Cardy and Kerr
arXiv:0909.1110 · doi:10.1007/JHEP02(2010)088
Abstract
The Kerr/CFT correspondence employs the Cardy formula to compute the entropy of the left moving CFT states. This computation, which correctly reproduces the Bekenstein--Hawking entropy of the four-dimensional extremal Kerr black hole, is performed in a regime where the temperature is of order unity rather than in a high-temperature regime. We show that the comparison of the entropy of the extreme Kerr black hole and the entropy in the CFT can be understood within the Cardy regime by considering a D0-D6 system with the same entropic properties.
20 pages; LaTeX; JHEP format; v.2 references added, v.3 Section 4 added
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- Beyond Logarithmic Corrections to Cardy Formula
- Extremal Three-point Correlators in Kerr/CFT
- Entanglement Entropy of Extremal BTZ
- Hidden conformal symmetry of extreme and non-extreme Einstein-Maxwell-Dilaton-Axion black holes
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- Hot Attractors
- New Perspectives on Attractor Flows and Trees from CFT
- Generalized Hot Attractors
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