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• W3106417623 abstract "A class of spherically symmetric Stephani cosmological models is examined in the context of evolution type. It is assumed that the equation of state at the symmetry centre of the models is barotropic (p(t) = αρ(t)) and the function k(t) playing the role of spatial curvature is proportional to the Stephani version of the Friedmann-Robertson-Lemaître-Walker scale factor R(t) (k(t) = βR(t))." @default.
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• W3106417623 date "2001-06-29" @default.
• W3106417623 modified "2023-09-27" @default.
• W3106417623 title "Non-homogeneity-driven universe acceleration" @default.
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• W3106417623 doi "https://doi.org/10.1088/0264-9381/18/14/303" @default.
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