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Energy extraction from Kerr--Bertotti--Robinson black holes: polar region collapse and the capture of negative energy protons
The Kerr-Bertotti-Robinson black hole is an exact Einstein-Maxwell solution describing a rotating black hole in an asymptotically uniform magnetic field. It differs from the Kerr black hole in the Wald solution: the magnetic field lines are no longer cylindrical, with the constant-\(A_ϕ\) lines satu
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