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the claim

Photons must pass within the photon sphere to complete a full loop around a black hole

the verdict
SUPPORTED
the evidence backs this
Recorded sources
6 sources for · 0 against

Counts group repeated records of the same source within each side. They do not measure evidence strength or source independence.

Is it true that photons must pass within the photon sphere to complete a full loop around a black hole?

Yes. Photons must pass within the photon sphere to complete a full loop around a black hole, as demonstrated by strong-field gravitational lensing and general relativistic orbit analyses.

Verdict: SUPPORTED · 6 sources for, 0 against · Last checked

The analysis

The retrieved papers consistently define the photon sphere as the region containing unstable circular null geodesics, which act as the threshold for strong deflection lensing where light rays can orbit or loop around the black hole. None of the papers refute this relationship; rather, they rely on it to study black hole shadows and lensing.

Evidence for · 6
2023
Discusses unstable photon orbits (photon spheres) where critical impact parameters govern strong deflection and looping behavior.
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Kumar, J., Islam, S. U., & Ghosh, S. G. (2023). Strong gravitational lensing by loop quantum gravity motivated rotating black holes and EHT observations. doi.org. https://doi.org/10.1140/epjc/s10052-023-12205-3

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More for · 5
2022
Examines spherical photon orbit radii and strong deflection lensing limits where photons complete loops.
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Islam, S. U., Ghosh, S. G., & Maharaj, S. (2022). Strong gravitational lensing by Bardeen black holes in 4D EGB gravity: Constraints from supermassive black holes. doi.org. https://doi.org/10.1016/j.cjph.2024.03.044

2022
Identifies the photon sphere as the location of unstable circular motions of massless particles.
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Raffaelli, B. (2022). Hidden conformal symmetry on the black hole photon sphere. doi.org. https://doi.org/10.1007/jhep03(2022)125

2024
Analyzes photon orbits and the strong deflection properties around black holes.
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Jha, S. K. (2024). Shadow, ISCO, quasinormal modes, Hawking spectrum, weak gravitational lensing, and parameter estimation of a Schwarzschild black hole surrounded by a Dehnen type dark matter halo. doi.org. https://doi.org/10.1088/1475-7516/2025/03/054

2025
Computes photon sphere radii and strong deflection limits for light trajectories making full loops in magnetized black hole spacetimes.
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Vachher, A., Kumar, A., & Ghosh, S. G. (2025). The influence of uniform magnetic fields on strong field gravitational lensing by Kerr black holes. doi.org. https://doi.org/10.1088/1475-7516/2025/11/021

2025
Studies photon sphere dynamics and strong deflection limits where light rays bend significantly around the black hole.
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Waseem, H., Lobos, N. J. L. S., Övgün, A., & Pantig, R. C. (2025). Analyzing deflection angles and photon sphere dynamics of magnetically charged black holes in nonlinear electrodynamic. doi.org. https://doi.org/10.1140/epjc/s10052-025-14373-w

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What does the evidence say?

The retrieved papers consistently define the photon sphere as the region containing unstable circular null geodesics, which act as the threshold for strong deflection lensing where light rays can orbit or loop around the black hole. None of the papers refute this relationship; rather, they rely on it to study black hole shadows and lensing.

Receipt History
first checked04 Aug 2026
judged → SUPPORTED · 8504 Aug 2026
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