A Static and Spherically Symmetric Hairy Black Hole in the Framework of the Gravitational Decoupling

DOI10.1002/prop.202200171arXiv2303.04119OpenAlexW4322102609MaRDI QIDQ6092857

E. Contreras, Pedro Bargueño, Rodrigo Avalos

Publication date: 23 November 2023

Published in: Fortschritte der Physik (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2303.04119

zbMATH Keywords

quasinormal modeshairy black holesgeodesic analysisgravitational decoupling

Mathematics Subject Classification ID

Quantum theory (81-XX)

Cites Work

• Unnamed Item
• Analytical correspondence between shadow radius and black hole quasinormal frequencies
• Geodesic motion around hairy black holes
• Decoupling gravitational sources in general relativity: the extended case
• Anisotropic Tolman V solution by minimal gravitational decoupling approach
• Probing the minimal geometric deformation with trace and Weyl anomalies
• Beyond Einstein gravity. The minimal geometric deformation approach in the brane-world
• Asymptotically flat black holes with scalar hair: A review
• Quasinormal modes of bumblebee wormhole
• Colored black holes
• Quasinormal ringing of regular black holes in asymptotically safe gravity: the importance of overtones
• Extended gravitational decoupling approach in f(𝒢) gravity
• Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
• Anisotropic ultracompact Schwarzschild star by gravitational decoupling