Extremal and nonextremal Kerr/CFT correspondences

Abstract

I rederive the Kerr/CFT correspondence without first taking the near-horizon extremal Kerr limit. This method extends easily to nonextremal black holes, for which the temperature and central charge behave poorly at the horizon but the entropy remains finite. A computation yields one-half of the standard Bekenstein-Hawking entropy, with hints that the other half may be related to a conformal field theory at the inner horizon. I then present an alternative approach, based on a stretched Killing horizon, in which the full entropy is obtained and the temperature and central charge remain well-behaved even in the nonextremal case.

v3: missing term restored in eqn. (A.10) for central term; does not affect conclusions of this paper, but important in other contexts

References in corpus (2)

• Microscopic Realization of the Kerr/CFT Correspondence
• Black Hole Entropy and the Problem of Universality

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