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arXiv · 1808.05171

Charged slowly rotating toroidal black holes in the (1+3)-dimensional Einstein-power-Maxwell theory

Grigoris Panotopoulos·Angel Rincon
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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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Grigoris Panotopoulos, Angel Rincon. 2018-08-15. Charged slowly rotating toroidal black holes in the (1+3)-dimensional Einstein-power-Maxwell theory. https://doi.org/10.1142/s0218271819500160

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