Supercurvaton
  We discuss observational consequences of the curvaton scenario, which
naturally appears in the context of the simplest model of chaotic inflation in
supergravity. The non-gaussianity parameter f_NL in this scenario can take
values in the observationally interesting range from O(10) to O(100). These
values may be different in different parts of the universe. The regions where
f_NL is particularly large form a curvaton web resembling a net of thick domain
walls, strings, or global monopoles.
