The Kerr-Newman-Gödel Black Hole
نویسنده
چکیده
By applying a set of Hassan-Sen transformations and string dualities to the Kerr-Gödel solution of minimal D = 5 supergravity we derive a four parameter family of five dimensional solutions in type II string theory. They describe rotating, charged black holes in a rotating background. For zero background rotation, the solution is D = 5 Kerr-Newman; for zero charge it is Kerr-Gödel. In a particular extremal limit the solution describes an asymptotically Gödel BMPV black hole.
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