K–P–Burgers equation in negative ion-rich relativistic dusty plasma including the effect of kinematic viscosity

Dev A N¹, Deka M K², Sarma J³, Saikia D⁴, Adhikary N C^{4, †,}

Spatial variations of the solitary wave amplitude for different relativistic plasma conditions, the dash line is for γ = 0.2, the solid line is for γ = 0.1, and the dash–dotted line is for γ = 0.01.