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Stationary Black Holes with Static and Counterrotating Horizons

Burkhard Kleihaus, Jutta Kunz, Francisco Navarro-Lérida

gr-qcarXiv:gr-qc/0309082

Abstract

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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