Abstract

In this paper, we have studied the three-dimensional (3D) electron-acoustic waves (EAWs) in a three-component complex plasma containing q-non-extensive distributed hot electrons and positrons. The propagation characteristics of the 3D electron-acoustic (EA) shock waves under the influence of magnetic field have been studied. Our present plasma model supports the negative potential shocks. Combined action of dissipation $$(\eta )$$ , non-extensivity (q), concentration of positrons ( $$\beta $$ ), temperature ratio of cold electrons to positrons ( $$\sigma $$ ) and magnetic field ( $$\omega _c$$ ) on the EA shock waves has been studied in detail and the findings obtained here will be beneficial in future astrophysical investigations.

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