Non-Einsteinian black holes in generic 3D gravity theories

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Non-Einsteinian_black_holes_in_generic_3D_gravity_theories.pdf

Date

2019-09-21

Author

Gürses, Metin
Şisman, Tahsin Çağrı
Tekin, Bayram

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The Banados-Teitelboim-Zanelli (BTZ) black hole metric solves the three-dimensional Einstein's theory with a negative cosmological constant as well as all the generic higher derivative gravity theories based on the metric; as such it is a universal solution. Here, we find, in all generic higher derivative gravity theories, new universal non-Einsteinian solutions obtained as Kerr-Schild type deformations of the BTZ black hole. Among these, the deformed nonextremal BTZ black hole loses its event horizon while the deformed extremal one remains intact as a black hole in any generic gravity theory.

Subject Keywords

Gravitation, Cosmology, Astrophysics

URI

https://dx.doi.org/10.1103/PhysRevD.100.064053
https://hdl.handle.net/11511/28656

Journal

Physical Review D

DOI

https://doi.org/10.1103/PhysRevD.100.064053

Collections

Department of Physics, Article

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Citation Formats

M. Gürses, T. Ç. Şisman, and B. Tekin, “Non-Einsteinian black holes in generic 3D gravity theories,” Physical Review D, 2019, Accessed: 00, 2020. [Online]. Available: https://dx.doi.org/10.1103/PhysRevD.100.064053.