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• W3100216653 abstract "We study a time-dependent five-dimensional (5D) metric which contains a static four-dimensional (4D) sub-metric whose three-dimensional (3D) part is spherically symmetric. An expansion in the metric coefficient allow us to obtain close-to Schwarzschild approximation to a class of spherically symmetric solutions. Using Campbell’s embedding theorem and the induced-matter formalism we obtain two 4D solutions. One describes a source with the stiff equation of state believed to be applicable to dense astrophysical objects, and the other describes a spherical source with a radial heat flow." @default.
• W3100216653 created "2020-11-23" @default.
• W3100216653 creator A5011131609 @default.
• W3100216653 creator A5043244187 @default.
• W3100216653 date "2001-10-01" @default.
• W3100216653 modified "2023-09-23" @default.
• W3100216653 title "Radiating sources in higher-dimensional gravity" @default.
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• W3100216653 doi "https://doi.org/10.1063/1.1401139" @default.
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