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arxiv: 1306.3691 · v1 · submitted 2013-06-16 · ✦ hep-th · astro-ph.CO· gr-qc

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Equilateral non-Gaussianity from heavy fields

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classification ✦ hep-th astro-ph.COgr-qc
keywords non-gaussianityfieldsheavyderiveequilateralinflationself-interactionsapproaches
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The effect of self-interactions of heavy scalar fields during inflation on the primordial non-Gaussianity is studied. We take a specific constant-turn quasi-single field inflation as an example. We derive an effective theory with emphasis on non-linear self-interactions of heavy fields and calculate the corresponding non-Gaussianity, which is of equilateral type and can be as relevant as those computed previously in the literature. We also derive the non-Gaussianity by directly using the in-in formalism, and verify the equivalence of these two approaches.

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