An analytic effective model for hairy black holes
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Publication:1632092
DOI10.1016/j.physletb.2018.05.018zbMath1404.83040arXiv1803.09089OpenAlexW2794857716WikidataQ126009751 ScholiaQ126009751MaRDI QIDQ1632092
Eugen Radu, Thomas Delplace, Yves Brihaye, Carlos A. R. Herdeiro
Publication date: 13 December 2018
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1803.09089
hairy black holeanalytic computation of thermodynamic quantitiesasymptotically flat black holebald horizon
Related Items (6)
Scalar charges and the first law of black hole thermodynamics ⋮ No scalar condensations outside reflecting stars with coupling terms from Ginzburg-Landau models ⋮ Black holes with scalar hair in light of the Event Horizon Telescope ⋮ Thermodynamically stable asymptotically flat hairy black holes with a dilaton potential ⋮ No-go theorem for static boson stars with negative cosmological constants ⋮ Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations
Cites Work
- Black rings in six dimensions
- Myers-Perry black holes with scalar hair and a mass gap: unequal spins
- Black holes in higher dimensional space-times
- Microscopic origin of the Bekenstein-Hawking entropy
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- Stationary black holes: uniqueness and beyond
- The four laws of black hole mechanics
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- Covariant Conservation Laws in General Relativity
- Quantum gravito-optics: a light route from semiclassical gravity to quantum gravity
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- General relativistic boson stars
- Black Holes and Entropy
- Schwarzschild field inn dimensions and the dimensionality of space problem
- Black holes in higher dimensions
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