Axion Inflation: Perturbative control in the strong backreaction regime
Valerie Domcke, Alexandros Papageorgiou, Marco Peloso, Stefan Sandner
Abstract
We study the strong backreaction regime in axion inflation, in which the friction from Abelian gauge fields generated via the pseudo-scalar interaction β4 Mp ϕF F is comparable to Hubble friction. The non-linear dynamics associated with the gauge fields render this regime phenomenologically particularly interesting, but also notoriously difficult to study with perturbative methods. Quantifying the perturbative control through the direct impact on the spectral backreaction using (i) a first-order gradient-expansion formalism including axion gradients, and (ii) a one-loop in-in calculation, we discover an extended mild backreaction regime at large couplings β, with a relatively large, nearly constant particle production parameter ξ. In passing, we point out that CMB non-Gaussianity bounds impose a general upper limit on the product of axion gauge field coupling and Hubble parameter during inflation, βH/Mp < 1.4· 10-3, independently of the choice of the axion potential.
Create a lesson
Related papers
Follow-up of SN 2025wny VI: The Rate and Detectable Population of Strongly Lensed SLSNe-I in ZTF
Jacob O. Hjortlund, Edvard Mörtsell, Ariel Goobar et al.
Cosmological anatomy of interacting dark energy
Miguel A. Sabogal, Sunny Vagnozzi, Eleonora Di Valentino
Void probability function in the Quijote simulations
Snehasish Bhattacharjee
Constraints of Big Bang Nucleosynthesis and Cosmological Observations on varying Higgs VEV
Hongrui Feng, Yudong Luo, Toshitaka Kajino et al.
Infrared Universality of Scalar Induced Gravitational Waves Beyond Second Order
Chen Yuan
Resolving 3 Exotic Hyperbolic-Umbilic Lensing Configurations in the "Cosmic Mantis": An Exploration of RXJ0437.1+0043 with JWST
Catherine Cerny, David J. Lagattuta, Keren Sharon et al.