Jeans modes in dusty plasmas with dust mass distributions

Details Jeans modes in dusty plasmas with dust mass distributions Jeans modes in dusty plasmas with dust mass distributions

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..537...53j&link_type=abstract

WAVES IN DUSTY, SOLAR, AND SPACE PLASMAS. AIP Conference Proceedings, Volume 537, pp. 53-60 (2000).

Physics

Magnetohydrodynamic Waves, Electrostatic Waves And Oscillations

Scientific paper

Self-gravitational modes in dusty plasmas have been extensively studied for both extreme cases of wave propagation: waves propagating parallel to an external magnetic field and perpendicularly propagating waves. Provided the presence of neutral is insignificant, the presence of charged dust species stabilizes plasmas against gravitational collapse, the mechanisms being induced by plasma thermal effects and/or magnetic field pressure. We present here the modifications of magnetosonic modes and electrostatic, parallel modes due to the possible distributions of the dust mass. The necessary adaptations of the corresponding critical Jeans lengths are discussed and extended to intermediate angles of propagation. .

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