Low-frequency nonlinear ion-acoustic cnoidal waves in a superthermal plasma with a monoenergetic electron beam

被引:6
|
作者
El-Tantawy, S. A. [1 ,2 ]
Khalid, Muhammad [3 ]
Kabir, Abdul [4 ]
Hussain, Akram A. [5 ,6 ]
Alrowaily, Albandari W. [7 ]
Tiofack, C. G. L. [8 ]
机构
[1] Port Said Univ, Fac Sci, Dept Phys, Port Said 42521, Egypt
[2] Al Baha Univ, Fac Sci & Arts, Res Ctr Phys RCP, Dept Phys, Al Baha 1988, Saudi Arabia
[3] Govt Post Grad Coll Swabi, Dept Phys, Khyber Pakhtunkhwa 23431, Pakistan
[4] Inst Space Technol, GNSS Res Lab Natl Ctr GIS & Space Applicat, Dept Space Sci, Islamabad 44000, Pakistan
[5] Zagazig Univ, Fac Sci, Biol Dept, Zagazig, Egypt
[6] Al Baha Univ, Fac Sci & Arts, Biol Dept, Al Baha 1988, Saudi Arabia
[7] Princess Nourah Bint Abdulrahman Univ, Coll Sci, Dept Phys, POB 84428, Riyadh 11671, Saudi Arabia
[8] Univ Maroua, Fac Sci, POB 814, Maroua, Cameroon
关键词
SOLITARY; GENERATION;
D O I
10.1063/5.0174386
中图分类号
TB3 [工程材料学];
学科分类号
0805 ; 080502 ;
摘要
This study analyzes the behavior of nonlinear electrostatic ion-acoustic cnoidal waves (IACWs) in a magnetoplasma characterized by two distinct temperatures of superthermal electrons and a monoenergetic electron beam. For this purpose and based on fluid theory, the reductive perturbation technique is applied to reduce the basic equations to a third-order Korteweg-de Vries (KdV) equation. Under certain conditions, the KdV equation can be used for modeling symmetric CWs; when these conditions are not met, it is replaced by a Kawahara equation to describe these waves correctly. The symmetric IACWs features are examined in detail to determine the effect of pertinent plasma parameters. This study may help model nonlinear structures in astrophysical and space plasmas and understand the mechanism of CWs in the plasma sheath region.
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页数:6
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