日本地球惑星科学連合2025年大会

講演情報

[J] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM17] 宇宙プラズマ科学

2025年5月27日(火) 09:00 〜 10:30 303 (幕張メッセ国際会議場)

コンビーナ:天野 孝伸(東京大学 地球惑星科学専攻)、三宅 洋平(神戸大学大学院システム情報学研究科)、諌山 翔伍(九州大学総合理工学研究院)、梅田 隆行(北海道大学 情報基盤センター)、座長:天野 孝伸(東京大学 地球惑星科学専攻)、岩本 昌倫(京都大学基礎物理学研究所)

10:15 〜 10:30

[PEM17-06] 電子・陽電子プラズマにおける高強度電磁波の伝搬

*岩本 昌倫1、井岡 邦仁1 (1.京都大学基礎物理学研究所)

キーワード:プラズマ波、パラメトリック不安定

Intence electromagnetic waves are subject to the nonlinear wave–plasma interactions, such as parametric instability, which has been widely studied in laboratory plasmas using cutting-edge laser pulses. Recently, the nonlinear interaction has attracted attention from astrophysics in the context of Fast Radio Bursts (FRBs). FRBs are extremely bright millisecond-duration pulses at radio frequency (Lorimer et al. 2007) and often show a high degree of linear polarization (e.g., Michilli et al. 2018). Magnetars are one of the promising progenitors (e.g., Andersen et al. 2020; Lyubarsky 2021) and thus the FRB radio pulse propagates through the magnetar wind, which consists of electron–positron plasmas. The nonlinear wave–plasma interaction between linearly polarized electromagnetic waves and electron–positron plasmas must be considered for the propagation of FRB radio pulses. In this study, we analytically derive the steady-state solution of the linearly polarized electromagnetic waves in cold pair plasmas for arbitrary wave amplitude and frequency. We will demonstrate the time evolution of the steady-state solution by using the particle-in-cell simulations and discuss the effect of the non-linear wave–plasma on the propagation of FRB radio pulses.