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Stationary circularly symmetric solutions of General Relativity with negative cosmological constant coupled to the Maxwell field are analyzed in three spacetime dimensions.
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M. Cataldo, “Azimuthal electric field in a static rotationally symmetric (2+1)-dimensional space-time,” Phys. Lett. B 529
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O. J. C. Dias and J. P. S. Lemos, “Rotating magnetic solution in three-dimensional Einstein gravity,” JHEP 0201
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G. Clement, “Black hole mass and angular momentum in 2+1 gravity,” Phys. Rev. D 68
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M. Cataldo, J. Crisostomo, S. del Campo and P. Salgado, “On magnetic solution to (2+1) Einstein-Maxwell gravity,” Phys. Lett. B 584
2004
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2004
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M. Henneaux, C. Martinez, R. Troncoso and J. Zanelli, “Asymptotically anti-de Sitter spacetimes and scalar fields with a logarithmic branch,” Phys. Rev. D 70
2004
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M. Banados and S. Theisen, “Scale invariant hairy black holes,” Phys. Rev. D 72
2005
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2011
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M. Banados, M. Henneaux, C. Teitelboim and J. Zanelli, “Geometry of the (2+1) black hole,” Phys. Rev. D 48
2013
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2013
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2013
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2013
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G. Barnich and P. H. Lambert, “Einstein-Yang-Mills theory: Asymptotic symmetries,” Phys. Rev. D 88
2013
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2014
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2014
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2015
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2015
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