Scaling attractors for quintessence in flat universe with cosmological term
arXiv:gr-qc/0611064 · doi:10.1088/1475-7516/2008/01/019
Abstract
For evolution of flat universe, we classify late time and future attractors with scaling behavior of scalar field quintessence in the case of potential, which, at definite values of its parameters and initial data, corresponds to exact scaling in the presence of cosmological constant.
arXiv comment11 pages, 16 eps-figures, revtex4, reference with comment added
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