Several recent approaches to black hole entropy obtain the density of state
s from the central charge of a Liouville theory. If Liouville theory is cou
pled to a dynamical spacetime background, however, the classical central ch
arge vanishes. I show that the central charge can be restored by introducin
g appropriate constraints, which may be interpreted ax fall-off conditions
at a boundary such as a black hole horizon. (C) 2001 Published by Elsevier
Science B.V.