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Rotating Black Holes which Saturate a Bogomol'nyi Bound

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arxiv hep-th/9509108 v1 pith:M4BAGTBG submitted 1995-09-20 hep-th gr-qc

classification hep-thgr-qc
keywords blackbogomolbounddimensionalholerotatingsolutionextremal
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abstract

We construct and study the electrically charged, rotating black hole solution in heterotic string theory compactified on a $(10-D)$ dimensional torus. This black hole is characterized by its mass, angular momentum, and a $(36-2D)$ dimensional electric charge vector. One of the novel features of this solution is that for $D >5$, its extremal limit saturates the Bogomol'nyi bound. This is in contrast with the $D=4$ case where the rotating black hole solution develops a naked singularity before the Bogomol'nyi bound is reached. The extremal black holes can be superposed, and by taking a periodic array in $D>5$, one obtains effectively four dimensional solutions without naked singularities.

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  1. De Sitter space constraints on brane tensions and couplings

    hep-th 2024-11 conditional novelty 6.0 of 10

    The Festina Lente bound on particle masses is generalized to p-branes with world-volume Chern-Simons couplings, giving tension bounds in de Sitter space that string theory D-branes satisfy.

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