In Bianchi-I mLQC-I, the apparent isotropization is an emergent Planckian de Sitter phase that leaves the post-bounce universe non-classical, and it fails for vacuum and selected perfect-fluid initial conditions.
The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems
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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.
In Gauss-Bonnet inflation with monomial potential and coupling, gravitational waves from preheating produce a present-day energy density spectrum consistent with Planck constraints when the coupling strength, equation of state, and efficiency are set to specific values.
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The Steep Price of No Hair in a Modified Loop Quantum Cosmology
In Bianchi-I mLQC-I, the apparent isotropization is an emergent Planckian de Sitter phase that leaves the post-bounce universe non-classical, and it fails for vacuum and selected perfect-fluid initial conditions.
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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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Gravitational waves production during preheating within GB gravity with monomial coupling
In Gauss-Bonnet inflation with monomial potential and coupling, gravitational waves from preheating produce a present-day energy density spectrum consistent with Planck constraints when the coupling strength, equation of state, and efficiency are set to specific values.