Thermodynamics of Slowly Rotating Charged Black Holes in anti-de Sitter Einstein-Gauss-Bonnet Gravity
arXiv:1011.4348 · doi:10.1088/0256-307X/28/2/020402
Abstract
By using a new approach, we demonstrate analytic expressions for slowly rotating Gauss-Bonnet charged black holes with negative cosmological constant. Up to the linear order of the rotating parameter a, the mass, Hawking temperature and entropy of the charged black holes get no corrections from rotation.
9 Pages, submitted to Chin. Phys. Lett
References in corpus (6)
- Thermodynamics of Rotating Black Branes in Gauss-Bonnet-nonlinear Maxwell Gravity
- Electromagnetic Properties of Kerr-Anti-de Sitter Black Holes
- Kerr-Schild ansatz in Einstein-Gauss-Bonnet gravity: An exact vacuum solution in five dimensions
- Five-dimensional rotating black holes in Einstein-Gauss-Bonnet theory
- Slowly Rotating Charged Gauss-Bonnet Black holes in AdS Spaces
- Thermodynamics of Rotating Solutions in Gauss-Bonnet-Maxwell Gravity and the Counterterm Method