Solitary waves and double layers in complex plasma media

被引:10
作者
Mamun, A. A. [1 ,3 ]
Mannan, Abdul [1 ,2 ]
机构
[1] Jahangirnagar Univ, Dept Phys, Dhaka, Bangladesh
[2] Martin Luther Univ Halle Wittenberg, Inst Math, Halle, Germany
[3] Jahangirnagar Univ, Wazed Miah Sci Res Ctr, Dhaka, Bangladesh
关键词
Positive dust; non-thermal electrons; subsonic and supersonic SWs; double layers; INDUCED COULOMB CRYSTALLIZATION; CHARGED DUST; SOLAR-RADIATION; GRAINS; PARTICLES; DYNAMICS; JUPITER;
D O I
10.1080/17455030.2021.1936285
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A complex plasma medium (containing Cairns nonthermal electron, adiabatically warm inertial ion, and stationary positively charged dust (PCD) species (making a plasma system very complex) is considered. The effects of PCD species, nonthermal electron species, and adiabatic ion-temperature on ion-acoustic (IA) solitary waves (SWs) and double layers (DLs) are investigated by the pseudo-potential approach, which is valid for the arbitrary amplitude time-independent SWs and DLs. It is observed that the presence of the PCD species reduces the phase speed of the IA waves, and consequently supports the IA subsonic compressive SWs in electron-ion-PCD plasmas. On the other hand, the increase in both adiabatic ion-temperature and the number of nonthermal or fast electrons causes to reduce the possibility for the formation of subsonic SWs, and thus convert subsonic SWs into supersonic ones. It is observed that after at a certain value of the nonthermal parameter, the IA supersonic SWs with both positive and negative potentials as well as DLs with only negative potential exist. The applications of the work in space environments (viz. Earth's mesosphere, cometary tails, Jupiter's magnetosphere, etc.) and laboratory devices, where warm ion and nonthermal electron species along with PCD species have been observed, are briefly discussed.
引用
收藏
页码:1319 / 1330
页数:12
相关论文
共 27 条
[1]   EXACT NONLINEAR PLASMA OSCILLATIONS [J].
BERNSTEIN, IB ;
GREENE, JM ;
KRUSKAL, MD .
PHYSICAL REVIEW, 1957, 108 (03) :546-550
[2]   ELECTROSTATIC SOLITARY STRUCTURES IN NONTHERMAL PLASMAS [J].
CAIRNS, RA ;
MAMUM, AA ;
BINGHAM, R ;
BOSTROM, R ;
DENDY, RO ;
NAIRN, CMC ;
SHUKLA, PK .
GEOPHYSICAL RESEARCH LETTERS, 1995, 22 (20) :2709-2712
[3]   ROLE OF GRAIN-SIZE AND PARTICLE-VELOCITY DISTRIBUTION IN SECONDARY-ELECTRON EMISSION IN-SPACE PLASMAS [J].
CHOW, VW ;
MENDIS, DA ;
ROSENBERG, M .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1993, 98 (A11) :19065-19076
[4]   Chemical model for positively charged dust particles [J].
Davletov, A. E. ;
Kurbanov, F. ;
Mukhametkarimov, Ye. S. .
PHYSICS OF PLASMAS, 2018, 25 (12)
[5]   Large-amplitude dust-ion acoustic solitary waves in a dusty plasma with nonthermal electrons [J].
El-Labany, S. K. ;
El-Taibany, W. F. ;
El-Fayoumy, M. M. .
ASTROPHYSICS AND SPACE SCIENCE, 2012, 341 (02) :527-534
[6]   Dynamics of ion-acoustic waves in nonrelativistic magnetized multi-ion quantum plasma: the role of trapped electrons [J].
El-Monier, S. Y. ;
Atteya, A. .
WAVES IN RANDOM AND COMPLEX MEDIA, 2022, 32 (01) :299-317
[7]   Finite amplitude solitary excitations in rotating magnetized nonthermal complex (dusty) plasmas [J].
El-Taibany, W. F. ;
Mushtaq, A. ;
Moslem, W. M. ;
Wadati, Miki .
PHYSICS OF PLASMAS, 2010, 17 (03)
[8]   Sagdeev potential analysis for positively charged dust grains in nonthermal dusty plasma near Mars [J].
El-Taibany, W. F. ;
Wadati, Miki .
PHYSICS OF PLASMAS, 2007, 14 (10)
[9]   Dusty plasma induced by solar radiation under microgravitational conditions: an experiment on board the Mir orbiting space station [J].
Fortov, VE ;
Nefedov, AP ;
Vaulina, OS ;
Lipaev, AM ;
Molotkov, VI ;
Samaryan, AA ;
Nikitski, VP ;
Ivanov, AI ;
Savin, SF ;
Kalmykov, AV ;
Solov'ev, AY ;
Vinogradov, PV .
JOURNAL OF EXPERIMENTAL AND THEORETICAL PHYSICS, 1998, 87 (06) :1087-1097
[10]   Dynamics of dust grains in an electron-dust plasma induced by solar radiation under microgravity conditions [J].
Fortov, VE ;
Nefedov, AP ;
Vaulina, OS ;
Petrov, OF ;
Dranzhevski, IE ;
Lipaev, AM ;
Semenov, YP .
NEW JOURNAL OF PHYSICS, 2003, 5 :102.1-102.17