Cosmic dust-ion-acoustic waves, spherical modified Kadomtsev-Petviashvili model, and symbolic computation

Details Cosmic dust-ion-acoustic waves, spherical modified Kadomtsev-Petviashvili model, and symbolic computation Cosmic dust-ion-acoustic waves, spherical modified Kadomtsev-Petviashvili model, and symbolic computation

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phpl...13k2901g&link_type=abstract

Physics of Plasmas, Volume 13, Issue 11, pp. 112901-112901-6 (2006).

Computer Science

Sound

78

Dusty Or Complex Plasmas, Plasma Crystals, Sound Waves, Nonlinear Phenomena: Waves, Wave Propagation, And Other Interactions, Rings And Dust, Saturn, Planetary Rings

Scientific paper

The spherical modified Kadomtsev-Petviashvili (smKP) model is hereby derived with symbolic computation for the dust-ion-acoustic waves with zenith-angle perturbation in a cosmic dusty plasma. Formation and properties of both dark and bright smKP nebulons are obtained and discussed. The relevance of those smKP nebulons to the supernova shells and Saturn's F-ring is pointed out, and possibly observable nebulonic effects for the future cosmic plasma experiments are proposed. The difference of the smKP nebulons from other types of nebulons is also analyzed.

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