BLACK-HOLE SOLUTION WITHOUT CURVATURE SINGULARITY

DOI10.1142/S0217732313501368zbMath1277.83031arXiv1304.2305MaRDI QIDQ2865959

F. R. Klinkhamer

Publication date: 12 December 2013

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

Full work available at URL: https://arxiv.org/abs/1304.2305

zbMATH Keywords

exact solutionstopologygeneral relativityquantum aspects of black holes

Mathematics Subject Classification ID

Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (7)

The remnants in Reissner–Nordström–de Sitter quintessence black hole ⋮ Black hole solutions in a cosmological spacetime background ⋮ Comparison of spacetime defects which are homeomorphic but not diffeomorphic ⋮ A ‘Regularized’ Schwarzschild Solution ⋮ Negative energy particle as an expanding wormhole ⋮ The thermodynamical properties of charged dilaton–axion black hole and its quasi-localized energy ⋮ A new type of nonsingular black-hole solution in general relativity

Cites Work

• Maximal Extension of Schwarzschild Metric

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