Scaling attractors for quintessence in flat universe with cosmological term

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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.
11 pages, 16 eps-figures, revtex4, reference with comment added

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/194284

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0611064
 http://arxiv.org/abs/gr-qc/0611064
 JCAP0801:019,2008
 doi:10.1088/1475-7516/2008/01/019

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arXiv