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Five-Dimensional Charged Rotating Black Holes

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arxiv gr-qc/0503010 v1 pith:6E6S5YN7 submitted 2005-03-02 gr-qc

Jutta Kunz , Francisco Navarro-Lerida , Anna Katinka Petersen This is my paper · ORCID
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keywords blackholesangularchargedhorizonmomentarotatingassociated
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We consider charged rotating black holes in 5-dimensional Einstein-Maxwell theory. These black holes are asymptotically flat, they possess a regular horizon of spherical topology and two independent angular momenta associated with two distinct planes of rotation. We discuss their global and horizon properties, and derive a generalized Smarr formula. We construct these black holes numerically, focussing on black holes with a single angular momentum, and with two equal-magnitude angular momenta.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Charged and rotating near-horizon geometries in five dimensions

    hep-th 2026-06 conditional novelty 7.0 of 10

    New closed-form charged rotating five-dimensional near-horizon geometries exist with two independent angular momenta and constant co-rotating electric field, characterized by Sasakian structure and matching expected e...

  2. Proca-type Hair of Rotating Black Holes in Higher Dimensions

    hep-th 2026-05 unverdicted novelty 6.0 of 10

    Spacetime symmetries generate stealth Proca vector fields on arbitrary backgrounds, enabling exact Proca-haired rotating black holes in all dimensions.

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