Abstract
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.
Original language | English |
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Article number | 043 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2013 |
Issue number | 11 |
DOIs | |
State | Published - Nov 2013 |
Keywords
- cosmological perturbation theory
- inflation
- non-gaussianity