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.
Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season,
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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.