Journal
PHYSICAL REVIEW D
Volume 80, Issue 12, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.80.124008
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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/h. 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/h for the CFT, which reproduces the macroscopic Bekenstein-Hawking entropy S-macro = Area/4hG. 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/h, and, in particular, that the near-extreme black hole GRS 1915+105 is approximately dual to a CFT with c(L) similar to 2 x 10(79).
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