The Four-point Correlator in Multifield Inflation, the Operator Product
  Expansion and the Symmetries of de Sitter
  We study the multifield inflationary models where the cosmological
perturbation is sourced by light scalar fields other than the inflaton. We
exploit the operator product expansion and partly the symmetries present during
the de Sitter epoch to characterize the non-Gaussian four-point correlator in
the squeezed limit. We point out that the contribution to it from the intrinsic
non-Gaussianity of the light fields at horizon crossing can be larger than the
usually studied contribution arising on superhorizon scales and it comes with a
different shape. Our findings indicate that particular attention needs to be
taken when studying the effects of the primordial NG on real observables, such
as the clustering of dark matter halos.
