2012
DOI: 10.1007/s12648-012-0080-8
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Ion acoustic solitary waves in an electron–ion–positron plasma

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Cited by 12 publications
(7 citation statements)
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“…Recently, a number of authors have studied the nonlinear propagation of the IA waves in EPI plasmas either considering non-degenerate plasma [14][15][16][17][18][19] or degenerate plasmas. [13,[20][21][22][23][24][25] In a degenerate dense plasma, Mamun and Shukla [13] studied the SWs, and implied their results in white dwarfs.…”
Section: Introductionmentioning
confidence: 99%
“…Recently, a number of authors have studied the nonlinear propagation of the IA waves in EPI plasmas either considering non-degenerate plasma [14][15][16][17][18][19] or degenerate plasmas. [13,[20][21][22][23][24][25] In a degenerate dense plasma, Mamun and Shukla [13] studied the SWs, and implied their results in white dwarfs.…”
Section: Introductionmentioning
confidence: 99%
“…For better approximation regarding the solution of the differential equation ( 28), taking terms upto 𝜙 4 we get finally from equation ( 28)…”
Section: Solutions and Amplitudes Of Two-temperature Isothermal Elect...mentioning
confidence: 99%
“…Thus negative, ion plasma is inevitable for our consideration. This negative ion together with positive ion, positron with two-temperature and single temperature isothermal electron plasma have been studied theoretically and experimentally by many authors [1][2][3][4][5][6][7][8][9][10][11][12] for the propagation of ion-acoustic solitary waves. After showing the characteristics of solitary waves in the plasmas, they have reviewed the behaviour of the solitons in various types of plasma models making a close relationship between theoretical and experimental results.…”
Section: Introductionmentioning
confidence: 99%
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“…Thus, it is important to study the behavior of linear and nonlinear waves in e-p-i plasmas. During the past few decades, the research works on linear as well as nonlinear wave propagation in e-p-i plasmas have attracted a considerable interest from many authors [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16][17], because they have great importance to understand the behavior of astrophysical plasmas viz. cluster explosions, pulsar environments, supernovas, and active galactic nuclei [10,18,19].…”
Section: Introductionmentioning
confidence: 99%