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Plasma lensing and particle dynamics in the vicinity of a Dyonic black hole solution in the context a perfect fluid

Allah DittaDepartment of Mathematics, School of Science, University of Management and Technology, Lahore 5400, PakistanSikander MehmoodGovernment Graduate College Sahiwal, Department of Mathematics, Sahiwal, PakistanWajiha TanveerGovernment Graduate College Sahiwal, Department of Mathematics, Sahiwal, PakistanWaleed AhmadGovernment Graduate College Sahiwal, Department of Mathematics, Sahiwal, PakistanAwad A. IbraheemDepartment of Physics, Faculty of Science, King Khalid University, Abha, Saudi ArabiaRana Muhammad ZulqarnainDepartment of Mathematics, Saveetha School of Engineering, SIMATS Thandalam, Chennai - 602105 Tamilnadu, IndiaFarruh AtamurotovNew Uzbekistan University, Movarounnahr str. 1, Tashkent 100000, Uzbekistan
Nuclear Physics Bjournal2025en
ABI

Аннотация

This article investigates the particle motion properties, and plasma lensing in weak gravitational field around a Dyonic black hole solution in a perfect fluid. We analyze the motion of massive and massless particles by studying the effective potential, energy, and angular momentum as a function of electric and magnetic charge, the fluid parameters, a , and the surrounding field parameter ω . We have examined the features using Dyonic black holes, including horizon structure, photon orbits, and ISCO radius, to better understand the effect of black hole parameters on their behaviour. Our findings indicate that by increasing the electric charge q E , magnetic charge, q M , and surrounding field parameter ω brings the orbits closer to the central compact object. In contrast, the fluid parameter a has an opposing effect, shifting the ISCO outward. Wa have also determined the deflection angle of light rays surrounding the black hole in a weak plasma environment using the uniform and SIS plasma fields, and found that black holes parameters have clear effect on deflection angle.

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