We examine cylindrically symmetric solutions to the Einstein equations under the assumption of functional separability of the metric coefficients. Under the further assumption that the energymomentum tensor is of the form T: = Tf= --a(r,t), all such solutions, with their vacuum exteriors, are found. It is shown that the vacua cannot be matched smoothly onto a Robertson-Walker background.
The matching of Friedmann-Lemaftre-Robertson-Walker space-times onto a Kasner vacuum region is investigated. We apply the Darmois junction conditions to show that a spatially flat Einstein-de Sitter region can be joined smoothly to a special case of the Kasner vacuum space-time. This result suggests an intriguing cosmological model. PACS numberk): 98.80.H~
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