Charged Bardeen and Hayward metrics become singular under deformed Einstein–Maxwell equations; more stringent regularity conditions are derived and improved regular charged metrics are constructed.
Gravitational field of a spinning mass as an example of algebraically special metrics
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gr-qc 2years
2026 2representative citing papers
A pedagogical introduction to GR starting from the weak-field limit, deriving Einstein's equations, and applying them to black holes, gravitational waves, and cosmology.
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Charging up regular black holes
Charged Bardeen and Hayward metrics become singular under deformed Einstein–Maxwell equations; more stringent regularity conditions are derived and improved regular charged metrics are constructed.
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A short course in general relativity
A pedagogical introduction to GR starting from the weak-field limit, deriving Einstein's equations, and applying them to black holes, gravitational waves, and cosmology.