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- W2045653452 abstract "It is shown that cosmological models, based on the self-interacting scalar field theory or on the theory of the chiral non-linear sigma model. Can describe the global evolution of the Universe, extending from an inflationary stage to the present time epoch. The method of cosmological perturbations decomposition for inflaton and non-inflaton ones is applied for two-component chiral cosmological model in the spatially flat Friedmann-Robertson-Walker (FRW) Universe. New non-inflaton mode of cosmological perturbations is found." @default.
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- W2045653452 date "2002-11-20" @default.
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- W2045653452 title "COSMOLOGICAL MODELS OF GLOBAL UNIVERSE EVOLUTION AND DECOMPOSITION OF PERTURBATIONS" @default.
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- W2045653452 doi "https://doi.org/10.1142/s0217751x02013538" @default.
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