“…[1][2][3][4][5] The study of electron-positronion (EPI) plasmas has been growing extensively due to their presence in the early universe, in the active galactic nuclei, in the pulsar magnetosphere, ionosphere, in the solar atmospheres, etc. [6][7][8][9][10][11] It is well known that when positrons are introduced into an electron-ion plasma, the response of the electrostatic waves changes significantly in comparison to the usual two component plasmas. [5,12,13] Therefore, it is worthwhile to study the nonlinear wave propagation in electronpositron-ion plasmas for understanding the dynamical behaviour of astrophysical and laboratory plasmas.…”