Abstract
We study the general relation between the power spectrum and the squeezed limit of the bispectrum of the comoving curvature perturbation produced during single-field slow-roll inflation when the initial state is a general vacuum. Assuming the scale invariance of the power spectrum, we derive a formula for the squeezed limit of the bispectrum, represented by the parameter fNL, which is not slow-roll suppressed and is found to contain a single free parameter for a given amplitude of the power spectrum. Then, we derive the conditions for achieving a scale-invariant fNL and discuss a few examples.
Original language | English |
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Article number | 095005 |
Journal | Classical and Quantum Gravity |
Volume | 30 |
Issue number | 9 |
DOIs | |
State | Published - 7 May 2013 |