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- W2080353921 abstract "The slow-roll approximation is specified for cosmological models in scalar-tensor gravity theories. Specific isotropic cosmological models with zero curvature are found for the class of theories in which the gravitational coupling function ensuremath{omega}(cphi) is a power-law function of the gravitational scalar field cphi when the Universe contains other scalar fields with constant, power-law, and exponential potentials, respectively. Some new types of inflation are found, but intermediate inflationary behavior is displayed by a wide class of models." @default.
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- W2080353921 title "Slow-roll inflation in scalar-tensor theories" @default.
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- W2080353921 doi "https://doi.org/10.1103/physrevd.51.2729" @default.
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