Kerr/CFT correspondence - Misplaced Pages

Correspondence between a Kerr black hole and a conformal field theory

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The Kerr/CFT correspondence is an extension of the AdS/CFT correspondence or gauge-gravity duality to rotating black holes (which are described by the Kerr metric).

The duality works for black holes whose near-horizon geometry can be expressed as a product of AdS₃ and a single compact coordinate. The AdS/CFT duality then maps this to a two-dimensional conformal field theory (the compact coordinate being analogous to the S factor in Maldacena's original work), from which the correct Bekenstein entropy can then be deduced.

The original form of the duality applies to black holes with the maximum value of angular momentum, but it has now been speculatively extended to all lesser values.

References

Bredberg, Irene; Keeler, Cynthia; Lysov, Vyacheslav; Strominger, Andrew (2011). "Cargese Lectures on the Kerr/CFT Correspondence". Nuclear Physics B - Proceedings Supplements. 216 (1): 194–210. arXiv:1103.2355. Bibcode:2011NuPhS.216..194B. doi:10.1016/j.nuclphysbps.2011.04.155. S2CID 117563696.
Compere, Geoffrey (24 February 2009). "Kerr/CFT: A paradigm to understand the entropy of real black holes?". Archived from the original on 23 July 2011. Retrieved 23 July 2011.
Castro, Alejandra; Maloney, Alexander; Strominger, Andrew (2010). "Hidden Conformal Symmetry of the Kerr Black Hole". Physical Review D. 82 (2): 024008. arXiv:1004.0996. Bibcode:2010PhRvD..82b4008C. doi:10.1103/PhysRevD.82.024008. S2CID 118600898.

External links

Compère, Geoffrey (2017). "The Kerr/CFT correspondence and its extensions". Living Rev Relativ. 20 (1): 1. Bibcode:2017LRR....20....1C. doi:10.1007/s41114-017-0003-2. PMC 5479153. PMID 28690421.
Motl, Luboš (2010). Kerr black hole: the CFT entropy works for all M,J
Guica, Monica; Hartman, Thomas; Song, Wei; Strominger, Andrew (2009). "The Kerr/CFT correspondence". Phys. Rev. D. 80 (12): 124008. arXiv:0809.4266. Bibcode:2009PhRvD..80l4008G. doi:10.1103/PhysRevD.80.124008. S2CID 15010088.

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