Abstract

We investigate the dependency of Higgs inflation on the non-renormalisable matching between the low energy Standard Model limit and the inflationary regime at high energies. We show that for the top mass range mt≳171.8m_t \gtrsim 171.8 GeV the scenario robustly predicts the spectral index ns≃0.97n_s \simeq 0.97 and the tensor-to-scalar ratio r≃0.003r\simeq 0.003. The matching is however non-trivial, even the best-fit values mh=125.09m_h=125.09 GeV and mt=173.21m_t=173.21 GeV require a jump δλ∼0.01δλ\sim 0.01 in the Higgs coupling below the inflationary scale. For mt≲171.8m_t\lesssim 171.8 GeV, the matching may generate a feature in the inflationary potential. In this case the predicted values of nsn_s and rr vary but the model is still falsifiable. For example, a detection of negative running of spectral index at level αs≲−0.01α_s \lesssim -0.01 would rule out Higgs inflation.

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