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curve, is allowed within an order of magnitude below m$_{0}$ ∼ 10 3 GeV. The values of f$_{NL}$ and g$_{NL}$ for a thermal waterfall field mass of m$_{0}$ ∼ 10 3 GeV are shown in Table 4.4, with them both being within current observational bounds [55]. 

n$_{s}$ and n ′ $_{s}$: Chaotic Inflation 

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We provide results for the spectral index and its running when the period of 

