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Stationary Black Holes with Static and Counterrotating Horizons

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arxiv gr-qc/0309082 v1 pith:NTSFYJU6 submitted 2003-09-17 gr-qc

Burkhard Kleihaus , Jutta Kunz , Francisco Navarro-Lérida This is my paper · ORCID
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keywords blackholesstaticcounterrotatinghorizonhorizonsangularbifurcate
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We show that rotating dyonic black holes with static and counterrotating horizon exist in Einstein-Maxwell-dilaton theory when the dilaton coupling constant exceeds the Kaluza-Klein value. The black holes with static horizon bifurcate from the static black holes. Their mass decreases with increasing angular momentum, their horizons are prolate.

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  1. Charged, rotating black holes in Einstein-Maxwell-dilaton theory

    gr-qc 2025-06 unverdicted novelty 7.0 of 10

    Numerical construction of asymptotically flat charged rotating black holes in EMd theory for arbitrary dilaton coupling gamma, with analysis of parameter space, zero-temperature limits, and hints of non-uniqueness.

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