Charged slowly rotating toroidal black holes in the (1+3)-dimensional Einstein-power-Maxwell theory
General Relativity and Quantum Cosmology
2018-09-05 v3
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.
Keywords
Cite
@article{arxiv.1808.05171,
title = {Charged slowly rotating toroidal black holes in the (1+3)-dimensional Einstein-power-Maxwell theory},
author = {Grigoris Panotopoulos and Angel Rincon},
journal= {arXiv preprint arXiv:1808.05171},
year = {2018}
}
Comments
v3: References added