A new metric for rotating black holes in Gauss-Bonnet gravity
arXiv:1107.2743 · doi:10.1088/1674-1056/20/5/050401
Abstract
This paper presents a new metric and studies slowly rotating Gauss-Bonnet black holes with one nonvanishing angular momentum in five dimensional anti-de Sitter spaces. Taking the angular momentum parameter up to second order, the slowly rotating black hole solutions are obtained by working directly in the action. In addition, it also finds that this method is applicable in higher order Lovelock gravity.
9 pages
References in corpus (5)
- A Note on Thermodynamics of Black Holes in Lovelock Gravity
- Rotating Black Holes in Higher Dimensional Einstein-Maxwell Gravity
- Electromagnetic Properties of Kerr-Anti-de Sitter Black Holes
- Slowly Rotating Charged Gauss-Bonnet Black holes in AdS Spaces
- Hawking radiation from the Schwarzschild black hole with a global monopole via gravitational anomaly
Cited by in corpus (5)
- Static spherically symmetric star in Gauss-Bonnet gravity
- Rotating Black Holes in Einstein-Gauss-Bonnet Gravity: Mass and Angular Momentum in Extremality
- Thermodynamics of Third Order Lovelock-Born-Infeld Black Holes
- Gravitational Perfect Fluid Collapse in Gauss-Bonnet Gravity
- Spontaneous emission of a two-level static atom coupling with the electromagnetic vacuum fluctuations outside a high-dimensional Einstein Gauss-Bonnet black hole