O. Coussaert et al., THE ASYMPTOTIC DYNAMICS OF 3-DIMENSIONAL EINSTEIN GRAVITY WITH A NEGATIVE COSMOLOGICAL CONSTANT, Classical and quantum gravity, 12(12), 1995, pp. 2961-2966
Liouville theory is shown to describe the asymptotic dynamics of three
-dimensional Einstein gravity with a negative cosmological constant. T
his is because (i) Chern-Simons theory with a gauge group SL(2, R) x S
L(2, R) on a spacetime with a cylindrical boundary is equivalent to th
e non-chiral SL(2, R) WZW model; and (ii) the anti-de Sitter boundary
conditions implement the constraints that reduce the WZW model to the
Liouville theory.