We study the procedure of the reconstruction of phantom-scalar field potentials in two-field cosmological models. It is shown that while in the one-field case the chosen cosmological evolution defines uniquely the form of the scalar potential, in the two-field case one has an infinite number of possibilities. The classification of a large class of possible potentials is presented and the dependence of cosmological dynamics on the choice of initial conditions is investigated qualitatively and numerically for two particular models.

Reconstruction of scalar potentials in two-field cosmological models

KAMENCHTCHIK, ALEXANDR;REGOLI, DANIELE
2008

Abstract

We study the procedure of the reconstruction of phantom-scalar field potentials in two-field cosmological models. It is shown that while in the one-field case the chosen cosmological evolution defines uniquely the form of the scalar potential, in the two-field case one has an infinite number of possibilities. The classification of a large class of possible potentials is presented and the dependence of cosmological dynamics on the choice of initial conditions is investigated qualitatively and numerically for two particular models.
A.A. Andrianov; F. Cannata; A.Y. Kamenshchik; D. Regoli
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11585/55783
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