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arxiv: astro-ph/0511198 · v1 · submitted 2005-11-07 · 🌌 astro-ph · hep-ph· hep-th

Non-Gaussianity from Broken Symmetries

classification 🌌 astro-ph hep-phhep-th
keywords inflationmodelnon-gaussianityworkapproximatebrokencharacterizedcompute
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Recently we studied inflation models in which the inflaton potential is characterized by an underlying approximate global symmetry. In the first work we pointed out that in such a model curvature perturbations are generated after the end of the slow-roll phase of inflation. In this work we develop further the observational implications of the model and compute the degree of non-Gaussianity predicted in the scenario. We find that the corresponding nonlinearity parameter, $f_{NL}$, can be as large as 10^2.

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