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Scale dependent local non-gaussianity from loops

We analyze multi-field inflationary systems which yield strongly scale dependent non-Gaussianity with a shape that is very close to the local shape. As in usual multi-field models, the non-Gaussianity arises from the non-linear transfer of scalar field fluctuations to curvature perturbations. Here we consider models in which higher order terms (loops) dominate over the lowest order source of non-linearity. The magnitude of non-Gaussianity depends on an infrared cutoff which is determined by our observational probes measuring non-Gaussianity. In our models, the running is positive and large (nNG ∼ 0.2) on CMB scales. The magnitude of the bispectrum is maximally of order 𝒪(100), and grows on small scales. This can lead to interesting signals for large scale structure.