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Resonant non-Gaussianity with equilateral properties

Published 1 Nov 2012 in hep-th and astro-ph.CO | (1211.0070v2)

Abstract: We discuss the effect of superimposing multiple sources of resonant non-Gaussianity, which arise for instance in models of axion inflation. The resulting sum of oscillating shape contributions can be used to "Fourier synthesize" different non-oscillating shapes in the bispectrum. As an example we reproduce an approximately equilateral shape from the superposition of O(10){\cal O}(10) oscillatory contributions with resonant shape. This implies a possible degeneracy between the equilateral-type non-Gaussianity typical of models with non-canonical kinetic terms, such as DBI inflation, and an equilateral-type shape arising from a superposition of resonant-type contributions in theories with canonical kinetic terms. The absence of oscillations in the 2-point function together with the structure of the resonant NN-point functions, imply that detection of equilateral non-Gaussianity at a level greater than the PLANCK sensitivity of fNL∼O(5)f_{NL}\sim{\cal O}(5) will rule out a resonant origin. We comment on the questions arising from possible embeddings of this idea in a string theory setting.

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