Smoothness of the future and past trapped sets in Kerr–Newman–Taub-NUT spacetimes

DOI10.1088/1361-6382/AAAA5BzbMath1386.83087arXiv1710.02403OpenAlexW3099940128MaRDI QIDQ4637795

Marius A. Oancea, Claudio F. Paganini

Publication date: 26 April 2018

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1710.02403

zbMATH Keywords

black holesshadowsKerr-Newman-Taub-NUT

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)

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Cites Work

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• Decay for solutions of the wave equation on Kerr exterior spacetimes. III: The full subextremalcase \(|a| < M\).
• Aberrational Effects for Shadows of Black Holes
• Photon regions and shadows of accelerated black holes
• Shadows of Kerr black holes with and without scalar hair
• The fingerprints of black holes—shadows and their degeneracies
• Global Structure of the Kerr Family of Gravitational Fields
• Global analysis of the Kerr-Taub-NUT metric
• Physical interpretation of the NUT family of solutions
• Exact Space-Times in Einstein's General Relativity

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