Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation

Sep, 2009
5 pages
Published in:
  • Phys.Rev.D 81 (2010) 063511
e-Print:
Report number:
  • MIT-CTP-4071

Citations per year

200920132017202120250510152025
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