Abstract
The spherically symmetric vacuum stress-energy tensor with one assumption concerning its specific form generates the exact analytic solution of the Einstein equations which for larger coincides with the Schwarzschild solution, for smallr behaves like the de Sitter solution and describes a spherically symmetric black hole singularity free everywhere.
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This essay received the fifth award from the Gravity Research Foundation, 1991
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Dymnikova, I. Vacuum nonsingular black hole. Gen Relat Gravit 24, 235–242 (1992). https://doi.org/10.1007/BF00760226
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DOI: https://doi.org/10.1007/BF00760226