Magnetized current filaments as a source of circularly polarized light

被引:0
作者
Sinha, U. [1 ,2 ]
Schoeffler, K. M. [1 ]
Martins, J. [1 ]
Vieira, J. [1 ]
Fonseca, R. A. [1 ,3 ]
Silva, L. O. [1 ]
机构
[1] Univ Lisbon, GoLP, Inst Plasmas & Fus Nucl, Inst Super Tecn, P-1049001 Lisbon, Portugal
[2] Forschungszentrum Julich, Inst Adv Simulat, Julich Supercomp Ctr, D-52425 Julich, Germany
[3] Univ Lisbon, DCTI, ISCTE, P-1649026 Lisbon, Portugal
基金
欧洲研究理事会;
关键词
astrophysical plasmas; PARTICLE-ACCELERATION; WEIBEL INSTABILITY; PLASMA; FIELD; AFTERGLOW; GENERATION; SHOCKS;
D O I
10.1017/S0022377821000040
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We show that the Weibel or current filamentation instability can lead to the emission of circularly polarized radiation. Using particle-in-cell simulations and a radiation post-processing numerical algorithm, we demonstrate that the level of circular polarization increases with the initial plasma magnetization, saturating at similar to 13% when the magnetization, given by the ratio of magnetic energy density to the electron kinetic energy density, is larger than 0.05. Furthermore, we show that this effect requires an ion-electron mass ratio greater than unity. These findings, which could also be tested in currently available laboratory conditions, show that the recent observation of circular polarization in gamma-ray burst afterglows could be attributed to the presence of magnetized current filaments driven by the Weibel or current filamentation instability.
引用
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页数:13
相关论文
共 40 条
[1]   Transverse electron-scale instability in relativistic shear flows [J].
Alves, E. P. ;
Grismayer, T. ;
Fonseca, R. A. ;
Silva, L. O. .
PHYSICAL REVIEW E, 2015, 92 (02)
[2]   LARGE-SCALE MAGNETIC FIELD GENERATION VIA THE KINETIC KELVIN-HELMHOLTZ INSTABILITY IN UNMAGNETIZED SCENARIOS [J].
Alves, E. P. ;
Grismayer, T. ;
Martins, S. F. ;
Fiuza, F. ;
Fonseca, R. A. ;
Silva, L. O. .
ASTROPHYSICAL JOURNAL LETTERS, 2012, 746 (02)
[3]  
[Anonymous], 2012, Classical Electrodynamics
[4]   Radio polarization maps of shell-type supernova remnants - I. Effects of a random magnetic field component and thin-shell models [J].
Bandiera, R. ;
Petruk, O. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 459 (01) :178-198
[5]   Electron acceleration in laboratory-produced turbulent collisionless shocks [J].
Fiuza, F. ;
Swadling, G. F. ;
Grassi, A. ;
Rinderknecht, H. G. ;
Higginson, D. P. ;
Ryutov, D. D. ;
Bruulsema, C. ;
Drake, R. P. ;
Funk, S. ;
Glenzer, S. ;
Gregori, G. ;
Li, C. K. ;
Pollock, B. B. ;
Remington, B. A. ;
Ross, J. S. ;
Rozmus, W. ;
Sakawa, Y. ;
Spitkovsky, A. ;
Wilks, S. ;
Park, H-S .
NATURE PHYSICS, 2020, 16 (09) :916-+
[6]   Weibel-Instability-Mediated Collisionless Shocks in the Laboratory with Ultraintense Lasers [J].
Fiuza, F. ;
Fonseca, R. A. ;
Tonge, J. ;
Mori, W. B. ;
Silva, L. O. .
PHYSICAL REVIEW LETTERS, 2012, 108 (23)
[7]   Exploiting multi-scale parallelism for large scale numerical modelling of laser wakefield accelerators [J].
Fonseca, R. A. ;
Vieira, J. ;
Fiuza, F. ;
Davidson, A. ;
Tsung, F. S. ;
Mori, W. B. ;
Silva, L. O. .
PLASMA PHYSICS AND CONTROLLED FUSION, 2013, 55 (12)
[8]  
Fonseca RA, 2002, LECT NOTES COMPUT SC, V2331, P342
[9]   Filamentation Instability of Counterstreaming Laser-Driven Plasmas [J].
Fox, W. ;
Fiksel, G. ;
Bhattacharjee, A. ;
Chang, P. -Y. ;
Germaschewski, K. ;
Hu, S. X. ;
Nilson, P. M. .
PHYSICAL REVIEW LETTERS, 2013, 111 (22)
[10]   Gamma-ray burst afterglow: Polarization and analytic light curves [J].
Gruzinov, A ;
Waxman, E .
ASTROPHYSICAL JOURNAL, 1999, 511 (02) :852-861