On non-gaussianities in single-field inflation

Preprint

25 September 2003

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0306122

Abstract

We study the impact of higher dimension operators in the inflaton Lagrangian on the non-gaussianity of the scalar spectrum. These terms can strongly enhance the effect without spoiling slow-roll, though it is difficult to exceed f_NL ~ 1, because the scale which suppresses the operators cannot be too low, if we want the effective field theory description to make sense. In particular we explicitly calculate the 3-point function given by an higher derivative interaction of the form (\nabla\phi)^4, which is expected to give the most important contribution. The angular dependence of the result turns out to be quite different from the minimal case without higher dimension operators.

Keywords

All Related Versions

Version 1, 2003-06-05, ArXiv
Version 2, 2003-09-25, ArXiv
Published version: Journal of Cosmology and Astroparticle Physics, 2003 (10), 003.

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