Non-Einsteinian Black Holes in Generic 3D Gravity Theories
arXiv:1907.03498 · doi:10.1103/PhysRevD.100.064053
Abstract
The Bañados-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 non-extremal BTZ black hole loses its event horizon while the deformed extremal one remains intact as a black hole in any generic gravity theory.
arXiv comment5 pages; v2: Clarifications added. Version to appear in PRD
References in corpus (15)
- The Black Hole in Three Dimensional Space Time
- Geometry of the 2+1 Black Hole
- Massive Gravity in Three Dimensions
- Gravitational Energy in Quadratic Curvature Gravities
- Three-dimensional quantum geometry and black holes
- Black Hole Thermodynamics
- Metrics With Vanishing Quantum Corrections
- New Exact Solutions of Quadratic Curvature Gravity
- AdS-plane wave and pp-wave solutions of generic gravity theories
- Uniqueness of the asymptotic AdS3 geometry
- AdS-Wave Solutions of f(Riemann) Theories
- Three-dimensional black holes and descendants
- Kerr-Schild--Kundt Metrics are Universal
- Gravity Waves in Three Dimensions
- From Smooth Curves to Universal Metrics