Nashed, G. G. L. Charged three-dimensions black holes in Weitzenböck geometry. (English) Zbl 1376.83025 Int. J. Geom. Methods Mod. Phys. 14, No. 7, Article ID 1750105, 16 p. (2017). Summary: In this study, we propose to derive circularly symmetric black holes in three-dimensions Maxwell-teleparallel gravity using a non-diagonal traid. Singularities and horizons of these black holes are analyzed. The conserved quantities are calculated using Komar formula and vanishing values are obtained. Therefore, a regularization through relocalization method is applied and finite values of mass and angular momentum are obtained. MSC: 83C57 Black holes 83D05 Relativistic gravitational theories other than Einstein’s, including asymmetric field theories 53Z05 Applications of differential geometry to physics 83C22 Einstein-Maxwell equations 83C80 Analogues of general relativity in lower dimensions Keywords:\(f(T)\) theories of gravity; axially symmetric solution; total conserved charge; black hole; Weitzenböck geometry; Maxwell-teleparallel gravity; Komar formula PDFBibTeX XMLCite \textit{G. G. L. Nashed}, Int. J. Geom. Methods Mod. Phys. 14, No. 7, Article ID 1750105, 16 p. (2017; Zbl 1376.83025) Full Text: DOI References: [1] Singh, D. V. and Siwach, S., J. Phys. Conf. Ser.481 (2014) 012014. [2] Banados, M., Teitelboim, C. and Zanelli, J., Phys. Rev. Lett.69 (1992) 1849. [3] Carlip, S., Class. Quantum Grav.12 (1995) 2853. [4] Carlip, S., Class. Quantum Grav.22 (2005) R85. [5] Ross, S. F. and Mann, R. B., Phys. Rev. D47 (1993) 3319. [6] Horowitz, G. T. and Welch, D. L., Phys. Rev. Lett.71 (1993) 328. [7] M. 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