Non-Singular Charged Black Hole Solution for Non-Linear Source
arXiv:gr-qc/9911084 · doi:10.1023/A:1026640911319
Abstract
A non-singular exact black hole solution in General Relativity is presented. The source is a non-linear electromagnetic field, which reduces to the Maxwell theory for weak field. The solution corresponds to a charged black hole with |q| \leq 2s_c m \approx 0.6 m, having metric, curvature invariants, and electric field bounded everywhere.
3 pages, RevTex
Cited by in corpus (221)
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