Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations

Abstract

The holographic dark energy model is proposed by Li as an attempt for probing the nature of dark energy within the framework of quantum gravity. The main characteristic of holographic dark energy is governed by a numerical parameter $c$ in the model. The parameter $c$ can only be determined by observations. Thus, in order to characterize the evolving feature of dark energy and to predict the fate of the universe, it is of extraordinary importance to constrain the parameter $c$ by using the currently available observational data. In this paper, we derive constraints on the holographic dark energy model from the latest observational data including the gold sample of 182 Type Ia supernovae (SNIa), the shift parameter of the cosmic microwave background (CMB) given by the three-year {\it Wilkinson Microwave Anisotropy Probe} ({\it WMAP}) observations, and the baryon acoustic oscillation (BAO) measurement from the Sloan Digital Sky Survey (SDSS). The joint analysis gives the fit results in 1-$\sigma$: $c=0.91_{-0.18}^{+0.26}$ and ${\Omega }_{m0}=0.29\pm 0.03$. That is to say, though the possibility of $c<1$ is more favored, the possibility of $c>1$ can not be excluded in one-sigma error range, which is somewhat different from the result derived from previous investigations using earlier data. So, according to the new data, the evidence for the quintom feature in the holographic dark energy model is not as strong as before.

22 pages, 8 figures; accepted for publication in Phys. Rev. D

References in corpus (17)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Dynamics of dark energy
• Cosmology and the Fate of Dilatation Symmetry
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Cosmological Evolution of a Quintom Model of Dark Energy
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Reconstruction of the deceleration parameter and the equation of state of dark energy
• Reconstructing holographic quintessence
• Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
• A String-Inspired Quintom Model Of Dark Energy
• Probing for dynamics of dark energy and curvature of universe with latest cosmological observations
• Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• Inflation with Holographic Dark Energy
• Accelerating cosmologies tested by distance measures
• Confronting pNGB quintessence with data
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets

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