Generic inference of inflation models by local non-Gaussianity
  The presence of multiple fields during inflation might seed a detectable amount of non-Gaussianity in the curvature perturbations, which in turn becomes observable in present data sets like the cosmic microwave background (CMB) or the large scale structure (LSS). Within this proceeding we present a fully analytic method to infer inflationary parameters from observations by exploiting higher-order statistics of the curvature perturbations. To keep this analyticity, and thereby to dispense with numerically expensive sampling techniques, a saddle-point approximation is introduced whose precision has been validated for a numerical toy example. Applied to real data, this approach might enable to discriminate among the still viable models of inflation. 
Sebastian Dorn, Erandy Ramirez, Kerstin E. Kunze, Stefan Hofmann, and   Torsten A. En{\ss}lin
astro-ph.CO astro-ph.IM