Large-amplitude dust inertial Alfvén waves in an electron-depleted dusty plasma
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Final Accepted Manuscript
Affiliation
Department of Planetary Sciences-Lunar and Planetary Laboratory, University of ArizonaIssue Date
2021-11-18Keywords
52.35.Bj52.27.Lw
52.35.Sb
94.05.Fg
52.35.–g
Dusty plasmas
electron depleted
inertial Alfvén waves
Sagdeev pseudopotential
solitary waves
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Springer Science and Business Media LLCCitation
Singh, M., Singh, K., & Saini, N. S. (2021). Large-amplitude dust inertial Alfvén waves in an electron-depleted dusty plasma. Pramana - Journal of Physics.Journal
Pramana - Journal of PhysicsRights
© Indian Academy of Sciences.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The existence of the large-amplitude dust inertial Alfvén waves (DIAWs) has been presented in an electron-depleted, two-fluid dust-ion plasma. Linear analysis shows that the DIAWs travel slower than the dust Alfvén waves. DIAWs are the obliquely (with respect to the external magnetic field) propagating oscillations of dust density, having the characteristics of a solitary wave. In order to observe the nonlinear behaviour of the DIAWs, the Sagdeev pseudopotential method has been used to derive the energy balance equation and from the expression of the Sagdeev pseudopotential, the existence conditions for the DIAWs have also been determined. It is observed that density rarefactions travelling at sub- and super-Alfvénic speeds are associated with DIAWs.Note
12 month embargo; published: 18 November 2021ISSN
0304-4289EISSN
0973-7111Version
Final accepted manuscriptae974a485f413a2113503eed53cd6c53
10.1007/s12043-021-02226-6