Wormhole solutions in the Randall-Sundrum scenario
arXiv:gr-qc/0306017 · doi:10.1016/j.physletb.2003.08.042
Abstract
In the simplest form of the Randall-Sundrum model, we consider the metric generated by a static, spherically symmetric distribution of matter on the physical brane. The solution to the five-dimensional Einstein equations, obtained numerically, describes a wormhole geometry.
10 pages, 2 figures, revtex4
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