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Plasma effects on weak gravitational lensing and shadows of Sen black holes*

Dilmurod UmarovNational Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, UzbekistanOdil YunusovInha University in Tashkent, Ziyolilar 9, Tashkent 100170, UzbekistanFarruh AtamurotovAlfraganus University, Yukori Karakamish street 2a, 100190 Tashkent, UzbekistanAhmadjon AbdujabbarovNew Uzbekistan University, Movarounnahr street 1, Tashkent 100000, UzbekistanSushant G. GhoshAstrophysics and Cosmology Research Unit, School of Mathematics, Statistics and Computer Science, University of KwaZulu-Natal, Durban 4000, South Africa
Chinese Physics Cjournal2025en
ABI

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Abstract We investigate the optical properties of the spacetime surrounding a Sen black hole, focusing on the black hole shadow, weak gravitational lensing, and time delay effects. Our analysis reveals that the effective charge of the Sen black hole significantly influences these phenomena. Specifically, an increase in the effective charge leads to a decrease in the radius of the photon sphere and a corresponding decrease in the size of the black hole shadow. Additionally, the bending angle of light rays diminishes as the effective charge increases. Our study provides observational bounds on the effective charge based on these optical characteristics. We also examine the magnification of source brightness using the lens equation and analyze the time delay of light in the presence of a surrounding plasma medium. Our findings offer new insights into the impact of effective charge and plasma on the observational signatures of Sen black holes.

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Koʻrsatkichlar — AkademScholar · Tez orada