1a supernovae. Using these select constraints we identify viable, target models for further analysis.

6 pages, 9 color figures, latex

References in corpus (44)

• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Cosmological Imprint of an Energy Component with General Equation of State
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• Exploring the Expansion History of the Universe
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• Cosmological Results from High-z Supernovae
• Cosmological Tracking Solutions
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
• CDM Models with a Smooth Component
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology
• The Microwave Anisotropy Probe (MAP) Mission
• Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB
• Big-Bang Nucleosynthesis Predictions for Precision Cosmology
• Cosmic Concordance and Quintessence
• High Resolution Observations of the CMB Power Spectrum with ACBAR
• The Anisotropy of the Microwave Background to l = 3500: Deep Field Observations with the Cosmic Background Imager
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks
• The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager
• Tracking and coupled dark energy as seen by WMAP
• Dynamical Lambda Models of Structure Formation
• Probing the dark side: Constraints on the dark energy equation of state from CMB, large scale structure and Type Ia supernovae
• A model independent approach to the dark energy equation of state
• Measuring the Speed of Sound of Quintessence
• II: Bayesian Methods for Cosmological Parameter Estimation from Cosmic Microwave Background Measurements
• Resolving the Cosmological Missing Energy Problem
• Exhaustive Study of Cosmic Microwave Background Anisotropies in Quintessential Scenarios
• Current constraints on the dark energy equation of state
• Effects of the Sound Speed of Quintessence on the Microwave Background and Large Scale Structure
• SUSY QCD and Quintessence
• Observational Constraints on General Relativistic Energy Conditions, Cosmic Matter Density and Dark Energy from X-Ray Clusters of Galaxies and Type-Ia Supernovae
• Constraining the quintessence equation of state with SnIa data and CMB peaks
• Early Quintessence in Light of WMAP
• Natural Quintessence?
• Constraints on flat cosmologies with tracking Quintessence from Cosmic Microwave Background observations
• Condensate cosmology -- dark energy from dark matter
• Implications for quintessence models from MAXIMA-1 and BOOMERANG-98
• Constraining Quintessence with the New CMB Data
• WMAP Constraints on Quintessence

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• Energy conditions in $f(Q,L_m)$ gravity
• Cosmological Model-independent Gamma-ray Bursts Calibration and its Cosmological Constraint to Dark Energy
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• Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
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