Spinning black holes with axion hair

DOI10.1088/1361-6382/acf9d6arXiv2306.03662MaRDI QIDQ6047210

Pedro G. S. Fernandes, Richard Brito, Clare Burrage, Vitor Cardoso

Publication date: 9 October 2023

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

Full work available at URL: https://arxiv.org/abs/2306.03662

zbMATH Keywords

charged black holeaxionhairy black hole

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) Computational methods for problems pertaining to relativity and gravitational theory (83-08)

Related Items (1)

Scalarized Kerr-Newman black holes

Cites Work

• Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality
• Numerical methods for finding stationary gravitational solutions
• NON-UNIQUENESS, COUNTERROTATION, AND NEGATIVE HORIZON MASS OF EINSTEIN–MAXWELL–CHERN–SIMONS BLACK HOLES
• Black holes as particle detectors: evolution of superradiant instabilities
• Construction and physical properties of Kerr black holes with scalar hair
• Proof of uniqueness of the Kerr-Newman black hole solution
• On long range axion hairs for black holes

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