“…However, RMHD has limitations when modeling several astrophysical systems, like pulsar, gamma-ray burst, etc., see [12] for a detailed discussion. Following the development of non-relativistic two-fluid plasma flow equations [13], [14], [15], [16], [17], [18], [19], several authors have considered an analogous relativistic two-fluid plasma flow equations [20], [21], [22], [23], [24]. Two-fluid relativistic plasma flow equations describe each fluid (ion and electron) in plasma using the equations of special relativistic hydrodynamics (RHD).…”