arXiv · 1009.3020
Strongly Scale-dependent Non-Gaussianity
Abstract
We discuss models of primordial density perturbations where the non-Gaussianity is strongly scale-dependent. In particular, the non-Gaussianity may have a sharp cut-off and be very suppressed on large cosmological scales, but sizeable on small scales. This may have an impact on probes of non-Gaussianity in the large-scale structure and in the cosmic microwave background radiation anisotropies.
Explore related subjects
Keep this discovery
Antonio Riotto, Martin S. Sloth. 2010-09-15. Strongly Scale-dependent Non-Gaussianity. https://doi.org/10.1103/physrevd.83.041301
Cite the original work for its findings. Save a collection to share your selection of sources.