Probing for dynamics of dark energy and curvature of universe with latest cosmological observations

Abstract

We use the newly released 182 Type Ia supernova data combined with the third-year Wilkinson Microwave Anisotropic Probe data (WMAP3) and large scale structure (LSS) information including SDSS and 2dFGRS to constrain the dark energy equation of state (EoS) as well as the curvature of universe ${\Omega }_K$. Using the full dataset of Cosmic Microwave Background (CMB) and LSS rather than the shift parameter and linear growth factor, we make a Markov Chain Monte Carlo (MCMC) global fit, while paying particular attention to the dark energy perturbation. Parameterizing the EoS as $w_{DE}(a)=w_0+w_1(1-a)$, we find the best fit of ($w_0,w_1$) is ($-1.053,0.944$) and for $w_{DE}(a)=w_0+w_1\sin (3/2\pi \ln (a))$, the best fit for ($w_0,w_1$) is ($-1.614,-1.046$). We find that a flat universe is a good approximation, namely, $|{\Omega }_K|>0.06$ has been excluded by 2$\sigma$ yet the inclusion of ${\Omega }_K$ can affect the measurement of DE parameters owing to their correlation and the present systematic effects of SNIa measurements.

The wrongly-generated last page of pdf file is removed

References in corpus (1)

• Cosmological Evolution of a Quintom Model of Dark Energy

Cited by in corpus (13)

• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• On Perturbations of Quintom Bounce
• Dark Energy Model with Spinor Matter and Its Quintom Scenario
• Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
• Determining Cosmological Parameters with Latest Observational Data
• Testing Cosmology with Cosmic Sound Waves
• High-resolution temporal constraints on the dynamics of dark energy
• Constraints on oscillating dark energy models
• Non-parametric Dark Energy Degeneracies
• Theoretic Limits on the Equation of State Parameter of Quintessence
• The Hubble constant and dark energy from cosmological distance measures
• Constraints on Dark Energy Models from Weak Gravity Conjecture
• How to Measure the Cosmic Curvature