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.
Quantum Fluctuations and a Nonsingular Universe,
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Dyson-Schwinger methods applied to gravity theories produce conformally flat metrics and a sequence of cosmological phase transitions from conformal symmetry breaking that non-minimal scalar couplings can suppress.
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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.
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Review of strongly coupled regimes in gravity with Dyson-Schwinger approach
Dyson-Schwinger methods applied to gravity theories produce conformally flat metrics and a sequence of cosmological phase transitions from conformal symmetry breaking that non-minimal scalar couplings can suppress.