Abstract
We analyze primordial non-Gaussianity in single-field inflationary models when the tensor-to-scalar ratio is large. Our results show that detectable levels of non-Gaussianity fNL∼50 are still possible in the simplest class of models described by the effective theory of inflation. However, the shape is very tightly constrained, making a sharp prediction that could be confirmed or falsified by a future detection of non-Gaussianity.
Original language | English (US) |
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Article number | 081301 |
Journal | Physical Review Letters |
Volume | 113 |
Issue number | 8 |
DOIs | |
State | Published - Aug 20 2014 |
ASJC Scopus subject areas
- General Physics and Astronomy