English

Dilaton-Flattened Axion Inflation

High Energy Physics - Phenomenology 2026-04-23 v2 General Relativity and Quantum Cosmology

Abstract

We present a solvable same-sector effective theory for anomaly-inspired axion inflation, in which a heavy trace-anomaly mode dynamically backreacts on the axion potential. The tree-level elimination of the radial field resums the backreaction into a closed-form Lambert-WW potential, naturally flattening the hilltop potential without external plateau operators. By deriving the exact trough metric, we evaluate all the observables on the fully reduced one-field action, bypassing uncontrolled kinetic approximations. Calibrated at N=56N_\star=56, reheating-compatible branches yield r0.033r\simeq0.033--0.0360.036 and αs(4.6\alpha_s\simeq-(4.6--4.7)×1044.7)\times10^{-4}, comfortably satisfying the current ACT/SPT/BICEP constraints. The evolution remains strictly adiabatic (m2/H26.1m_\perp^2/H^2\gtrsim6.1, Ω/H7.6×104\Omega/H\lesssim7.6\times10^{-4}) with negligible sound-speed and metric corrections. We provide analytic control over the constant-weffw_{\rm eff} reheating map, the Nre=0N_{\rm re}=0 boundary, and robustness against vacuum-offset deformations. This Lambert-WW backbone establishes a precise, deformable benchmark for confining axion inflation, with microscopic matching and reheating microphysics accessible as systematic EFT refinements.

Keywords

Cite

@article{arxiv.2604.15194,
  title  = {Dilaton-Flattened Axion Inflation},
  author = {Pirzada and Ali Muhammad and Tianjun Li and Imtiaz Khan and Mussawir Khan},
  journal= {arXiv preprint arXiv:2604.15194},
  year   = {2026}
}

Comments

13,13 any comments are welcome

R2 v1 2026-07-01T12:12:57.925Z