Function spaces, differential operators and nonlinear analysis (Friedrichroda, 1992).
Teubner, Stuttgart.
1993.
P. 256-263
Summary: "The scalar fields are of considerable current use in homogeneous isotropic cosmological models. Such a description is generally believed to be more complete as compared with that employing the barotropic equation of state of a perfect fluid. The two descriptions are shown to be completely equivalent for the scalar fields with exponential potentials."