Three-Dimensional Hairy Black Holes in Teleparallel Gravity

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.

18 pages, 8 figures, improved version

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Cited by in corpus (7)

• Teleparallel Equivalent of Lovelock Gravity
• Onset of acceleration in a Universe initially filled by dark and baryonic matters in nonminimally coupled teleparallel model
• Black Holes, Dark Wormholes and Solitons in f(T) Gravities
• Dirac field as a source of the inflation in 2+1 dimensional Teleparallel gravity
• Teleparallel Equivalent of Lovelock Gravity, Generalizations and Cosmological Applications
• Hyperscaling violating black holes in scalar-torsion theories
• Gravity coupled to a scalar field from a Chern-Simons action: describing rotating hairy black holes and solitons with gauge fields