This paper discusses corrections to black hole theory in general relativity, indicating flaws in traditional models and proposing numerical methods for the Kerr problem.
We discuss corrections to the mainstream theory of black holes in general relativity. We discuss the Schwarzschild point-mass and extended-mass solutions of the Einstein Field Equations, concluding that many of the features traditionally associated with black hole theory are absurd and incorrect. The picture of a point singularity surrounded by a surface singularity at the Schwarzschild radius does not hold water. As an afterthought, we suggest how to solve the Kerr problem (rotating black hole): by numerical methods/machine computation.
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Stuart Boehmer (2025) studied this question.
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