Three-dimensional hairy black holes in teleparallel gravity

P. A. González; Joel Saavedra; Yerko Vásquez

doi:10.1007/s10509-015-2374-8

Three-dimensional hairy black holes in teleparallel gravity

P. A. González, Joel Saavedra, Yerko Vásquez

Research output: Contribution to journal › Article › peer-review

7 Scopus citations

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.

Original language	English
Article number	143
Journal	Astrophysics and Space Science
Volume	357
Issue number	2
DOIs	https://doi.org/10.1007/s10509-015-2374-8
State	Published - 1 Jun 2015
Externally published	Yes

Keywords

Hairy black holes
Teleparallel gravity

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10.1007/s10509-015-2374-8

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title = "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.",

keywords = "Hairy black holes, Teleparallel gravity",

author = "Gonz{\'a}lez, {P. A.} and Joel Saavedra and Yerko V{\'a}squez",

note = "Funding Information: This work was funded by Comisi{\'o}n Nacional de Ciencias y Tecnolog{\'i}a 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. Publisher Copyright: {\textcopyright} 2015, Springer Science+Business Media Dordrecht.",

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doi = "10.1007/s10509-015-2374-8",

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T1 - Three-dimensional hairy black holes in teleparallel gravity

AU - González, P. A.

AU - Saavedra, Joel

AU - Vásquez, Yerko

N1 - Funding Information: 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. Publisher Copyright: © 2015, Springer Science+Business Media Dordrecht.

PY - 2015/6/1

Y1 - 2015/6/1

N2 - 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.

AB - 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.

KW - Hairy black holes

KW - Teleparallel gravity

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DO - 10.1007/s10509-015-2374-8

M3 - Article

AN - SCOPUS:84929080022

VL - 357

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

SN - 0004-640X

IS - 2

M1 - 143

ER -

Three-dimensional hairy black holes in teleparallel gravity

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