Abstract
The nonlinear properties of dust ion-acoustic (DIA) shock waves in a magnetorotating plasma consisting of inertial ions, nonextensive electrons and positrons, and immobile negatively charged dust are examined. The effects of dust charge fluctuations are not included in the present investigation, but the ion kinematic viscosity (collisions) is a source of dissipation, leading to the formation of stable shock structures. The Zakharov-Kuznetsov-Burgers (ZKB) equation is derived using the reductive perturbation technique, and from its solution the effects of different physical parameters, i.e. nonextensivity of electrons and positrons, kinematic viscosity, rotational frequency, and positron and dust concentrations, on the characteristics of shock waves are examined. It is observed that physical parameters play a very crucial role in the formation of DIA shocks. This study could be useful in understanding the electrostatic excitations in dusty plasmas in space (e.g. interstellar medium).
Original language | English |
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Pages (from-to) | 215-223 |
Number of pages | 9 |
Journal | Zeitschrift fur Naturforschung - Section A Journal of Physical Sciences |
Volume | 73 |
Issue number | 3 |
DOIs | |
State | Published - Feb 23 2018 |
Externally published | Yes |
Funding
Acknowledgement: This work was supported by the University Grants Commission, New Delhi, India, under DRS-II (SAP) No. F 530/17/DRS-II/2015 (SAP-I).
Funders | Funder number |
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DRS-II | |
University Grants Commission |
Keywords
- Dust Ion Acoustic
- Nonextensive Distribution
- Shock Waves
- ZKB Equation