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Excitation of kinetic Alfvén wave s by streaming ions in a dusty magnetoplasma with generalized ( r , q ) distribution function
Author(s) -
Rubab Nazish,
Riaz Farrukh,
Zaheer Sadia,
Noreen Naila,
Shah Hassan A.
Publication year - 2021
Publication title -
contributions to plasma physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.531
H-Index - 47
eISSN - 1521-3986
pISSN - 0863-1042
DOI - 10.1002/ctpp.202000182
Subject(s) - physics , excitation , dispersion relation , kinetic energy , distribution function , ion , dispersion (optics) , instability , range (aeronautics) , magnetic field , plasma , atomic physics , wavenumber , electron , streaming instability , function (biology) , computational physics , quantum electrodynamics , classical mechanics , condensed matter physics , quantum mechanics , astrophysics , materials science , solar system , planetesimal , composite material , evolutionary biology , biology
We investigate the parallel streaming effects on the dispersion characteristics of a kinetic Alfvén wave (KAW) in a low β dusty magnetoplasma. To analyse the influence of streaming ions obeying generalized ( r , q ) distribution function, hot and magnetized electrons, and mobile charged dust, a theoretical approach has been used for the instability analysis by employing two potential theories. A linear kinetic dispersion relation of Alfvén waves is derived, whose solutions are used to interpret the numerical and analytical results. The solutions of dispersion relation indicate that the characteristics of KAWs are transformed when generalized ( r , q ) distribution function is employed instead of its Maxwellian counterpart. We also found that the unstable modes have a strong dependence on spectral indices r and q , dust parameters, and plasma β . For the excitation of KAWs, the streaming velocity has been observed to be within the sub‐Alfvén range, whereas when it extends to the super‐Alfvén range, the growth rates are significantly suppressed. The observations further show that an ambient magnetic field and superthermal particles inhibit the growth of an electromagnetic wave to a significant degree and have a stabilizing effect on the wave mode, whereas an increasing concentration of low‐energy particles contributes to enhancing growth rates.