Role of Neutrinos in Magnetospheric Plasma Environments: A Theoretical Analysis of Particle Dynamics and Aurora Interaction

This study investigates the theoretical interplay between neutrinos and the magnetospheric plasma, focusing on the implications for auroral physics. We explore the potential coupling between the neutrino magnetic moment (\mu_\nu) and intense geomagnetic fields (\mathbf{B}), utilizing the Mikheyev-Smirnov-Wolfenstein (MSW) framework to analyze neutrino flavor evolution in high-density plasma regions. Particle trajectories under these perturbed conditions are simulated using a Runge-Kutta-Fehlberg (RK۴۵) numerical approach. Through a comprehensive sensitivity analysis of coupling constants, we find that although the direct impact of neutrino flux on auroral intensity remains below current spectroscopic detection thresholds, a viable theoretical coupling mechanism exists. Our results suggest that during extreme solar-terrestrial events, this interaction may function as a secondary energy dissipation channel. These findings provide new insights into non-standard neutrino interactions and suggest unexplored avenues for studying neutral lepton dynamics in high-energy astrophysical and geophysical environments.

کلیدواژه ها:

Neutrino Physics ، Magnetospheric Plasma ، Aurora Physics ، Neutrino-Matter Interactions ، Magnetic Field Coupling