Hamilton-Jacobi analysis of noncanonical inflation in gravity: Constraints from Planck/ACT data, and theoretical bounds
arXiv:2301.08319 · doi:10.1016/j.jheap.2025.100531
Abstract
The latest CMB data from ACT DR6, combined with Planck, DESI, and BICEP/Keck, indicate a slight upward shift in the scalar spectral index, placing several previously favored inflationary models under tension. We study an inflationary scenario within the framework of gravity, featuring a nonminimal matter-curvature coupling, where the inflaton is a noncanonical scalar field with a generalized kinetic energy. Using the Hamilton-Jacobi formalism, we express the Hubble parameter as a function of the scalar field and consider two forms of , a power-law and an exponential one, deriving the scalar spectral index and tensor-to-scalar ratio . Comparison with ACT DR6 allows us to explore the parameter space, showing that the power-law case is compatible with the data across a wide range, while the exponential form requires a large number of e-folds. We then study reheating, noting its close link with the inflationary dynamics. By imposing the bound on overproduction of primordial gravitational waves encoded in the constraint on , we obtain a lower limit on the reheating temperature, which becomes particularly restrictive for the stiff reheating equation of state . This bound implies that the total number of e-folds should not exceed . The predicted gravitational-wave spectrum shows an enhanced high-frequency amplitude, potentially observable by future detectors. We also examine consistency with the Swampland conjectures and the Trans-Planckian Censorship Conjecture, finding that combining gravity with noncanonical dynamics provides a rich and testable framework for the early universe.
arXiv comment22 pages, 11 figures, 4 tables
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