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(16) 6 However, the integral usually cannot be solved out in an explicit form

Deflection angle According to [58], the deflection angle of light by the rotating black hole at x0 is determined as: αD(x0)= I(x0)− π, (15) where I (x0)= 2 ∫ ∞ x0 dφ dx dx= 2 ∫ ∞ x

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Strong gravitational lensing effects around rotating regular black holes

gr-qc · 2024-12-31 · conditional · novelty 4.0

Strong lensing by rotating regular black holes shifts lensing coefficients, image positions, magnifications, and time delays relative to Kerr, with M87* time delays differing by up to tens of hours while image position shifts remain below 10 microarcseconds.

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  • Strong gravitational lensing effects around rotating regular black holes gr-qc · 2024-12-31 · conditional · none · ref 4

    Strong lensing by rotating regular black holes shifts lensing coefficients, image positions, magnifications, and time delays relative to Kerr, with M87* time delays differing by up to tens of hours while image position shifts remain below 10 microarcseconds.