On the strength of the Kerr singularity and cosmic censorship

DOI10.1016/S0375-9601(00)00185-7zbMath0959.83027arXivgr-qc/0003068OpenAlexW2052445948MaRDI QIDQ1569624

Paweł Ziȩba, Wiesław Rudnicki

Publication date: 3 July 2000

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0003068

zbMATH Keywords

cosmic censorshipstrong curvature singularitycollapse situationsKerr singularityKerr-like naked singularitiesrepulsive effects

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Equations of motion in general relativity and gravitational theory (83C10)

Cites Work

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• Conditions for the occurrence of strong curvature singularities
• Black hole interiors cannot be totally vicious
• Cosmic censorship for Kerr-like collapse
• The formation of black holes in nonspherical collapse and cosmic censorship
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Curvature conditions for the occurrence of a class of spacetime singularities
• Maximal Analytic Extension of the Kerr Metric
• Global Structure of the Kerr Family of Gravitational Fields
• The Large Scale Structure of Space-Time

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