Dispersion Properties of a Dusty Plasma Containing Nonspherical Rotating Dust Grains

Details Dispersion Properties of a Dusty Plasma Containing Nonspherical Rotating Dust Grains Dispersion Properties of a Dusty Plasma Containing Nonspherical Rotating Dust Grains

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000phrvl..84.2626m&link_type=abstract

Physical Review Letters, Volume 84, Issue 12, March 20, 2000, pp.2626-2629

Astronomy and Astrophysics

Astrophysics

26

Scientific paper

The dispersion relation for a dusty plasma containing elongated and rotating charged dust grains is obtained by assuming that the dipole moments of the dust particulates are nonzero. The longitudinal waves with frequency close to the angular rotation frequency of the dust grains are found to be unstable. The results should be relevant to enhanced fluctuations in astrophysical environments.

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