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Shadows and weak gravitational lensing for black holes within Einstein-Maxwell-scalar theory*

Ahmad Al‐BadawiDepartment of Physics, Al-Hussein Bin Talal University, P. O. Box: 20, Ma'an, 71111, JORDANMirzabek Alloqulov, Institute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, Uzbekistan, Tashkent , UZBEKISTANSanjar ShaymatovZhejiang University of Technology, Institute for Theoretical Physics and Cosmology, Zheijiang University of Technology, Hangzhou 310023, China, Hangzhou, Zhejiang, 310014, CHINABobomurat AhmedovUlugh Beg Astron Inst, Astronomicheskaya 33, Tashkent, UZBEKISTAN
Chinese Physics Cjournal2024en
ABI

Аннотация

Abstract In this study, we investigated the optical properties of charged black holes within the Einstein-Maxwell-scalar (EMS) theory. We evaluated the shadow cast by these black holes and obtained analytical solutions for both the radius of the photon sphere and that of the shadow. We observed that black hole parameters γ and β both influence the shadow of black holes. We also found that the photon sphere and shadow radius increase as a consequence of the presence of the parameter γ . Interestingly, the shadow radius decreases first and then remains unchanged owing to the impact of the parameter β . Finally, we analyzed the weak gravitational lensing and total magnification of lensed images around black holes. We found that the charge of the black holes and the parameter β both have a significant impact, reducing the deflection angle. Similarly, the same behavior for the total magnification was observed, also as a result of the effect of the charge of the black holes and the parameter β .

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