ION ACOUSTIC SOLITONS IN DENSE MAGNETIZED PLASMAS WITH NONRELATIVISTIC AND ULTRARELATIVISTIC DEGENERATE ELECTRONS AND POSITRONS

被引:30
|
作者
Sadiq, Safeer [1 ]
Mahmood, S. [1 ,2 ]
Haque, Q. [1 ]
Ali, Munazza Zulfiqar [3 ]
机构
[1] PINSTECH, Div Theoret Phys, Islamabad 44000, Pakistan
[2] Univ Fed Rio Grande do Sul, Inst Phys, BR-91505197 Porto Alegre, RS, Brazil
[3] Univ Punjab, Dept Phys, Lahore 54000, Pakistan
来源
ASTROPHYSICAL JOURNAL | 2014年 / 793卷 / 01期
关键词
plasmas; pulsars: general; stars: atmospheres; waves; PULSAR MAGNETOSPHERE; RELATIVISTIC PLASMAS; GALACTIC-CENTER; DRIFT WAVES; STARS; EMISSION; PHYSICS; MAGNETARS; CORONA;
D O I
10.1088/0004-637X/793/1/27
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The propagation of electrostatic waves in a dense magnetized electron-positron-ion (EPI) plasma with nonrelativistic and ultrarelativistic degenerate electrons and positrons is investigated. The linear dispersion relation is obtained for slow and fast electrostatic waves in the EPI plasma. The limiting cases for ion acoustic wave (slow) and ion cyclotron wave (fast) are also discussed. Using the reductive perturbation method, two-dimensional propagation of ion acoustic solitons is found for both the nonrelativistic and ultrarelativistic degenerate electrons and positrons. The effects of positron concentration, magnetic field, and mass of ions on ion acoustic solitons are shown in numerical plots. The proper form of Fermi temperature for nonrelativistic and ultrarelativistic degenerate electrons and positrons is employed, which has not been used in earlier published work. The present investigation is useful for the understanding of linear and nonlinear electrostatic wave propagation in the dense magnetized EPI plasma of compact stars. For illustration purposes, we have applied our results to a pulsar magnetosphere.
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页数:12
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