Black hole image in Heisenberg-Euler electrodynamics

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In this paper we use a geodesic method for constructing a black hole shadow. It’s based on numerical integration of geodesic equations by the 5th order Dormand-Prince method. We construct an image of charged black hole shadow in the framework of Heisenberg-Euler electrodynamics and perform a comparative analysis of this image with a similar image in the classical case of Maxwell electrodynamics

Black hole image, nonlinear electrodynamics, gravitational lensing

Короткий адрес: https://sciup.org/142241763

IDR: 142241763   |   DOI: 10.17238/issn2226-8812.2024.1.132-135

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