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The propagation characteristics of nonlinear dust acoustic solitary waves in a complex plasma system with nonthermal electrons and trapped ions are investigate in this work. The nonlinear dispersion relation of dust acoustic waves is obtained by using the linear method, and the two-dimensional autonomous system governing the motion of nonlinear dust acoustic waves is derived by using the Sagdeev potential method. At the same time, the specific expression of the Sagdeev potential function is obtained based on the Sagdeev potential equation. The numerical simulations are used to analyze the phase portraits of the two-dimensional autonomous system, revealing the linear periodic wave orbits, nonlinear periodic wave orbits, and homoclinic orbits co-existing in the complex dusty plasma system with nonthermal electrons and trapped ions. Furthermore, from the variations of the Sagdeev potential function with different system parameters it follows that only the compressive solitary waves exist in this complex plasma system. The significant influences of various system parameters on the amplitude, width, and waveform of the nonlinear dust acoustic solitary wave in the complex plasma system are discussed in detail. The results demonstrate that the Mach number, the nonthermal electrons and trapped ions, undisturbed dust particle number density, temperature, and charge have important effects on the propagating characteristics of the nonlinear dust acoustic solitary waves in a complex plasma with nonthermal electrons and trapped ions.
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Keywords:
- nonlinear dust acoustic solitary waves /
- Sagdeev potential method /
- nonthermal electron distribution /
- trapped ions distribution
[1] Gill T S, Bains A S, Bedi C 2010 Phys. Plasmas. 17 013701Google Scholar
[2] Zahed H, Emadi E 2016 Phys. Plasmas. 23 083706Google Scholar
[3] Singh K, Kaur N, Saini N S 2017 Phys. Plasmas. 24 063703Google Scholar
[4] Akhter T, Mannan A, Mamun A A 2013 Plasma. Phys. Rep. 39 548Google Scholar
[5] Anowarm G M, Mamuna A 2008 Phys. Lett. 372 5896Google Scholar
[6] Rasheed A, Tsintsadze N L, Murtaza G 2011 Phys. Plasmas. 18 112701Google Scholar
[7] Rao N N, Shukla P K, Yu M Y 1990 Planet. Space. Sci. 38 543Google Scholar
[8] Barkan A, Merlino R L, N D Angelo 1995 Phys. Plasmas 2 3563Google Scholar
[9] Xie B S, He K F, Huang Z Q 1998 Chin. Phys. Lett. 15 892Google Scholar
[10] Lin M M, Duan W S 2005 Commun. Theor. Phys. 44 719Google Scholar
[11] Murad A, Zakir U, Haque Q 2019 Braz. J. Phys. 49 79Google Scholar
[12] Sarmah B, Devi A, Sarma J 2019 InfoKara 8 115Google Scholar
[13] Soni P K, Aravindakshan H, Kakad B, Kakad A 2021 Phys. Scr. 96 105604Google Scholar
[14] Jahan S, Banik S, Chowdhury N A, Mannan A, Mamun A A 2022 Gases 2 22Google Scholar
[15] 林麦麦, 付颖捷, 宋秋影, 于腾萱, 文惠珊, 蒋蕾 2022 物理学报 71 095203Google Scholar
Lin M M, Fu Y J, Song Q Y, Yu T X, Wen H S, Jiang L 2022 Acta Phys. Sin. 71 095203Google Scholar
[16] 林麦麦, 王明月, 蒋蕾 2023 物理学报 72 035201Google Scholar
Lin M M, Wang M Y, Jiang L 2023 Acta Phys. Sin. 72 035201Google Scholar
[17] Mamani C 2023 Braz. J. Phys. 53 110Google Scholar
[18] Saha T, Chatterjee P 2009 Phys. Plasmas 16 013707Google Scholar
[19] Mamun A A, Shukla P K 2009 Phys. Rev. E 80 037401Google Scholar
[20] Selim M M 2016 Eur. Phys. J. Plus 131 93Google Scholar
[21] Gill T S, Kaur H, Bansal S, Saini N S, Bala P 2007 Eur. Phys. J. D 41 151Google Scholar
[22] Mamun A A, Alam M N, Azad A K 1998 Phys. Plasmas 5 1212Google Scholar
[23] Mandal D, Lesur M, Gravier E, Sama J N, Guillevic A, Sarazin Y 2023 Plasma Phys. Controlled Fusion 65 055001Google Scholar
[24] Kaniadakis G, Lavagno A, Quarati P 1996 Phys. Lett. B 369 308Google Scholar
[25] El-Labany S K, El-Taibany W F, El-Abbasy O M 2007 Chaos, Solitons Fractals 33 813Google Scholar
[26] Salam M A, Akbar M A, Ali M Z 2021 Results Phys. 26 104376Google Scholar
[27] Kian R B, Mahdieh M H 2023 Fluid Dyn. Res. 55 35503Google Scholar
[28] Taylor H A, Daniell R E, Hartle R E, Brinton H C, Bauer S J, Scarf F L 1981 Adv. Space Res. 1 247Google Scholar
[29] Sabry R, Moslem W M, Shukla P K 2009 Phys. Plasmas 16 032302Google Scholar
[30] Amour R, Tribeche M 2010 Plasma Phys. 17 063702Google Scholar
[31] Haider M M, Ferdous T, Duha S S 2014 Cent. Eur. J. Phys. 12 701Google Scholar
[32] Ghai Y, Saini S N 2017 Astrophys. Space Sci. 362 3Google Scholar
[33] Annou K, Bahamida S, Annou R 2011 Pramana-J. Phys. 76 513Google Scholar
[34] Mamun A A 1998 Phys. Scr. 57 258Google Scholar
[35] Demiray H, Abdikian A 2019 Chaos, Solitons Fractals 121 50Google Scholar
[36] Rasheed A, Murtaza G, Tsintsadze NL 2010 Phys. Rev. E 82 016403Google Scholar
[37] El-Shamy E, Al-Chouikh R, El-Depsy A, Al-Wadie N 2016 Phys. Plasmas 23 122122Google Scholar
[38] Cairns R A, Mamum A A, Bingham R, Boström R, Dendy R O, Nairn C M C, Shukla P K 1995 Geophys. Res. Lett. 22 2709Google Scholar
[39] Misra A P, Wang Y L 2015 Commun. Nonlinear Sci. Numer. Simul. 22 1360Google Scholar
[40] Pakzad H R, Tribeche M 2012 J. Fusion Energy 31 611Google Scholar
[41] El-Labany S K, El-Taibany W F, El-Bedwehy N A, Zedan N A 2017 Plasmas Phys. Rep. 43 756Google Scholar
[42] Nejoh Y 1992 IEEE Trans. Plasmas Sci. 20 80Google Scholar
[43] Saha A, Tamang J 2019 Adv. Space Res. 63 1596Google Scholar
[44] Saha A, Chatterjee P 2014 Astrophys. Space Sci. 350 631Google Scholar
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图 8 Sagdeev势函数$ V\left( \phi \right) $随不同系统参数的变化规律 (a) α = 0.4, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (b) M = 1.3, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (c) M = 1.3, α = 0.4, σi = 0.5, σd = 0.02, δ = 2; (d) M = 1.3, α = 0.4, b = 0.8, σd = 0.02, δ = 2; (e) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, δ = 2; (f) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, σd = 0.02
Figure 8. Variations of Sagdeev potential $ V\left( \phi \right) $ with different parameters: (a) α = 0.4, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (b) M = 1.3, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (c) M = 1.3, α = 0.4, σi = 0.5, σd = 0.02, δ = 2; (d) M = 1.3, α = 0.4, b = 0.8, σd = 0.02, δ = 2; (e) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, δ = 2; (f) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, σd = 0.02.
图 9 孤立波$ \phi $的波形随不同参数的变化规律 (a) α = 0.4, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (b) M = 1.3, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (c) M = 1.3, α = 0.4, σi = 0.5, σd = 0.02, δ = 2; (d) M = 1.3, α = 0.4, b = 0.8, σd = 0.02, δ = 2; (e) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, δ = 2; (f) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, σd = 0.02
Figure 9. Waveform variations of the solitary waves $ \phi $ with different parameters: (a) α = 0.4, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (b) M = 1.3, b = 0.8, σi = 0.5, σd = 0.02, δ = 2; (c) M = 1.3, α = 0.4, σi = 0.5, σd = 0.02, δ = 2; (d) M = 1.3, α = 0.4, b = 0.8, σd = 0.02, δ = 2; (e) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, δ = 2; (f) M = 1.3, α = 0.4, b = 0.8, σi = 0.5, σd = 0.02.
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[1] Gill T S, Bains A S, Bedi C 2010 Phys. Plasmas. 17 013701Google Scholar
[2] Zahed H, Emadi E 2016 Phys. Plasmas. 23 083706Google Scholar
[3] Singh K, Kaur N, Saini N S 2017 Phys. Plasmas. 24 063703Google Scholar
[4] Akhter T, Mannan A, Mamun A A 2013 Plasma. Phys. Rep. 39 548Google Scholar
[5] Anowarm G M, Mamuna A 2008 Phys. Lett. 372 5896Google Scholar
[6] Rasheed A, Tsintsadze N L, Murtaza G 2011 Phys. Plasmas. 18 112701Google Scholar
[7] Rao N N, Shukla P K, Yu M Y 1990 Planet. Space. Sci. 38 543Google Scholar
[8] Barkan A, Merlino R L, N D Angelo 1995 Phys. Plasmas 2 3563Google Scholar
[9] Xie B S, He K F, Huang Z Q 1998 Chin. Phys. Lett. 15 892Google Scholar
[10] Lin M M, Duan W S 2005 Commun. Theor. Phys. 44 719Google Scholar
[11] Murad A, Zakir U, Haque Q 2019 Braz. J. Phys. 49 79Google Scholar
[12] Sarmah B, Devi A, Sarma J 2019 InfoKara 8 115Google Scholar
[13] Soni P K, Aravindakshan H, Kakad B, Kakad A 2021 Phys. Scr. 96 105604Google Scholar
[14] Jahan S, Banik S, Chowdhury N A, Mannan A, Mamun A A 2022 Gases 2 22Google Scholar
[15] 林麦麦, 付颖捷, 宋秋影, 于腾萱, 文惠珊, 蒋蕾 2022 物理学报 71 095203Google Scholar
Lin M M, Fu Y J, Song Q Y, Yu T X, Wen H S, Jiang L 2022 Acta Phys. Sin. 71 095203Google Scholar
[16] 林麦麦, 王明月, 蒋蕾 2023 物理学报 72 035201Google Scholar
Lin M M, Wang M Y, Jiang L 2023 Acta Phys. Sin. 72 035201Google Scholar
[17] Mamani C 2023 Braz. J. Phys. 53 110Google Scholar
[18] Saha T, Chatterjee P 2009 Phys. Plasmas 16 013707Google Scholar
[19] Mamun A A, Shukla P K 2009 Phys. Rev. E 80 037401Google Scholar
[20] Selim M M 2016 Eur. Phys. J. Plus 131 93Google Scholar
[21] Gill T S, Kaur H, Bansal S, Saini N S, Bala P 2007 Eur. Phys. J. D 41 151Google Scholar
[22] Mamun A A, Alam M N, Azad A K 1998 Phys. Plasmas 5 1212Google Scholar
[23] Mandal D, Lesur M, Gravier E, Sama J N, Guillevic A, Sarazin Y 2023 Plasma Phys. Controlled Fusion 65 055001Google Scholar
[24] Kaniadakis G, Lavagno A, Quarati P 1996 Phys. Lett. B 369 308Google Scholar
[25] El-Labany S K, El-Taibany W F, El-Abbasy O M 2007 Chaos, Solitons Fractals 33 813Google Scholar
[26] Salam M A, Akbar M A, Ali M Z 2021 Results Phys. 26 104376Google Scholar
[27] Kian R B, Mahdieh M H 2023 Fluid Dyn. Res. 55 35503Google Scholar
[28] Taylor H A, Daniell R E, Hartle R E, Brinton H C, Bauer S J, Scarf F L 1981 Adv. Space Res. 1 247Google Scholar
[29] Sabry R, Moslem W M, Shukla P K 2009 Phys. Plasmas 16 032302Google Scholar
[30] Amour R, Tribeche M 2010 Plasma Phys. 17 063702Google Scholar
[31] Haider M M, Ferdous T, Duha S S 2014 Cent. Eur. J. Phys. 12 701Google Scholar
[32] Ghai Y, Saini S N 2017 Astrophys. Space Sci. 362 3Google Scholar
[33] Annou K, Bahamida S, Annou R 2011 Pramana-J. Phys. 76 513Google Scholar
[34] Mamun A A 1998 Phys. Scr. 57 258Google Scholar
[35] Demiray H, Abdikian A 2019 Chaos, Solitons Fractals 121 50Google Scholar
[36] Rasheed A, Murtaza G, Tsintsadze NL 2010 Phys. Rev. E 82 016403Google Scholar
[37] El-Shamy E, Al-Chouikh R, El-Depsy A, Al-Wadie N 2016 Phys. Plasmas 23 122122Google Scholar
[38] Cairns R A, Mamum A A, Bingham R, Boström R, Dendy R O, Nairn C M C, Shukla P K 1995 Geophys. Res. Lett. 22 2709Google Scholar
[39] Misra A P, Wang Y L 2015 Commun. Nonlinear Sci. Numer. Simul. 22 1360Google Scholar
[40] Pakzad H R, Tribeche M 2012 J. Fusion Energy 31 611Google Scholar
[41] El-Labany S K, El-Taibany W F, El-Bedwehy N A, Zedan N A 2017 Plasmas Phys. Rep. 43 756Google Scholar
[42] Nejoh Y 1992 IEEE Trans. Plasmas Sci. 20 80Google Scholar
[43] Saha A, Tamang J 2019 Adv. Space Res. 63 1596Google Scholar
[44] Saha A, Chatterjee P 2014 Astrophys. Space Sci. 350 631Google Scholar
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