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For intermediate inflation, where the cosmological scale factor expands as: $a(t)=a_0\\exp(At^f)$ ($A>0, 0<f<1$), $N\\geq 100$ cases lead to $0.02<r<0.11$ ($r$ is tensor-scalar ratio) and $N\\simeq50 $ case leads to $n_s\\simeq 0.96$ ($n_s$ is spectral index). 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