English

The Kerr/CFT Correspondence

High Energy Physics - Theory 2013-05-29 v1 Astrophysics General Relativity and Quantum Cosmology

Abstract

Quantum gravity in the region very near the horizon of an extreme Kerr black hole (whose angular momentum and mass are related by J=GM^2) is considered. It is shown that consistent boundary conditions exist, for which the asymptotic symmetry generators form one copy of the Virasoro algebra with central charge c_L=12J / \hbar. This implies that the near-horizon quantum states can be identified with those of (a chiral half of) a two-dimensional conformal field theory (CFT). Moreover, in the extreme limit, the Frolov-Thorne vacuum state reduces to a thermal density matrix with dimensionless temperature T_L=1/2\pi and conjugate energy given by the zero mode generator, L_0, of the Virasoro algebra. Assuming unitarity, the Cardy formula then gives a microscopic entropy S_{micro}=2\pi J / \hbar for the CFT, which reproduces the macroscopic Bekenstein-Hawking entropy S_{macro}=Area / 4\hbar G. The results apply to any consistent unitary quantum theory of gravity with a Kerr solution. We accordingly conjecture that extreme Kerr black holes are holographically dual to a chiral two-dimensional conformal field theory with central charge c_L=12J / \hbar, and in particular that the near-extreme black hole GRS 1915+105 is approximately dual to a CFT with c_L \sim 2 \times 10^{79}.

Keywords

Cite

@article{arxiv.0809.4266,
  title  = {The Kerr/CFT Correspondence},
  author = {Monica Guica and Thomas Hartman and Wei Song and Andrew Strominger},
  journal= {arXiv preprint arXiv:0809.4266},
  year   = {2013}
}

Comments

21 pages, no figures

R2 v1 2026-06-21T11:23:53.274Z