2019
DOI: 10.1016/j.cjph.2019.06.010
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Higher order corrections and temperature effects to ion acoustic shock waves in quantum degenerate electron-ion plasma

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Cited by 33 publications
(7 citation statements)
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“…For our numerical analysis, we have considered the range of the plasma parameters as Z l = 6 ∼ 13, Z h = 35 ∼ 65, n l0 = 3 × 10 30 cm −3 ∼ 7 × 10 30 cm −3 , n h0 = 4 × 10 29 cm −3 ∼ 07 × 10 33 cm −3 , and n p0 = 1 × 10 31 cm −3 ∼ 10 × 10 31 cm −3 . A number of authors considered inertial non-relativistic ion(s) [14,16,40,[44][45][46][47][48][49][50][51] and inertialess non-relativistic and/or ultra-relativistic [14][15][16]28,40,[44][45][46][47][48][49][50][51][52][53] electrons and positrons to investigate electrostatic [14][15][16]28,40,[44][45][46][47][48][49][51][52][53] or gravito-acoustic [50] waves in DQP, especially in white dwarfs and neutron stars.…”
Section: Resultsmentioning
confidence: 99%
“…For our numerical analysis, we have considered the range of the plasma parameters as Z l = 6 ∼ 13, Z h = 35 ∼ 65, n l0 = 3 × 10 30 cm −3 ∼ 7 × 10 30 cm −3 , n h0 = 4 × 10 29 cm −3 ∼ 07 × 10 33 cm −3 , and n p0 = 1 × 10 31 cm −3 ∼ 10 × 10 31 cm −3 . A number of authors considered inertial non-relativistic ion(s) [14,16,40,[44][45][46][47][48][49][50][51] and inertialess non-relativistic and/or ultra-relativistic [14][15][16]28,40,[44][45][46][47][48][49][50][51][52][53] electrons and positrons to investigate electrostatic [14][15][16]28,40,[44][45][46][47][48][49][51][52][53] or gravito-acoustic [50] waves in DQP, especially in white dwarfs and neutron stars.…”
Section: Resultsmentioning
confidence: 99%
“…They took the aid of Abel's theorem and the variation of parameter method to analyze such equations. In the last decade, a lot of researchers conducted several analytical investigations on the higher-order effect in changing the behavior of shock waves [32][33][34][35][36] and other nonlinear waves [37][38][39]. El-Labany et al [32], El-Monier et al [33], and Hossen et al [34] investigated DIA shock structures in dense plasmas.…”
Section: Introductionmentioning
confidence: 99%
“…Many authors have emphasized the importance and significance of higher-order corrections/effects in studying the various nonlinear structures in different plasma environments [17,18]. To determine how higher-order nonlinear dispersion and dissipation terms affect the higher-order KdV-type/Burgers-type equation, a variety of investigations have been conducted [19,20].…”
mentioning
confidence: 99%
“…By using single variable transformation, ς = ξ − Uτ in eq. ( 15), the stationary localized shock solution is obtained as [7,26]…”
mentioning
confidence: 99%