The influence of non-Maxwellian ions on the ion-dust streaming instability in a complex plasma is investigated. The ion susceptibility employed for the calculations self-consistently accounts for the acceleration of the ions by a homogeneous background electric field and their collisions with neutral gas particles via a Bhatnagar-Gross-Krook collision term [e.g., A. V. Ivlev et al., Phys. Rev. E 71, 016405 (2005)], leading to significant deviations from a shifted Maxwellian distribution. The dispersion relation and the properties of the most unstable mode are studied in detail and compared with the Maxwellian case. The largest deviations occur at low to intermediate ion-neutral damping. In particular, the growth rate of the instability for ion streaming below the Bohm speed is found to be lower than in the case of Maxwellian ions, yet remains on a significant level even for fast ion flows above the Bohm speed. (C) 2015 AIP Publishing LLC.
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Univ Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USAUniv Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USA
Rosenberg, M.
Shukla, P. K.
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Ruhr Univ Bochum, Fac Phys & Astron, Int Ctr Adv Studies Phys Sci, D-44780 Bochum, GermanyUniv Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USA
机构:
Indian Inst Technol Madras, Dept Aerosp Engn, Chennai 600036, Tamil Nadu, IndiaIndian Inst Technol Madras, Dept Aerosp Engn, Chennai 600036, Tamil Nadu, India
Sundar, Sita
Moldabekov, Zhandos A.
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Al Farabi Kazakh Natl Univ, Inst Expt & Theoret Phys, 71 Al Farabi Str, Alma Ata 050040, Kazakhstan
Inst Appl Sci & IT, 40-48 Shashkin Str, Alma Ata 050038, KazakhstanIndian Inst Technol Madras, Dept Aerosp Engn, Chennai 600036, Tamil Nadu, India