Ion-acoustic solitary waves in e-p-i plasmas with (r, q)-distributed electrons and kappa-distributed positrons
Shahnaz Kouser
Department of Physics, GC University, Lahore, Pakistan
Search for more papers by this authorCorresponding Author
Muhammad Nouman Sarwar Qureshi
Department of Physics, GC University, Lahore, Pakistan
Correspondence
Muhammad Nouman Sarwar Qureshi, Department of Physics, GC University, 54000 Lahore, Pakistan.
Email: nouman_sarwar@yahoo.com
Search for more papers by this authorKhalid Hussain Shah
Department of Physics, GC University, Lahore, Pakistan
Search for more papers by this authorHassan Amir Shah
Department of Physics, FCC (A Charted University), Lahore, Pakistan
Search for more papers by this authorShahnaz Kouser
Department of Physics, GC University, Lahore, Pakistan
Search for more papers by this authorCorresponding Author
Muhammad Nouman Sarwar Qureshi
Department of Physics, GC University, Lahore, Pakistan
Correspondence
Muhammad Nouman Sarwar Qureshi, Department of Physics, GC University, 54000 Lahore, Pakistan.
Email: nouman_sarwar@yahoo.com
Search for more papers by this authorKhalid Hussain Shah
Department of Physics, GC University, Lahore, Pakistan
Search for more papers by this authorHassan Amir Shah
Department of Physics, FCC (A Charted University), Lahore, Pakistan
Search for more papers by this authorAbstract
In this paper, we have studied the propagation of non-linear ion-acoustic waves in a plasma comprising of (r, q)-distributed electrons and kappa-distributed positrons. We have investigated the effect of complete electron distribution profile on the propagation of small, as well as arbitrary, amplitude solitons (via pseudopotential technique) by using generalized (r, q) distribution, which exhibits a spiky and flat top nature at low energies and a super-thermal tail at high energies. Interestingly, for negative values of r, solitons are formed with both polarities, positive (compressive) and negative (rarefactive), separately within a small amplitude limit and exist simultaneously in an arbitrary amplitude limit. We also found that the propagation of solitons has been affected by the change in parameters r, q, positron concentration, and electron to positron temperature ratio. The results presented in this study add to the fundamental understanding of the complete profile of the electron distribution function, high- and low-energy parts, and in the formation of compressive and rarefactive small and finite amplitude solitons in both space and astrophysical plasmas.
REFERENCES
- 1M. L. Burns, Positron-Electron Pairs in Astrophysics, American Institute of Physics, Melville, NY 1983.
- 2F. C. Miller, P. J. Wiita, Active Galactic Nuclei, Springer, Berlin 1987.
- 3F. C. Michel, Rev. Mod. Phys. 1982, 54, 869.
- 4F. C. Michel, Theory of Neutron Star Magnetosphere, Chicago University, Chicago, IL 1991.
- 5V. Berezhiani, D. D. Tskhakaya, P. K. Shukla, Phys. Rev. A 1992, 46, 6608.
- 6T. Kotani, N. Kawai, M. Matsuoka, W. Brinkmann, Publ. Astron. Soc. Jpn. 1996, 48, 619.
- 7R. Greaves, C. Surko, Phys. Rev. Lett. 1995, 75, 3846.
- 8P. Helander, D. J. Ward, Phys. Rev. Lett. 2003, 90, 135004.
- 9S. Mahmood, A. Mushtaq, H. Saleem, New J. Phys. 2003, 5, 281.
- 10H. Saleem, S. Mahmood, Phys. Plasmas 2003, 10, 2612.
- 11H. Saleem, Q. Haque, J. Vranges, Phys. Rev. E 2003, 67, 057402.
- 12H. Saleem, Phys. Plasmas 2006, 13, 034503.
- 13R. Saeed, A. Shah, M. N. Ui Haq, Phys. Plasmas 2010, 17, 102301.
- 14S. Ali Shan, S. A. El-Tantawy, W. M. Moslem, Phys. Plasmas 2013, 20, 082104.
- 15A. P. Misra, A. R. Chowdhury, Chaos, Solitons Fractals 2003, 15, 801.
- 16R. G. Greaves, M. D. Tinkle, C. M. Surko, Phys. Plasmas 1994, 1, 1439.
- 17G. Sarri, W. Schumaker, A. Di Piazza, M. Vargas, B. Dromey, M. E. Dieckmann, V. Chvykov, A. Maksimchuk, V. Yanovsky, Z. He, Phys. Rev. Lett. 2013, 110, 255002.
- 18H. Washimi, T. Taniuiti, Phys. Rev. Lett. 1966, 17, 966.
- 19S. I. Popal, S. V. Vladimirov, P. K. Shukla, Phys. Plasmas 1995, 2, 716.
- 20Y. N. Nejoh, Phys. Plasmas 1996, 3, 1447.
- 21E. I. El-Awady, S. A. El-Tantawy, W. M. Moslem, P. K. Shukla, Phys. Lett. A 2010, 374, 3216.
- 22K. H. Shah, M. N. S. Qureshi, W. Masood, H. A. Shah, Phys. Plasmas 2018, 25, 042303.
- 23K. Saba, M. N. S. Qureshi, W. Masood, Astrophys. Space Sci. 2018, 363, 216.
- 24W. Massod, M. N. S. Qureshi, P. H. Yoon, H. A. Shah, J. Geophys. Res. 2015, 120, 101.
- 25M. N. S. Qureshi, K. H. Shah, J. Shi, W. Masood, H. A. Shah, Contrib. Plasma Phys. 2019, 60, e201900065.
- 26S. Sumbul, M. N. S. Qureshi, H. A. Shah, AIP Adv. 2019, 9, 025315.
- 27D. Summers, R. M. Thorne, Phys. Fluids B 1991, 3, 1835.
- 28V. M. Vasyliunas, J. Geophys. Res. 1968, 73, 2839.
- 29W. Feldman, S. Bame, S. Gary, J. Gosling, D. McComas, M. Thomsen, G. Paschmann, N. Sckopke, M. Hoppe, C. Russell, Phys. Rev. Lett. 1982, 49, 199.
- 30V. Pierrard, J. Lemaire, J. Geophys. Res. 1996, 101, 7923.
- 31M. Maksimovic, V. Pierrard, J. F. Lemaire, Astron. Astrophys. 1997, 324, 725.
- 32S. Magni, H. E. Roman, R. Bami, C. Riccardi, T. Pierre, D. Guyomarc'h, Phys. Rev. E 2005, 72, 026403.
- 33S. Sultana, I. Kourakis, N. S. Saini, M. A. Hellberg, Phys. Plasmas 2010, 17, 032310.
- 34S. Sultana, G. Sarri, I. Kourakis, Phys. Plasmas 2012, 19, 012310.
- 35A. Tahir, W. Masood, M. N. S. Qureshi, H. A. Shah, P. H. Yoon, Phys. Plasmas 2016, 23, 062307.
- 36K. Saba, M. N. S. Qureshi, W. Masood, Phys. Plasmas 2019, 26, 092114.
- 37M. N. S. Qureshi, W. Nasir, W. Masood, P. H. Yoon, H. A. Shah, S. J. Schwartz, J. Geophys. Res. 2014, 119, 10059.
- 38M. N. S. Qureshi, H. A. Shah, G. Murtaza, S. J. Schwartz, F. Mahmood, Phys. Plasmas 2004, 11, 3819.
- 39K. H. Shah, M. N. S. Qureshi, W. Masood, H. A. Shah, AIP Advances 2018, 8, 085010.
- 40K. Saba, M. N. S. Qureshi, W. Masood, AIP Adv. 2020, 10, 025002.
- 41H. Khalilpour, Astrophys. Space Sci. 2016, 361, 271.
- 42S. Asif, S. Mahmood, Q. Haque, Phys. Plasmas 2011, 18, 114501.
- 43G. Lu, Y. Liu, Y. Wang, L. Stenflo, S. I. Popel, M. Y. Yu, J. Plasma Phys. 2010, 76, 267.
- 44J. Srinivas, S. I. Popel, P. K. Shukla, J. Plasma Phys. 1996, 55, 209.
- 45T. V. Losseva, S. I. Popel, A. P. Golub, P. K. Shukla, Phys. Plasmas 2009, 16, 093704.
- 46T. V. Losseva, S. I. Popel, A. P. Golub, Y. N. Izvekova, P. K. Shukla, Phys. Plasmas 2011, 19, 013703.
- 47T. V. Losseva, S. I. Popel, A. P. Golub, Plasma Phys. Rep. 2012, 38, 729.
- 48M. N. S. Qureshi, G. Pallocchia, R. Bruno, M. B. Cattaneo, V. Formisano, H. Reme, M. J. Bosqued, I. Dandouras, J. A. Sauvard, L. M. Kistler, E. Mobius, B. Klecker, C. W. Carlson, J. P. McFadden, G. K. Parks, M. McCarthy, A. Korth, R. Lundin, A. Balogh, H. A. Shah, Solar wind ten 2003 Edited: M. Velli, R. Bruno, F. Malara.
- 49G. K. Parks, E. Lee, N. Lin, F. Mozer, M. Wilber, I. Dandouras, H. Reme, E. Lucek, A. Fazakerley, M. Goldstein, C. Gurgiolo, P. Canu, N. Cornilleau-Wehrlin, P. Decreau, Phys. Rev. Lett. 2007, 98, 265001.
- 50Z. Kiran, H. A. Shah, M. N. S. Qureshi, G. Murtaza, Solar Phys. 2006, 236, 167.
- 51D. Strickland, G. Mourou, Opt. Commun. 1985, 56, 219.
- 52R. A. Smith, Bull. Am. Phys. Soc. 2008, 53, 221.