Generating the primordial curvature perturbation from inflation

Abstract

The scale--independence of the primordial curvature perturbation suggests that it comes from the vacuum fluctuation during inflation of a light scalar field. This field may be the inflaton, or a different `curvaton' field. The observation of primordial non--gaussianity would be a smoking gun for the curvaton model, while the observation of gravitational waves originating during slow--roll inflation would rule out the model.

Comments: Invited talk at Moriond `The Cosmological Model'. v2 corrects minor typos and alters a few words