What happens to Petrov classification, on horizons of axisymmetric dirty black holes

DOI10.1063/1.4865995zbMath1290.83049arXiv1211.4376OpenAlexW3104246678MaRDI QIDQ5414775

Igor V. Tanatarov, Oleg B. Zaslavskii

Publication date: 7 May 2014

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1211.4376

zbMATH Keywords

black holesPetrov classificationhorizonsboosted Petrov type (BPT)Petrov type (PT)

Mathematics Subject Classification ID

Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Space-time singularities, cosmic censorship, etc. (83C75) Equations of motion in general relativity and gravitational theory (83C10)

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Cites Work

• Unnamed Item
• Singular space-times
• Black hole physics. Basic concepts and new developments
• Global properties of warped solutions in general relativity
• Symmetries at stationary Killing horizons
• Near-horizon symmetries of extremal black holes
• Exact Solutions of Einstein's Field Equations
• Curvature invariants in type-III spacetimes
• Type D Einstein spacetimes in higher dimensions
• Curvature tensors on distorted Killing horizons and their algebraic classification
• Exact Space-Times in Einstein's General Relativity
• The classification of spaces defining gravitational fields

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