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Angular momentum-area proportionality of extremal charged black holes in odd dimensions

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arxiv 1309.2088 v1 pith:FXMS3V55 submitted 2013-09-09 gr-qc hep-th

Jose Luis Blazquez-Salcedo , Jutta Kunz , Francisco Navarro-Lerida This is my paper · ORCID
classification gr-qchep-th
keywords angularmomentumhorizonproportionalareablackbranchbranches
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Extremal rotating black holes in Einstein-Maxwell theory feature two branches. On the branch emerging from the Myers-Perry solutions their angular momentum is proportional to their horizon area, while on the branch emerging from the Tangherlini solutions their angular momentum is proportional to their horizon angular momentum. The transition between these branches occurs at a critical value of the charge, which depends on the value of the angular momentum. However, when a dilaton is included, the angular momentum is always proportional to the horizon area.

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  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...

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