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Deep conceptual problems associated with classical black holes can be addressed in string theory by the ``fuzzball'' paradigm, which provides a microscopic description of a black hole in terms of a thermodynamically large number of regular, horizonless, geometries with much less symmetry than the corresponding black hole.
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https://doi.org/10.5281/zenodo.3522086 . To find out more, visit http://einsteintoolkit.org
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M. Bianchi, D. Consoli, A. Grillo, and F. Morales, “Black Hole and Fuzzball Quasinormal Modes from quantum Seiberg-Witten curves,”. to appear (2021)
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