Anti-de Sitter Quotients, Bubbles of Nothing, and Black Holes
arXiv:0801.4214 · doi:10.1007/s10714-008-0639-z
Abstract
In 3+1 dimensions there are anti-de quotients which are black holes with toroidal event horizons. By analytic continuation of the Schwarzschild-anti-de Sitter solution (and appropriate identifications) one finds two one parameter families of spacetimes that contain these quotient black holes. One of these families consists of B-metrics ("bubbles of nothing"), the other of black hole spacetimes. All of them have vanishing conserved charges.
arXiv comment14 pages, 3 figures. References added, one explanation improved
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