Mixed non-Gaussianity in multiple-DBI inflation
arXiv:1303.3975 · doi:10.1088/1475-7516/2013/05/021
Abstract
We study a model of multiple-field DBI inflation leading to mixed form of primordial non-Gaussianity, including equilateral and local bispectrum shapes. We present a general formalism based on the Hamilton-Jacobi approach, allowing us to go beyond slow-roll, combining the three-point function for the fields at Hubble-exit with the non-linear evolution of super-Hubble scales. We are able to obtain analytic results by taking a separable Ansatz for the Hubble rate. We find general expressions for both the equilateral and local type non-Gaussianity parameter fNL. The equilateral non-Gaussianity includes the usual enhancement for small sound speeds, but multiplied by an analytic factor which can lead to a suppression. We illustrate our results with two scenarios. In the first model, previously found to have detectable local non-Gaussianity, we find that the equilateral signal is not sufficiently suppressed to evade current observational bounds. In our second scenario we construct a model which exhibits both a detectable equilateral fNL and a negative local fNL.
29 pages, 2 figures; typos corrected, references added, accepted for publication in JCAP. arXiv admin note: text overlap with arXiv:1203.6625
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- D-brane Potentials in the Warped Resolved Conifold and Natural Inflation
- Hubble multi-scalar inflation
- Scale-dependent CMB power asymmetry from primordial speed of sound and a generalized N formalism
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- Multi-brid DBI Inflation