A new type of nonsingular black-hole solution in general relativity

DOI10.1142/S0217732314300183zbMath1295.83004arXiv1309.7011OpenAlexW3105937802MaRDI QIDQ2879218

F. R. Klinkhamer

Publication date: 8 September 2014

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1309.7011

zbMATH Keywords

exact solutionstopologygeneral relativity

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (4)

A stealth defect of spacetime ⋮ Comparison of spacetime defects which are homeomorphic but not diffeomorphic ⋮ Lensing and imaging by a stealth defect of spacetime ⋮ A ‘Regularized’ Schwarzschild Solution

Cites Work

• BLACK-HOLE SOLUTION WITHOUT CURVATURE SINGULARITY
• Oscillatory Character of Reissner-Nordström Metric for an Ideal Charged Wormhole
• Maximal Extension of Schwarzschild Metric
• Black-hole Solution Without Curvature Singularity and Closed Timelike Curves
• The Large Scale Structure of Space-Time
• Theory of Diffraction by Small Holes
• Causality and CPT violation from an Abelian Chern-Simons-like term

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