Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset

Abstract

Recently, many efforts have been made to build dark energy models whose equation-of-state parameter can cross the so-called phantom divide $w_{de}=-1$. One of them is the so-called hessence dark energy model in which the role of dark energy is played by a non-canonical complex scalar field. In this work, we develop a simple method based on Hubble parameter $H(z)$ to reconstruct the hessence dark energy. As examples, we use two familiar parameterizations for $H(z)$ and fit them to the latest 182 type Ia supernovae Gold dataset. In the reconstruction, measurement errors are fully considered.

14 pages, 6 figures, revtex4; v2: references added; v3: published version

References in corpus (4)

• Cosmological Evolution of a Quintom Model of Dark Energy
• Can dark energy evolve to the Phantom?
• Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
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