The onset of the strong backreaction regime in axion inflation, an analytical study
astro-ph.CO, hep-ph, hep-th
Submitted: 2026-08-29
Updated: 2026-10-17
Sources
- A Natural Framework for Chaotic Inflation
- Completing Natural Inflation
- Trajectories with suppressed tensor-to-scalar ratio in Aligned Natural Inflation
- Monodromy inflation at strong coupling: $4\pi$ in the sky
- Strongly Coupled Quintessence
- Leptogenesis from left-handed neutrino production during axion inflation
- Fermion production during and after axion inflation
- Phenomenology of fermion production during axion inflation
- Gauge Field and Fermion Production during Axion Inflation
- Gravitational waves from fermion production during axion inflation
- Reviving chaotic inflation with fermion production: a supergravity model
- Spectra of fermions produced by a time-dependent axion in the radiation- and matter-dominated Universe
- Chromo-Natural Inflation: Natural inflation on a steep potential with classical non-Abelian gauge fields
- Emerging chromo-natural inflation
- Gravity waves and non-Gaussian features from particle production in a sector gravitationally coupled to the inflaton
- Scale-dependent gravitational waves from a rolling axion
- N-flationary magnetic fields
- Primordial magnetic fields from pseudo-Goldstone bosons
- Magnetogenesis from axion inflation
- Backreaction of electromagnetic fields and the Schwinger effect in pseudoscalar inflation magnetogenesis
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation