Abstract
A dusty plasma, composed of charge-fluctuating dust, and hybrid Cairns–Tsallis ions and Boltzmann electrons is considered to study the cylindrical/spherical dust acoustic shock waves. The reductive perturbation method is used to derive the cylindrical/spherical KdV–Burgers equation. It is important to note here that the main cause of dissipation term in the given plasma model is dust charge fluctuation. Nonplanar KdV–Burgers equation is later on solved by the weighted residual method in the limits of weak dissipation. The solution demonstrates that the wave attenuates quicker as one approaches the cylinder’s axis or the sphere’s center, and the consequences are depicted in various 2D graphics. We have studied the various parametric influences on such shock structure and also showed how the gradual variations of these parameters affect the generation and structure of the shocks in their respective domain. Much of the experiments on dusty plasma with nonadiabatic dust charge fluctuation will benefit from the parametric study.
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References
Allen J. E. 1992, Phys. Scr., 45, 497
Amour R., Tribeche M., Shukla P. K. 2012, Astrophys. Space Sci., 338, 287
Bala P., Gill T. S., Bains A. S., Kaur H. 2017, Indian J. Phys., 91, 1625
Baluku T. K., Hellberg M. A., Mace R. L. 2008, Phys. Plasmas, 15, 033701
Bansal S., Aggarwal M., Gill T. S. 2018, Braz. J. Phys., 48, 597
Bansal S., Aggarwal M., Gill T. S. 2019, Contrib. Plasma Phys., 59, e201900047
Bansal S., Aggarwal M. 2019, Pramana – J. Phys., 92, 49
Bansal S., Aggarwal M., Gill T. S. 2020, Phys. Plasmas, 27, 083704
Demiray H., El-Zaher E. R. 2020, Results Phys. 18, 103293
El-Labany S. K., Diab A. M., El-Shamy E. F. 2002, Astrophys. Space Sci., 282, 595
El-Hanbaly A. M., El-Shewy E. K., Sallah M., Darweesh H. F. 2016, Commun. Theor. Phys. J. Plasma Phys., 65, 606
Ergun R., Carlson B., McFadden M. 1998, Geophys. Res. Lett., 25, 2025
Ghosh S., Chaudhuri T. K., Sarkar S., Khan M., Gupta M. R. 2002, Phys. Rev. E, 46, 037401
Gill T. S., Kaur H. 2000, Pramana, 55, 855
Gill T. S., Bansal S. 2020, Chaos Solitons Fract. 147, 110953
Goertz C. K., Shan L., Havnes O. 1998, Geophys. Res. Lett., 15, 84
Gupta M. R., Sarkar S., Ghosh S., Debnath M., Khan M. 2001, Phys. Rev. E, 63, 046406
Havnes O., Aslaksen T., Hartquist T. W., et al. 1995, J. Geophys. Res., 100, 1731
Kakati M., Goswami K. S. 1998, Phys. Plasmas, 5, 4508
Kruger H. 2003, Jupiter’s Dust Disc. An Astrophysical Laboratory (Shaker Verlag: Aachen)
Kumar R., Malik H. K., Singh K. 2012, Phys. Plasmas, 19, 012114
Li F., Havnes O. 2001, Phys. Rev. E, 64, 066407, 1
Losseva T. V., Popel S. I., Golub A. P. 2012, Plasma Phys. Rep. 38, 729
Losseva T. V., Popel S. I., Golub A. P. 2020, Plasma Phys. Rep. 46, 1007
Lotko W., Kennel C. F. 1983, J. Geophys. Res., 88, 381
Luo Q-Z., D’Angelo N., Merlino R. L. 1999, Phys. Plasmas, 6, 3455
Mamun A. A., Shukla P. K. 2002, Geophys. Res. Lett., 29, 1870, https://doi.org/10.1029/2002GL015219
Mamun A. A. 2008, Phys. Lett. A, 372, 686
Mamun A. A., Shukla P. K. 2011, J. Plasma Phys., 77, 437
Merriche A., Tribeche M. 2017, Ann. Phys., 376, 436
Nakamura Y., Bailung H., Shukla P. K. 1999, Phys. Rev. Lett., 83, 1602
Popel S. I., Tsytovich V. N. 1999, Astrophys. Space Sci., 264, 219
Popel S. I., Golub A. P., Losseva T. V. 2001, JETP Lett., 74, 362
Popel S. I., Andreev S. N., Gisko A. A., Golub A. P., Losseva T. V. 2004, Plasma Phys. Rep., 30, 284
Popel S. I., Gisko A. A. 2006, Nonlinear Process. Geophys., 13, 223
Rao N. N., Shukla P. K., Yu M. Y. 1990, Planet Space Sci., 38, 543
Sakanaka P. H., Shukla P. K. 2000, Phys. Scr., T84, 181
Sethi P., Singh K., Saini N. S. 2018, Zeitschrift für Naturforschung A, 73, 795
Shukla P. K. 2001, Phys. Plasmas, 8, 1791
Shukla P. K., Mamun A. A. 2002, Introduction to Dusty Plasma Physics (Institute of Physics: Bristol)
Tribeche M., Amour R., Shukla P. K. 2012, Phys. Rev. E, 85, 037401
Verheest F. 2000, Waves in Dusty Space Plasmas (Kluwer Academic: Dordrecht)
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Bansal, S., Aggarwal, M. & Gill, T.S. Effects of nonadiabatic dust charge variation on cylindrical/spherical shock waves propagating in a hybrid Cairns–Tsallis plasma. J Astrophys Astron 43, 29 (2022). https://doi.org/10.1007/s12036-022-09811-0
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DOI: https://doi.org/10.1007/s12036-022-09811-0