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HERO ID
2658364
Reference Type
Journal Article
Title
Solar wind driven dust acoustic instability with Lorentzian kappa distribution
Author(s)
Arshad, K; Ehsan, Z; Khan, SA; Mahmood, S
Year
2014
Is Peer Reviewed?
1
Journal
Physics of Plasmas
ISSN:
1070-664X
EISSN:
1089-7674
Volume
21
Issue
2
DOI
10.1063/1.4865573
Web of Science Id
WOS:000332323400102
Abstract
In a three species electron-ion-dust plasma following a generalized non-Maxwellian distribution function (Lorentzian or kappa), it is shown that a kinetic instability of dust-acoustic mode exists. The instability threshold is affected when such (quasineutral) plasma permeates through another static plasma. Such case is of interest when the solar wind is streaming through the cometary plasma in the presence of interstellar dust. In the limits of phase velocity of the waves larger and smaller than the thermal velocity of dust particles, the dispersion properties and growth rate of dust-acoustic mode are investigated analytically with validation via numerical analysis. (C) 2014 AIP Publishing LLC.
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