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• W1973320634 abstract "We consider 5-dimensional cosmological solutions of a single brane. The correct cosmology on the brane, i.e., governed by the standard 4-dimensional Friedmann equation, and stable compactification of the extra dimension is guaranteed by the existence of a non-vanishing hat{T}^5_5 which is proportional to the 4-dimensional trace of the energy-momentum tensor. We show that this component of the energy-momentum tensor arises from the backreaction of the dilaton coupling to the brane. The same positive features are exhibited in solutions found in the presence of non-vanishing cosmological constants both on the brane (Lambda_{br}) and in the bulk (Lambda_B). Moreover, the restoration of the Friedmann equation, with the correct sign, takes place for both signs of $Lambda_B$ so long as the sign of $Lambda_{br}$ is opposite $Lambda_B$ in order to cancel the energy densities of the two cosmological constants. We further extend our single-brane thin-wall solution to allow a brane with finite thickness." @default.
• W1973320634 created "2016-06-24" @default.
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• W1973320634 date "2000-04-24" @default.
• W1973320634 modified "2023-09-27" @default.
• W1973320634 title "Single-brane cosmological solutions with a stable compact extra dimension" @default.
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• W1973320634 doi "https://doi.org/10.1103/physrevd.61.106004" @default.
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