English

Extremal and nonextremal Kerr/CFT correspondences

General Relativity and Quantum Cosmology 2015-05-27 v3 High Energy Physics - Theory

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.

Keywords

Cite

@article{arxiv.1101.5136,
  title  = {Extremal and nonextremal Kerr/CFT correspondences},
  author = {S. Carlip},
  journal= {arXiv preprint arXiv:1101.5136},
  year   = {2015}
}

Comments

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

R2 v1 2026-06-21T17:17:30.404Z