“School of Physics”
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| Paper IPM / P / 7269 |
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| Abstract: | |
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We introduce two classes of rotating solutions of Einstein-Maxwell gravity in n+1 dimensions which are asymptotically anti-de Sitter type. They have no curvature singularity and no horizons. The first class of solutions, which has a conic singularity yields a spacetime with a longitudinal magnetic field and k rotation parameters. We show that when one or more of the rotation parameters are non zero, the spinning brane has a net electric charge that is proportional to the magnitude of the rotation parameters. The second class of solutions yields a spacetime with an angular magnetic field and
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