Propagation of strong electromagnetic waves in tenuous plasmas
Year: 2024
Type: article
Abstract: We study the propagation of electromagnetic waves in tenuous plasmas, where the wave frequency ω 0 is much larger than the plasma frequency ω P . We show that in pair plasmas, nonlinear effects are weak for a 0 ≪ ω 0 / ω P , where a 0 is the wave strength parameter. In electron-proton plasmas, a more restrictive condition must be satisfied, namely, either a 0 ≪ 1 / ω P τ 0 , where τ 0 is the duration of the radiation pulse, or a 0 ≪ 1 . We derive the equations that govern the evolution of the pulse in the weakly nonlinear regime. Our results have important implications for the modeling of fast radio bursts. We argue that (i) millisecond duration bursts with a smooth profile must be produced in a proton-free environment, where nonlinear effects are weaker, and (ii) propagation through an electron-proton plasma near the source can imprint a submicrosecond variability on the burst profile. Published by the American Physical Society 2024
Source: Physical Review Research
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $2,625
Awards: G1017154356, G1680718174, G2837684338, Collaborative Research: WoU-MMA: Multimessenger Plasma Physics Center (MPPC), Intrinsic dynamics of collisionless shocks and nonthermal particle acceleration, G518288856, THE INTERPLAY OF RECONNECTION AND TURBULENCE IN RELATIVISTIC PLASMAS: THE CASE OF BLACK HOLE ACCRETION FLOWS AND CORONAE, Standard Model and Cosmology of Fast Radio Bursts, 天体衝撃波における高強度コヒーレント放射についての数値的研究, G978507763
OpenAlex ID: W4404757329
