Lifting Primordial Non-Gaussianity Above the Noise
  Primordial non-Gaussianity (PNG) in Large Scale Structures is obfuscated by
the many additional sources of non-linearity. Within the Effective Field Theory
approach to Standard Perturbation Theory, we show that matter non-linearities
in the bispectrum can be modeled sufficiently well to strengthen current bounds
with near future surveys, such as Euclid. We find that the EFT corrections are
crucial to this improvement in sensitivity. Yet, our understanding of
non-linearities is still insufficient to reach important theoretical benchmarks
for equilateral PNG, while, for local PNG, our forecast is more optimistic. We
consistently account for the theoretical error intrinsic to the perturbative
approach and discuss the details of its implementation in Fisher forecasts.
