Abstract
We consider three-dimensional gravity based on torsion. Specifically, we consider an extension of the so-called Teleparallel Equivalent of General Relativity in the presence of a scalar field with a self-interacting potential, where the scalar field is non-minimally coupled with the torsion scalar. Then, we find asymptotically AdS hairy black hole solutions, which are characterized by a scalar field with a power-law behavior, being regular outside the event horizon and null at spatial infinity and by a self-interacting potential, which tends to an effective cosmological constant at spatial infinity.
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Acknowledgements
This work was funded by Comisión Nacional de Ciencias y Tecnología through FONDECYT Grants 11140674 (PAG), and 11121148 (YV) and by DI-PUCV Grant 123713 (JS). P.A.G. acknowledge the hospitality of the Universidad de La Serena.
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González, P.A., Saavedra, J. & Vásquez, Y. Three-dimensional hairy black holes in teleparallel gravity. Astrophys Space Sci 357, 143 (2015). https://doi.org/10.1007/s10509-015-2374-8
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DOI: https://doi.org/10.1007/s10509-015-2374-8