Dispersion relations for electromagnetic waves in a dense magnetized plasma

被引:17
|
作者
Shukla, P. K. [1 ,2 ,3 ,4 ,5 ,6 ,7 ,10 ]
Stenflo, L. [8 ,9 ]
机构
[1] Univ KwaZulu Natal, Sch Phys, ZA-400 Durban, South Africa
[2] Ruhr Univ Bochum, Ctr Plasma Sci & Astrophys, D-44780 Bochum, Germany
[3] Umea Univ, Dept Phys, SE-90187 Umea, Sweden
[4] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[5] Univ Tecn Lisboa, Inst Super Tecn, Inst Plasma & Fusao Nucl, Grp Lasers & Plasmas, P-1049001 Lisbon, Portugal
[6] Ctr Fundamental Phys, Rutherford Appleton Lab, CCLRC, Didcot OX11 0QX, Oxon, England
[7] Univ Strathclyde, SUPA, Dept Phys, Glasgow G 40NG, Lanark, Scotland
[8] Umea Univ, Dept Phys, SE-90187 Umea, Sweden
[9] Linkoping Univ, Dept Phys, SE-58183 Linkoping, Sweden
[10] Ruhr Univ Bochum, Fak Phys & Astron, Inst Theoret Phys 4, Nonlinear Phys Ctr, D-44780 Bochum, Germany
关键词
D O I
10.1017/S0022377808007344
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
Dispersion relations for elliptically polarized extraordinary is well as linearly polarized ordinary, electromagnetic waves propagating across an external magnetic hold in a dense magnetoplasma are derived, taking into account the combined effects of the quantum electrodynamical (QED) field, as well as the quantum forces associated with the Bohm potential and the magnetization energy, of Me electrons due to the electron-1/2 spin effect. QED (vacuum polarization) effects, which contribute to the nonlinear electron current density, modify the refractive index. Our results concern the propagation characteristics of perpendicularly propagating high-frequency electromagnetic waves in dense astrophysical objects (e.g. neutron sows and magnetars), as well as the next-generation intense laser-solid density plasma interaction experiments and quantum free-electron laser schemes.
引用
收藏
页码:719 / 723
页数:5
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