https://doi.org/10.1140/epjp/s13360-021-01686-4
Regular Article
Dust-acoustic modulated structures in self-gravitating magnetized electron depleted dusty plasmas: multi-rogue waves and dark soliton collisions
1
Faculty of Sciences, University of Maroua, P.O. Box 814, Maroua, Cameroon
2
Higher Teachers’ Training College, University of Maroua, P.O. Box 55, Maroua, Cameroon
3
National Advanced School of Engineering, University of Maroua, P.O. Box 46, Maroua, Cameroon
4
The Max Planck Institute for the Physics of Complex Systems, Nothnitzer Strasse 38, 01187, Dresden, Germany
5
Department of Physics, College of Science and Humanities in Al-Kharj, Prince Sattam bin Addulaziz University, 11942, Al-Kharj, Saudi Arabia
6
Department of Physics, Faculty of Science, Ain Shams University, Cairo, Egypt
7
Department of Physics, Faculty of Science, Port Said University, 42521, Port Said, Egypt
8
Research Center for Physics (RCP), Department of Physics, Faculty of Science and Arts, Al-Mikhwah, Al-Baha University, Al Bahah, Saudi Arabia
Received:
2
September
2020
Accepted:
19
June
2021
Published online:
28
June
2021
A theoretical model has been developed to study the effects of the gravitational attraction and magnetic field on the waves instabilities as well as the dynamics of dust-acoustic rogue waves (RWs) and the collisions of the envelope dark soliton in self-gravitating non-Maxwellian magnetized electron depleted dusty plasma (EDDP). Using the derivative expansion method, the basic fluid equations of the model are converted to the normal nonlinear Schrödinger equation (NLSE). The modulational instability (MI) analysis is used for determining the regions of (un)stable envelope structures (RWs and envelope solitons). According to gravitational force, a new dispersion relation is obtained and analyzed numerically. It is noted that the presence of gravitational force provides the possibility of a novel purely growing instability mode. Effects of gravitational force and magnetic field on the growth rate of MI and the profile of the RWs in unstable regions and on the phase shifts of the colliding dark solitons in stable regions are discussed in detail. In general, the gravitational force leads to destabilized waves whereas the magnetic field plays the stabilizing role. The present investigation may be of relevance for understanding the mechanism which govern the formation and propagation of modulated DA structures (RWs and envelope solitons) in certain astrophysical objects such as Saturn rings, interstellar medium, dark interstellar clouds, HI and HII regions of galaxies.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2021
