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Charged slowly rotating toroidal black holes in the (1+3)-dimensional Einstein-power-Maxwell theory (1808.05171v3)
Published 15 Aug 2018 in gr-qc
Abstract: In this work we find charged slowly rotating solutions in the four-dimensional Einstein-power-Maxwell non-linear electrodynamics assuming a negative cosmological constant. By solving the system of coupled field equations explicitly we obtain an approximate analytical solution in the small rotation limit. The solution obtained is characterized by a flat horizon structure, and it corresponds to a toroidal black hole. The Smarr's formula, the thermodynamics and the invariants Ricci scalar and Kretschmann scalar are briefly discussed.
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