Confronting Tracker Field Quintessence with Data
Abstract
We confront tracker field quintessence with observational data. The potentials considered in this paper include V(φ)φ-α, (Mp/φ), (Mp/φ)-1, (β Mp/φ) and (γ Mp/φ)-1; while the data come from the latest SN Ia, CMB and BAO observations. Stringent parameter constraints are obtained. In comparison with the cosmological constant via information criteria, it is found that models with potentials (Mp/φ), (Mp/φ)-1 and (γ Mp/φ)-1 are not supported by the current data.
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