![]()
Large slow-roll corrections to the bispectrum of noncanonical inflation Nongaussian statistics are a powerful discriminant between inflationary models, particularly those with noncanonical kinetic terms. Focusing on theories where the Lagrangian is an arbitrary Lorentz-invariant function of a scalar field and its first derivatives, I report the calculation of the observable three-point function. I obtain quantitative estimates of their magnitude in DBI and power-law k-inflation. In the DBI case these results enable an estimate corrections from the shape of the potential and the warp factor: these can be of order several tens of percent. I also identify a new bispectrum shape available at next-order, which is similar to a shape encountered in Galileon models. If fNL is sufficiently large this shape may be independently detectable provided a new template for CMB analysis is devised. |
We use cookies to ensure that you get the best experience on our website, by continuing on this website you agree to the storing of cookies on your device. Learn more about our Privacy Policy .