Primordial Non-Gaussianities from Inflation Models

Figure 9

Numerical result (solid line) of the bispectrum running for the example (151) (𝑚=3×10⁻⁶𝑀_P,𝑐=5×10⁻⁷,Λ=0.0007𝑀_P,𝜙≈15𝑀_P), compared with the ansatz (148) (dashed line).