2012
DOI: 10.1007/s10509-012-1221-4
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Nonplanar ion-acoustic Gardner solitons in a pair-ion plasma with nonextensive electrons and positrons

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Cited by 39 publications
(22 citation statements)
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“…planetary rings, solar winds (Kopp et al 1997), stellar polytropes (Plastino and Plastino 1993), quark-gluon plasma (Gervino et al 2012), etc. Ghosh et al (2013) studied the IA GSs in e-p-i plasma composed of nonextensive distributed electrons and positrons, and inertial ions. El-Awady and Moslem (2011) investigated the formation of solitary and rogue waves in the nonextensive e-p-i plasmas and pointed out that the growth or damping of the rogue wave depends on the value of the q-nonextensive parameter.…”
Section: Introductionmentioning
confidence: 99%
“…planetary rings, solar winds (Kopp et al 1997), stellar polytropes (Plastino and Plastino 1993), quark-gluon plasma (Gervino et al 2012), etc. Ghosh et al (2013) studied the IA GSs in e-p-i plasma composed of nonextensive distributed electrons and positrons, and inertial ions. El-Awady and Moslem (2011) investigated the formation of solitary and rogue waves in the nonextensive e-p-i plasmas and pointed out that the growth or damping of the rogue wave depends on the value of the q-nonextensive parameter.…”
Section: Introductionmentioning
confidence: 99%
“…We well know that a number of authors have used this assumption in the literature, but unfortunately that does not make it generally correct, at least not without keeping several limitations in mind. Several authors [16][17][18][19][20][21][22][23][24][25][26][27][28][29][30][31][32][33][34][35] introduce the stretching (4) with a reference to papers by Maxon and Viecelli, 12,13 without mentioning any of the restrictions about its applicability, whereas more often than not other authors do not even advance any motivation whatsoever for its use, as if this were completely selfevident. Because of the fairly large literature on nonplanar waves, we have cited here only a representative selection of those papers addressing electrostatic modes in unmagnetized plasmas, where the description involves only one spatial coordinate, r, without angular dependence.…”
Section: Basic Equationsmentioning
confidence: 99%
“…However, one finds in the literature other plasma models, which then either lead to an equation like (23), but with more complicated coefficients, [12][13][14][15][16][17][18][19][20][21]24,25,30,32,33,36,[38][39][40][41][42]44,46,49,54 or to modifications of related evolution equations like the Burgers, 23,31,35 KdV-Burgers, 22,37,45,47,48 Gardner, [26][27][28][29]34,43,44,[50][51][52][53]55,56 or Schamel 23 equations. The standard forms of these equations have been well studied in the literature over many decades.…”
Section: Higher Orders and Nonlinear Evolution Equationsmentioning
confidence: 99%
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“…In reality, this solution is the double layer (DL) solution that has been shown in some recently published articles. [3][4][5][6][7][8][9] In fact, the GSs solution is completely different from their solution and has been studied by several authors 2,[6][7][8][9][10][11] We would like to point out the fact that both Gardner SWs and DLs are the solutions of the standard Gardner (sG) equation, which has been described elaborately in Refs. 2 and 3.…”
mentioning
confidence: 99%