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This work presents a unified mathematical framework for investigating the influence of an external magnetic field on Hamiltonian phase-space dynamics, Akhmediev breather solitons, and modulational instability in heavy ion-acoustic waves propagating through a magnetized four-component non-Maxwellian plasma. Using the multiscale perturbation method, a nonlinear Schrödinger equation is obtained to describe the evolution of nonlinear wave envelopes. A traveling-wave reduction transforms this equation into a planar Hamiltonian system, linking its phase-space geometry to analytical solitary-wave solutions. The resulting phase portraits exhibit periodic, superperiodic, and homoclinic trajectories, with the homoclinic orbits yielding paired solitary-wave envelope solutions related by polarity reversal. Furthermore, the results demonstrate that the plasma system supports both bright and dark solitons under the influence of combined kappa(κ)-Cairns statistics, depending on the balance between dispersion and nonlinearity. The influence of heavy ion-acoustic plasma parameters, including electron superthermality, magnetic field strength, positron concentration, charged-weighted ion-mass ratio, and temperature ratio on the instability threshold, growth rate, and spectral bandwidth is systematically examined. Exact Akhmediev breather solutions are constructed in the modulationally unstable regime using the Darboux transformation. The modulation frequency governs their spatial periodicity and localization during envelope evolution, while the magnetic field modifies their spatial period in a manner that depends on the carrier wavenumber. These findings elucidate how magnetic-field strength and non-Maxwellian particle statistics jointly influence nonlinear envelope dynamics. This study establishes a unified connection between Hamiltonian phase-space geometry, sign-reversal symmetric solitary waves, modulational instability spectra, and nonlinear breather excitations, providing a mathematical description of magnetic field effects on nonlinear wave dynamics in non-Maxwellian plasmas relevant to space and laboratory environments.
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Ikram et al. (2026) studied this question.
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