Pure low-temperature dissipation dominates warm Higgs inflation fits with n_s ≈ 0.965 and r ≈ 3.7×10^{-3}, while pure high-temperature is displaced and some multi-channel models fall below the warm threshold.
Early Universe Higgs dynamics in the presence of the Higgs-inflaton and non-minimal Higgs-gravity couplings,
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Comparison of Effective Dissipation Channels in Warm Higgs Inflation from Warm Background Evolution
Pure low-temperature dissipation dominates warm Higgs inflation fits with n_s ≈ 0.965 and r ≈ 3.7×10^{-3}, while pure high-temperature is displaced and some multi-channel models fall below the warm threshold.