Extremal Kerr black hole/CFT correspondence in the five-dimensional Gödel universe

2009/01/31 by Jun-Jin Peng, Shuang-Qing Wu, Shuang‐Qing Wu · 2 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #hep-th

paper · pdf · doi:10.1016/j.physletb.2009.02.020

published as Phys.Lett.B673:216-219,2009 · 11pages,no figures,accepted by PLB

arxiv created 2009/02/19 · openalex publication_date 2009/02/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31

Abstract

We extend the method of Kerr/CFT correspondence recently proposed in arXiv:0809.4266 [hep-th] to the extremal (charged) Kerr black hole embedded in the five-dimensional Gödel universe. With the aid of the central charges in the Virasoro algebra and the Frolov–Thorne temperatures, together with the use of the Cardy formula, we have obtained the microscopic entropies that precisely agree with the ones macroscopically calculated by Bekenstein–Hawking area law.

Citations

• The CFT-interpolating black hole in three dimensions
• Conserved Charges and Thermodynamics of the Spinning Gödel Black Hole
• D--branes and Spinning Black Holes
• Central charges in the canonical realization of asymptotic symmetries: An example from three dimensional gravity
• Microscopic Origin of the Bekenstein-Hawking Entropy

Cited by

• Kerr-CFT and gravitational perturbations
• Extremal Kerr/CFT correspondence of five-dimensional rotating (charged) black holes with squashed horizons