  We discuss nontrivial features of the large scale structure of the universe
in the simplest curvaton model proposed in our paper astro-ph/9610219. The
amplitude of metric perturbations in this model takes different values in
different parts of the universe. The spatial distribution of the amplitude
looks like a web consisting of exponentially large cells. Depending on the
relation between the cell size l_0 and the scale of the horizon l_H, one may
either live in a part of the universe dominated by gaussian perturbations
(inside a cell with l_0 >> l_H), or in the universe dominated by nongaussian
perturbations (for l_0 << l_H). We show that the curvaton contribution to the
total amplitude of adiabatic density perturbations can be strongly suppressed
if the energy density of the universe prior to the curvaton decay was dominated
not by the classical curvaton field but by the curvaton particles produced
during reheating. We describe the curvaton-inflaton transmutation effect: The
same field in different parts of the universe may play either the role of the
curvaton or the role of the inflaton. Finally, we discuss an interplay between
the curvaton web and anthropic considerations in the string theory landscape.
