Generalized Swiss-Cheese Cosmologies II: Spherical Dust
  The generalized Swiss - cheese model, consisting of a Lema\^itre - Tolman
(inhomogeneous dust) region matched, by way of a comoving boundary surface,
onto a Robertson-Walker background of homogeneous dust, has become a standard
construction in modern cosmology. Here we ask if this construction can be made
more realistic by introducing some evolution of the boundary surface. The
answer we find is no. To maintain a boundary surface using the Darmois - Israel
junction conditions, as opposed to the introduction of a surface layer, the
boundary must remain exactly comoving. The options are to drop the assumption
of dust or allow the development of surface layers. Either option fundamentally
changes the original construction.
