Abstract
A theoretical investigation on the formation of Mach cones in weakly and strongly coupled dusty magnetoplasmas has been presented. The salient features of dust‐acoustic and dust‐magnetoacoustic Mach cones in a weakly coupled dusty magnetoplasma as well as dust‐acoustic Mach cones in a strongly coupled dusty magnetoplasma have been clearly explained. The relevance of this theoretical investigation to the formation of such dust‐acoustic and dust‐magnetoacoustic Mach cones in Saturn’s dusty rings and laboratory dusty plasma experiments are discussed.
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