Investigation of solitary waves in warm plasma for smaller order relativistic effects with variable pressures and inertia of electrons

In the two component relativistic plasmas subject to pressure variation of adiabatic electrons and isothermal ions, both compressive and rarefactive KdV solitons are established in a quite different physical plasma model. It is desirable to define c(s) in a new way to substantiate the validity of the model under relativistic effects. The corresponding mathematical condition is also determined, which is a new report of this kind. It is also interesting to report that the relativistic rarefactive solitons cease to exist below some critical ion initial streaming speed v(i0) for a fixed temperature a and electron streaming speed v(e0). Besides, higher initial flux v(i0) of ions under constant temperature is observed to generate higher speed vi at the passage of time which causes to increase (in relativistic sense) its mass diminishing thereby the growth of soliton amplitudes.