journal article·2021-08-01Open access

Small amplitude ion-acoustic solitons with regularized κ-distributed electrons

F. F. Lu, S. Q. Liu

AIP Advances· Volume 11· Issue 8

Abstract

A theoretical investigation of ion-acoustic solitons in an unmagnetized plasma consisting of cold ions and regularized κ-distributed electrons has been carried out. The properties of stationary solitary structures are briefly studied by the reductive perturbation method in the small amplitude limit. It is found that in the small κ region, the ion-acoustic solitary waves propagate more slowly in the case of regularized κ distribution than in the case of standard κ distribution. The regularized κ-distributed electrons affect the width and amplitude of the solitary waves. As the cutoff parameter α increases, the amplitudes of both the compressive and rarefactive solitary waves decrease, and their widths also decrease. In addition, for a given value of κ, positive potential solitons will appear at large α, while negative potential solitons will appear at small α. The results of this paper may be useful for understanding nonlinear electrostatic phenomena in space plasmas.
Source: crossref · Quality: baseline

Research context

OpenAlex topics: Dust and Plasma Wave Phenomena · Ionosphere and magnetosphere dynamics

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Jiangxi Province Key Laboratory of Fusion and Information Control, Department of Physics, Nanchang University 1 , Nanchang 330031, China

School of Materials Science and Engineering, Nanchang University 2 , Nanchang 330031, China

NCU-ASIPP Magnetic Confinement Fusion Joint Lab, Institute of Fusion Energy and Plasma Application, Nanchang University 3 , Nanchang 330031, China

Funding

National Natural Science Foundation of China · Jiangxi Provincial Key Laboratory of Fusion and Information Control · Project of Scientific and Technological Innovation Base of Jiangxi Province

References (26)

Show source-provided references
1. 1966
2. Phys. Rev. Lett. · 1966 · 17 · 99610.1103/physrevlett.17.996 ↗
3. Phys. Rev. Lett. · 1970 · 25 · 1110.1103/physrevlett.25.11 ↗
4. Phys. Plasmas · 2003 · 10 · 161910.1063/1.1557071 ↗
5. Astrophys. Space Sci. · 2013 · 344 · 13510.1007/s10509-012-1309-x ↗
6. New J. Phys. · 2003 · 5 · 2810.1088/1367-2630/5/1/328 ↗
7. Phys. Plasmas · 2018 · 25 · 02211310.1063/1.5018228 ↗
8. Phys. Lett. A · 2014 · 378 · 352310.1016/j.physleta.2014.10.006 ↗
9. Phys. Lett. A · 2019 · 383 · 12584010.1016/j.physleta.2019.125840 ↗
10. Phys. Plasmas · 1995 · 2 · 71610.1063/1.871422 ↗
11. Phys. Rev. E · 1997 · 55 · 185210.1103/physreve.55.1852 ↗
12. Phys. Plasmas · 2009 · 16 · 06290310.1063/1.3143036 ↗
13. Phys. Plasmas · 2006 · 13 · 01230410.1063/1.2158148 ↗
14. Plasma Phys. Controlled Fusion · 2011 · 53 · 02500410.1088/0741-3335/53/2/025004 ↗
15. J. Geophys. Res. · 1968 · 73 · 283910.1029/ja073i009p02839 ↗
16. Astron. Astrophys. · 1997 · 324 · 72510.1086/118520 ↗
17. Phys. Plasmas · 2008 · 15 · 12370510.1063/1.3042215 ↗
18. Astron. Astrophys. · 2015 · 582 · A12410.1051/0004-6361/201526509 ↗
19. Phys. Plasmas · 2012 · 19 · 01230310.1063/1.3675875 ↗
20. Phys. Plasmas · 2010 · 17 · 12231410.1063/1.3528544 ↗
21. Phys. Plasmas · 2010 · 17 · 11230510.1063/1.3503664 ↗
22. Phys. Plasmas · 2011 · 18 · 09290110.1063/1.3629981 ↗
23. Adv. Space Res. · 2014 · 53 · 84510.1016/j.asr.2014.01.003 ↗
24. Europhys. Lett. · 2017 · 120 · 5000210.1209/0295-5075/120/50002 ↗
25. AIP Adv. · 2020 · 10 · 08502210.1063/5.0020345 ↗
26. Eur. Phys. J. D · 2000 · 11 · 14310.1007/s100530050017 ↗