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Induced Scattering of Strong Waves in Pair Plasmas

High Energy Astrophysical Phenomena 2026-04-20 v1 Plasma Physics

Abstract

We study induced (stimulated) scattering of linearly polarized, strong electromagnetic waves in pair plasmas, which is crucial for understanding the propagation of fast radio bursts (FRBs). Magnetars are the most promising progenitors of FRBs, and FRBs propagate through the magnetar wind and successfully escape before being significantly scattered. We revisit the steady-state solution of linearly polarized electromagnetic waves in pair plasmas with arbitrary amplitude, and demonstrate that the nonlinearity is characterized by the nonlinearity parameter a0ωpe/ω0a_0\omega_{pe}/\omega_0 rather than the dimensionless amplitude a0a_0, where ωpe\omega_{pe} is the electron plasma frequency and ω0\omega_0 is the wave frequency. We follow the time evolution of the steady-state solution for the linear regime a0ωpe/ω01a_0\omega_{pe}/\omega_0 \ll 1 by performing one-dimensional particle-in-cell simulations, and show that the conventional linear analysis of induced scattering assuming a01a_0 \ll 1 is applicable even for a0>1a_0 > 1 when the Lorentz boost due to the plasma motion in the incident wave is considered. The saturation level is controlled by a0ω0/ωpea_0\omega_0/\omega_{pe}, which corresponds to the ratio of the wave energy to the plasma energy, and the incident wave is hardly scattered for a0ω0/ωpe1a_0\omega_0/\omega_{pe} \gg 1. We discuss the application of our results to FRBs.

Keywords

Cite

@article{arxiv.2604.15798,
  title  = {Induced Scattering of Strong Waves in Pair Plasmas},
  author = {Masanori Iwamoto and Kunihito Ioka},
  journal= {arXiv preprint arXiv:2604.15798},
  year   = {2026}
}

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