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We derive the equation of state of tracker fields, which are typical examples of freezing quintessence (quintessence with the equation of state approaching toward -1), taking into account of the late-time departure from the tracker solution due to the nonzero density parameter of dark energy _. We calculate the equation of state as a function of _ for constant =VV^''/ (V^') ^2 (during matter era) models. The derived equation of state contains a single parameter, w (₀), which parametrizes the equation of state during the matter-dominated epoch. We derive observational constraints on w (₀) and find that observational data are consistent with the cosmological constant: -1. 11<w (₀) <-0. 96 (1).
Takeshi Chiba (Fri,) studied this question.