Abstract
We study quintessence and phantom field theory models based on linear-negative potentials of the form . We investigate the predicted redshift dependence of the equation of state parameter for a wide range of slopes in both quintessence and phantom models. We use the Gold data set of 157 SnIa and place constraints on the allowed range of slopes . We find for quintessence and for phantom models (the range is at the level and the units of are in where is the Planck mass). In both cases the best fit is very close to corresponding to a cosmological constant. We also show that specific model independent parametrizations of which allow crossing of the phantom divide line (hereafter PDL) provide significantly better fits to the data. Unfortunately such crossings are not allowed in any phantom or quintessence single field model minimally coupled to gravity. Mixed models (coupled phantom-quintessence fields) can in principle lead to a crossing the PDL but a preliminary investigation indicates that this does not happen for natural initial conditions.
- Received 13 December 2004
DOI:https://doi.org/10.1103/PhysRevD.71.063503
©2005 American Physical Society