Compares observational tests of black hole shadows and stability in astrophysical contexts, suggesting key predictions.
This is the second version (v2) of the Sharipov regular black hole model. It includes new sections on observational tests (shadow comparison with EHT, echoes with LIGO, microlensing with JWST), analytic extension beyond the core, and stability analysis. Two new figures have been added. The model predicts a shadow deviation of up to 5% for γ ≈ 0.70, making it testable with current EHT observations.
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Muhammad Saidjonovij Sharipow (2026) studied this question.
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