Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation
- ,
5 pages
Published in:
- Phys.Rev.D 81 (2010) 063511
e-Print:
- 0909.0496 [astro-ph.CO]
Report number:
- MIT-CTP-4071
View in:
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Abstract: (arXiv)
We study the slow-roll inflation models, where the inflaton slow-rolls along a trajectory whose orthogonal directions are lifted by potentials with masses of order the Hubble parameter. In these models large non-Gaussianities can be generated through the transformation from the isocurvature modes to the curvature mode, once the inflaton trajectory turns. We find large bispectra with one-parameter family of novel shapes, interpolating between the equilateral and local shape. According to the in-in formalism, the shapes of these non-Gaussianities are different from a simple projection from the isocurvature non-Gaussian correlation functions.- 98.70.Vc
- 98.80.Cq
- non-Gaussianity
- slow-roll approximation
- inflaton: trajectory
- inflation
- correlation function
- Hubble constant
- curvature
- power spectrum
References(29)
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