Instability of a Kerr-type naked singularity due to light and matter accretion and its shadow

DOI10.1088/1361-6382/ad2318arXiv2301.13751OpenAlexW4391250330MaRDI QIDQ6122666

Unnamed Author, Bayram Tekin

Publication date: 1 March 2024

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

Full work available at URL: https://arxiv.org/abs/2301.13751

zbMATH Keywords

shadownaked singularityKerr black holeinstability of naked singularity

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Cites Work

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• Spherical photon orbits around a Kerr black hole
• Observational phenomena related to primordial Kerr superspinars
• Appearance of Keplerian discs orbiting Kerr superspinars
• Evolution of Kerr superspinars due to accretion counterrotating thin discs
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Photon ring structure of rotating regular black holes and no-horizon spacetimes
• Gravitational Collapse and Space-Time Singularities
• Global Structure of the Kerr Family of Gravitational Fields

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