Propagation of strong electromagnetic waves in tenuous plasmas

被引:1
作者
Sobacchi, Emanuele [1 ,2 ]
Iwamoto, Masanori [3 ,4 ]
Sironi, Lorenzo [5 ,6 ,7 ]
Piran, Tsvi [8 ]
机构
[1] Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy
[2] INAF Osservatorio Astron Brera, Via E Bianchi 46, I-23807 Merate, Italy
[3] Kyoto Univ, Yukawa Inst Theoret Phys, Kitashirakawa Oiwakecho,Sakyo Ku, Kyoto 6068502, Japan
[4] Kyushu Univ, Fac Engn Sci, 6-1 Kasuga koen, Kasuga, Fukuoka 8168580, Japan
[5] Columbia Univ, Dept Astron, 550 West 120th St, New York, NY 10027 USA
[6] Columbia Univ, Columbia Astrophys Lab, 550 West 120th St, New York, NY 10027 USA
[7] Flatiron Inst, Ctr Computat Astrophys, 162 Fifth Ave, New York, NY 10010 USA
[8] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel
来源
PHYSICAL REVIEW RESEARCH | 2024年 / 6卷 / 04期
关键词
INTENSE LASER-PULSES; GIANT FLARE; INDUCED SCATTERING; FILAMENTATION; MECHANISMS; RADIATION; ECLIPSE; RAMAN;
D O I
10.1103/PhysRevResearch.6.043213
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We study the propagation of electromagnetic waves in tenuous plasmas, where the wave frequency omega(0) is much larger than the plasma frequency omega(P). We show that in pair plasmas, nonlinear effects are weak for a(0) << omega(0)/omega(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/omega(P)tau(0), where tau( 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.
引用
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页数:7
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