The paper derives potentials V = Λ²|f⁻¹(u_R/√2)|² from K = K₋(f(T)) and W = ΛST, and scans M and p to match Planck data with hilltop, Starobinsky-like, plateau, log-squared, and bell-curve shapes.
First Order Phase Transition of a Vacuum and Expansion of the Universe
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Inflation in supergravity from field redefinitions
The paper derives potentials V = Λ²|f⁻¹(u_R/√2)|² from K = K₋(f(T)) and W = ΛST, and scans M and p to match Planck data with hilltop, Starobinsky-like, plateau, log-squared, and bell-curve shapes.