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- W2077093567 abstract "Inflation as a dynamical effect of extra dimensions is discussed from the viewpoint of the evolution of the parameters Ω and q in the physical space. By reducing the dynamics of the models FLRW (k=±1)×T D (T D =S 1 ×... ×S 1 ) and FLRW (k=0)×S D , where FLRW denotes Friedmann, Lemaitre, Robertson, and Walker, to two dimensions it is shown that inflation need not imply Ω≃ 1 for the present time, i.e., that it does not solve the flatness problem. The energy-momentum tensor of the form T υ μ =(ρ,mρ,mρ,mρ,nρ,..., nρ) is assumed" @default.
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- W2077093567 date "1993-01-15" @default.
- W2077093567 modified "2023-09-25" @default.
- W2077093567 title "Evolution of the density parameter in multidimensional cosmology" @default.
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- W2077093567 doi "https://doi.org/10.1103/physrevd.47.460" @default.
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