Nonlinear Soliton Interactions in Relativistic Magnetized Systems: Implications for Space and Astrophysical Phenomena
This paper explores the formation and propagation of solitons in a three-fluid weakly relativistic plasma system influenced by an external magnetic field. Employing Normal Mode Analysis and the Reductive Perturbation Technique (RPT), we derive phase velocity relations and examine the effects of density inhomogeneity, relativistic corrections, and magnetic field strength on nonlinear wave evolution [1-3].