Dynamics of Peccei-Quinn Breaking Field after Inflation and Axion Isocurvature Perturbations
Keisuke Harigaya, Masahiro Ibe, Masahiro Kawasaki, Tsutomu T. Yanagida

TL;DR
This paper investigates the post-inflation dynamics of the Peccei-Quinn field, addressing isocurvature perturbations and proposing a model that prevents domain wall formation through suppressed parametric resonance.
Contribution
It introduces a novel model where parametric resonance is suppressed, avoiding domain wall formation and aligning with supersymmetric theories.
Findings
Proposes a model with suppressed parametric resonance.
Ensures consistency with supersymmetric theories.
Addresses isocurvature perturbation suppression.
Abstract
The Peccei-Quinn mechanism suffers from the problem of the isocurvature perturbations. The isocurvature perturbations are suppressed if the Peccei-Quinn breaking scale is large during inflation. The oscillation of the Peccei-Quinn breaking field after inflation, however, leads to the formation of domain walls due to the parametric resonance effect. In this paper, we discuss the evolution of the Peccei-Quinn breaking field after inflation in detail, and propose a model where the parametric resonance is ineffective and hence domain walls are not formed. We also discuss consistency of our model with supersymmetric theory.
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