Abstract
Long-ranged density correlations, varying on the scale of the capillary length Lc, exist in the liquid-vapor interface in a weak gravitational field. A scaling hypothesis, similar to that made near the bulk critical point, predicts that in dimensions d<3, the interface width W as Lc. For d>3, W can remain finite provided there is power-law decay of correlations for separations less than Lc. These results are consistent with capillary-wave theory.