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• W2023184065 abstract "Using the cosmological perturbation theory in terms of the delta-N formalism, we find the simple formulation of the evolution of the curvature perturbation in generalized gravity theories. Compared with the standard gravity theory, a crucial difference appears in the end-boundary of the inflationary stage, which is due to the non-ideal form of the energy momentum tensor that depends explicitly on the curvature scalar. Recent study shows that ultraviolet-complete quantum theory of gravity may be approximated by using a generalized gravity action. Our paper may give an important step in understanding the evolution of the curvature perturbation during inflation, where the energy momentum tensor may not be given by the ideal form due to the corrections from the fundamental theory." @default.
• W2023184065 created "2016-06-24" @default.
• W2023184065 creator A5033424080 @default.
• W2023184065 date "2009-07-02" @default.
• W2023184065 modified "2023-10-18" @default.
• W2023184065 title "Evolution of curvature perturbation in generalized gravity theories" @default.
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• W2023184065 doi "https://doi.org/10.1088/0264-9381/26/14/145016" @default.
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