Abstract
The propagation characteristics of weakly nonlinear electron acoustic waves in the presence of nonisothermal (trapped) hot electrons are investigated in collisional plasmas. The dynamics of the nonlinear waves are found to be governed by Schamel–Burgers and Schamel–Korteweg–de Vries–Burgers-type equations depending on the strength of the nonisothermal parameter. Burgers’ terms appear due to the anomalous dissipation introduced by the collisions between cold electrons and immobile ions in the presence of collective phenomena (plasma current). The derived nonlinear equations are solved analytically with the help of the Tanh method. The time-dependent computational results well agree with the analytical results and predict the possibility of the oscillatory and monotonic shock-like structures depending on the strength of the collisional drag and nonisothermality of hot electrons. The trapped electrons significantly modify the amplitude and width of the nonlinear pulse. The results may explain the shock formation and the particle acceleration mechanism in auroral plasma region.
Graphical Abstract
Similar content being viewed by others
Data Availability
This manuscript has associated data in a data repository. [Authors’ comment: The data that support the findings of this study are available from the corresponding author upon reasonable request.]
References
F.S. Mozer, C.W. Carlson, M.K. Hudson, R.B. Torbert, B. Parady, J. Yatteau, M.C. Kelley, Phys. Rev. Lett. 38, 292 (1977)
C.A. Cattell, J. Dombeck, J.R. Wygant, M.K. Hudson, F.S. Mozer, M.A. Temerin, W.K. Peterson, C.A. Kletzing, C.T. Russell, R.F. Pfaff, Geophys. Res. Lett. 26, 425 (1999)
R.L. Tokar, S.P. Gary, Geophys. Res. Lett. 11, 1180 (1984)
T. Miyake, Y. Omura, H. Matsumoto, J. Geophys. Res.: Space Phys. 105, 23239 (2000)
R. Ergun, C. Carlson, L. Muschietti, I. Roth, J.P. McFadden, Nonlinear Process. Geophys. 6, 187 (1999)
C. Cattell, J. Dombeck, J. Wygant, J.F. Drake, M. Swisdak, M.L. Goldstein, W. Keith, A. Fazakerley, M. André, E. Lucek et al., J. Geophys. Res.: Space Phys. 110, A01211 (2005)
S. Chowdhury, S. Biswas, N. Chakrabarti, R. Pal, Phys. Plasmas 24, 062111 (2017)
B.D. Fried, R.W. Gould, Phys. Fluids 4, 139 (1961)
M.F. Thomsen, H.C. Barr, S.P. Gary, W.C. Feldman, T.E. Cole, J. Geophys. Res.: Space Phys. 88, 3035 (1983)
W.C. Feldman, R.C. Anderson, S.J. Bame, J. Geophys. Res.: Space Phys. 88, 96 (1983)
S.P. Gary, R.L. Tokar, Phys. Fluids 28, 2439 (1985)
N. Dubouloz, R. Pottelette, M. Malingre, R.A. Treumann, Geophys. Res. Lett. 18, 155 (1991)
N. Dubouloz, R.A. Treumann, R. Pottelette, M. Malingre, J. Geophys. Res.: Space Phys. 98, 17415 (1993)
C. Cattell, R. Bergmann, K. Sigsbee, C. Carlson, C. Chaston, R. Ergun, J. McFadden, F.S. Mozer, M. Temerin M, R. Strangeway et al., Geophys. Res. Lett. 25, 2053 (1998)
D. Schriver, M.A. Abdalla, Geophys. Res. Lett. 16, 899 (1989)
R.E. Ergun, C.W. Carlson, J.P. McFadden, F.S. Mozer, G.T. Delory, W. Peria, C.C. Chaston, M. Temerin, I. Roth, L. Muschietti et al., Geophys. Res. Lett. 25, 2041 (1998)
J.R. Franz, P.M. Kintner, J.S. Pickett, Geophys. Res. Lett. 25, 1277 (1998)
R. Pottelette, R.E. Ergun, R.A. Treumann, M. Berthomier, C.W. Carlson, J.P. McFadden, I. Roth, Geophys. Res. Lett. 26, 2629 (1999)
R.L. Mace, S. Baboolal, R. Bharuthram, M.A. Hellberg, J. Plasma Phys. 45, 323 (1991)
S.V. Singh, G.S. Lakhina, Planet. Space Sci. 49, 107 (2001)
M. Berthomier, R. Pottelette, L. Muschietti, I. Roth, C.W. Carlson, J. Geophys. Res.: Space Phys. 30, 1 (2003)
M. Dutta, S. Ghosh, N. Chakrabarti, Phys. Rev. E 86, 066408 (2012)
A. Biswas, S. Ghosh, N. Chakrabarti, Phys. Scr. 95, 105603 (2020)
M. Ghosh, S. Pramanik, S. Ghosh, Phys. Lett. A 396, 127242 (2021)
J.R. Asbridge, S.J. Bame, I.B. Strong, J. Geophys. Res. 73, 5777 (1968)
Y. Futaana, S. Machida, Y. Saito, A. Matsuoka, H. Hayakawa, J. Geophys. Res.: Space Phys. 108, SMP-15-1 (2003)
R. Lundin, A. Zakharov, R. Pellinen, H. Borg, B. Hultqvist, N. Pissarenko, E.M. Dubinin, S.W. Barabash, I. Liede, H. Koskinen, Nature 341, 609 (1989)
D. Henry, J.P. Trguier, J. Plasma phys. 8, 311 (1972)
A. Mamun, Eur. Phys. J. D 45, 323 (2000)
T.S. Gill, P. Bala, H. Kaur, N.S. Saini, S. Bansal, J. Kaur, Eur. Phys. J. D 31, 91 (2004)
A.P. Misra, A.R. Chowdhury, Eur. Phys. J. D 37, 105 (2006)
D. Chakraborty, S. Ghosh, Eur. Phys. J. D 75, 1 (2021)
H. Schamel, Plasma Phys. 14, 905 (1972)
H. Schamel, J. Plasma Phys. 9, 377 (1973)
H. Schamel, Phys. Scr. 20, 306 (1979)
H. Schamel, Phys. Scr. T2A, 228 (1982)
H. Schamel and J. Korn, Phys. Scr. T63, 63 (1996)
W.F. El-Taibany, J. Geophys. Res.: Space Phys. 110, 1 (2005)
S. Sultana, A. Mannan, R. Schlickeiser, Eur. Phys. J. D 73, 220 (2019)
D.S. Montgomery, R.J. Focia, H.A. Rose, D.A. Russell, J.A. Cobble, J.C. Fernández, R.P. Johnson, Phys. Rev. Lett. 87, 155001 (2001)
G. Petraconi, H.S. Maciel, J. Phys. D: Appl. Phys. 36, 2798 (2003)
R.E. Ergun, Y.J. Su, L. Andersson, C.W. Carlson, J.P. McFadden, F.S. Mozer, D.L. Newman, M.V. Goldman, R.J. Strangeway, Phys. Rev. Lett. 87, 045003 (2001)
L. Andersson, R.E. Ergun, D.L. Newman, J.P. McFadden, C.W. Carlson, Y.J. Su, Phys. Plasmas 9, 3600 (2002)
R.E. Ergun, L. Andersson, D. Main, Y.J. Su, D.L. Newman, M.V. Goldman, C.W. Carlson, A.J. Hull, J.P. McFadden, F.S. Mozer, J. Geophys. Res.: Space Phys. 109, 1 (2004)
N.B. Nagel, Phys. Chem. Earth, Part A: Solid Earth Geod. 26, 3 (2001)
A.V. Volosevich, Y.I. Galperin, Ann. Geophys. 15, 890 (1997)
S. Watanabe, J. Phys. Soc. Jpn. 45, 276 (1978)
A. Adak, S. Sengupta, Eur. Phys. J. D 73, 197 (2019)
J.K. Xue, Eur. Phys. J. D 26, 211 (2003)
S. Sultana, I. Kourakis, Eur. Phys. J. D 66, 100 (2012)
O. Pezzia, F. Valentini, P. Veltri, Eur. Phys. J. D 68, 128 (2014)
A.R. Seadawy, I. Mujahid, L. Dianchen, Phys. A: Stat. Mech. Appl. 544, 123560 (2020)
W. Malfliet, W. Hereman, Phys. Scr. 54, 563 (1996)
R.C. Davidson, Methods in Nonlinear Plasma Theory (Academic, New York, 1972)
T. Taniuti, Prog. Theor. Phys. Suppl. 55, 1 (1974)
V.I. Karpman, Phys. Scr. 20, 462 (1979)
V.Y. Belashov, S.V. Vladimirov, Solitary Waves in Dispersive Complex Media (Springer, Berlin, 2005)
V.I. Karpman, Non-linear Waves in Dispersive Media: International Series of Monographs in Natural Philosophy, vol. 71 (Elsevier, Amsterdam, 2016)
H. Schamel, J. Korn, Phys. Scr. T63, 63 (1996)
R.S. Johnson, J. Fluid Mech. 42, 49 (1970)
Acknowledgements
The authors (A. S. and S. P.) would like to thank the DST and UGC, Govt. of India for providing INSPIRE Fellowship (Ref. DST/INSPIRE Fellowship/2017/IFI70322) and Dr. D. S. Kothari Post Doctoral Fellowship(Ref. PH/19-20/0016), respectively. The authors thank the referees for the careful reading and offering constructive suggestions to improve the manuscript. The authors would also like to acknowledge Mr. Debkumar Chakraborty for his valuable help and suggestions.
Author information
Authors and Affiliations
Contributions
All authors have contributed equally to the paper.
Corresponding author
Ethics declarations
Conflict of interest
The authors have no relevant financial or non-financial interests to disclose.
Appendix A: Derivations of the analytical shock solutions
Appendix A: Derivations of the analytical shock solutions
In Eq. (35), we put \(\phi _{1}(\chi )=f_1^2(Y)\) [where \(Y=\tanh (c\chi )\) and \(c^{-1}\) is the characteristic width of the solution] to eliminate the square root term and substituting this, we obtain
Following the standard procedure [53], \(f_1(Y)\) is expressed as the power series of Y as
Substituting this expansion in (A.1) and then balancing the highest powers (the second and fourth terms in right-hand side), we obtain \(N=1\). Finally, we assume the solution of Eq. (35) of the form
Putting this solution into the ODE [Eq. (35)] and equating the coefficients of like powers of \(\tanh (c\chi )\), we obtain the system of simultaneous homogeneous equations as
After some elementary matrix operations, we obtain the following system of equations
The last two equations are independent of \(u_f\), and therefore, solving the first equation, we obtain
However, only the \(\varPhi _{-}\) root yields the physically consistent solution (see Sect. 5) and thereby we consider only the root \(\varPhi _{-}\) as
This result well agree with our fixed point analysis of the SKdVB equation Eq.(18). Finally, the last two equations of Eq. (A.5) yields
This clearly shows in case of − sign, the \(c^{-1}\) (width) becomes infinite at a critical value of \(\mu \), which is unphysical, and therefore, we consider
Similarly, for SB equation [Eq. (21); \(b\gg O(\sqrt{\epsilon })\)], proceeding as before, we determine \(N=2\) and the solution is then assumed as
Substituting Eq. (A.10) into Eq. (44) and then equating the coefficients of different powers of \(\tanh (c\chi )\), we obtain the system of equations as
Again after some elementary matrix operations, we obtain the following system of equations,
From these equations, we obtain
These results are also well agree with our fixed point analysis of SB equation [Eq. (21)].
Rights and permissions
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
About this article
Cite this article
Shome, A., Pramanik, S. & Ghosh, S. Electron acoustic shock waves in nonisothermal dissipative plasmas. Eur. Phys. J. D 76, 217 (2022). https://doi.org/10.1140/epjd/s10053-022-00548-7
Received:
Accepted:
Published:
DOI: https://doi.org/10.1140/epjd/s10053-022-00548-7