Domain Wall as Cosmological Oscillator
Bo-Qiang Lu
TL;DR
This work recasts cosmological domain walls as oscillators driven by a periodic background field, deriving a collective-coordinate equation for wall displacement with natural frequency $\omega_0$ and damping $\gamma$. It analyzes both $Z_2$-breaking and $Z_2$-conserving interactions, showing that resonant forcing $\omega\approx\omega_0$ can amplify wall oscillations to a universal critical deformation and trigger rupture, thereby resolving the domain-wall problem in a broad class of models. The analysis employs a perturbative expansion around the static wall, a collective-coordinate projection, and, in the $Z_2$-conserving case, a Mathieu–Floquet framework to map stability regions and resonance tongues. The results highlight the roles of Hubble damping, radiation damping, and elastic-energy balance in determining the viability and timing of resonant destruction, with implications for early-universe cosmology and potential gravitational-wave signals.
Abstract
In this study, we examine the domain wall within the framework of a cosmological harmonic oscillator. We investigate the interaction between the domain wall and a periodic background field, which can induce perturbations in the oscillatory behavior of the wall. We propose a novel mechanism for resolving the domain wall problem through the phenomenon of resonant oscillation. Resonant oscillation occurs when the frequency of the external driving force aligns with the intrinsic frequency of the domain wall. This synchrony can significantly amplify the amplitude of the oscillation. If the amplitude of oscillation exceeds a predetermined critical deformation threshold, the domain wall may be deconstructed. Furthermore, we demonstrate that this mechanism remains valid in models that preserve discrete symmetry.
