Primordial Non-Gaussianities from Inflation Models

Figure 14

Numerical results for the shapes of bispectra with intermediate forms. We plot 𝑆 with 𝜈=0,0.3,0.5,1. The plot is normalized such that 𝑆=1 for 𝑝₁=𝑝₂=𝑝₃.

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