Charged BTZ-type solutions in Eddington-inspired Born-Infeld gravity

被引:6
|
作者
Guerrero, Merce [1 ,2 ]
Mora-Perez, Gerardo [3 ,4 ]
Olmo, Gonzalo J. [3 ,4 ]
Orazi, Emanuele [5 ,6 ]
Rubiera-Garcia, Diego [1 ,2 ]
机构
[1] Univ Complutense Madrid, Dept Fis Teor, Plaza Ciencias S-N, E-28040 Madrid, Spain
[2] Univ Complutense Madrid, IPARCOS, Plaza Ciencias S-N, E-28040 Madrid, Spain
[3] Univ Valencia, CSIC, Ctr Mixto Univ Valencia, Dept Fis Teor, Valencia 46100, Spain
[4] Univ Valencia, CSIC, Ctr Mixto Univ Valencia, IFIC, Valencia 46100, Spain
[5] Univ Fed Rio Grande do Norte, Int Inst Phys, Campus Univ Lagoa Nova, BR-59078970 Natal, RN, Brazil
[6] Univ Fed Rio Grande do Norte, Escola Ciencia & Tecnol, Caixa Postal 1524, BR-59078970 Natal, RN, Brazil
关键词
modified gravity; Exact solutions; black holes and black hole thermodynamics in GR and beyond; Wormholes; TIME;
D O I
10.1088/1475-7516/2021/11/025
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We construct an axially symmetric solution of Eddington-inspired Born-Infeld gravity coupled to an electromagnetic field in 2 + 1 dimensions including a (negative) cosmological constant term. This is achieved by using a recently developed mapping procedure that allows to generate solutions in certain families of metric-affine gravity theories starting from a known seed solution of General Relativity, which in the present case corresponds to the electrically charged Banados-Teitelboim-Zanelli (BTZ) solution. We discuss the main features of the new configurations, including the modifications to the ergospheres and horizons, the emergence of wormhole structures, and the consequences for the regularity (or not) of these space-times via geodesic completeness.
引用
收藏
页数:23
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