Black holes with only one Killing field
From MaRDI portal
Publication:467208
DOI10.1007/JHEP07(2011)115zbMath1298.83075arXiv1105.4167OpenAlexW3100570632MaRDI QIDQ467208
Jorge E. Santos, Óscar J. C. Dias, Gary T. Horowitz
Publication date: 3 November 2014
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1105.4167
Black holes (83C57) Kaluza-Klein and other higher-dimensional theories (83E15) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (48)
Holographic thermalization, quasinormal modes and superradiance in Kerr-AdS ⋮ Extremal hairy black holes ⋮ Gravitating scalar stars in the large \(D\) limit ⋮ Hairy black holes in \(\mathrm{AdS}_{5}\times S^{5}\) ⋮ Collapse and revival in holographic quenches ⋮ A rotating hairy \(\mathrm{AdS}_{3}\) black hole with the metric having only one Killing vector field ⋮ Black holes with a single Killing vector field: black resonators ⋮ Shaping black holes with free fields ⋮ Non-singular space-times with a negative cosmological constant. V: Boson stars ⋮ Gregory-Laflamme and superradiance encounter black resonator strings ⋮ Flows of rotating extremal attractor black holes ⋮ Rotating hairy black holes in $\mathrm{AdS}_5 \times S^5 $ ⋮ Microstrata ⋮ Superradiance and black resonator strings encounter helical black strings ⋮ New phases of \(\mathcal{N} = 4\) SYM at finite chemical potential ⋮ No-go theorems for hairy black holes in scalar- or vector-tensor-Gauss–Bonnet theory ⋮ Internal structure of hairy rotating black holes in three dimensions ⋮ Kaluza-Klein monopole with scalar hair ⋮ Hairy black holes and the endpoint of \(AdS_{4}\) charged superradiance ⋮ Energy extraction from AdS black holes via superradiance ⋮ \(D = 5\) static, charged black holes, strings and rings with resonant, scalar \(Q\)-hair ⋮ Grey galaxies' as an endpoint of the Kerr-AdS superradiant instability ⋮ Dynamical formation of a hairy black hole in a cavity from the decay of unstable solitons ⋮ Universality of the holographic angular momentum cutoff ⋮ Non-singular spacetimes with a negative cosmological constant: IV. Stationary black hole solutions with matter fields ⋮ Gregory-Laflamme encounters superradiance ⋮ Almost all extremal black holes in AdS are singular ⋮ Resonating AdS soliton ⋮ Attempts at vacuum counterexamples to cosmic censorship in AdS ⋮ Gravitating solitons and black holes with synchronised hair in the four dimensional O(3) sigma-model ⋮ Stirring a black hole ⋮ A new spin on black hole hair ⋮ Hairy black holes and solitons in global \(\mathrm{AdS}_5\) ⋮ Hairy black hole chemistry ⋮ Four-dimensional asymptotically AdS black holes with scalar hair ⋮ Inside black holes with synchronized hair ⋮ Multioscillating black holes ⋮ Phase diagram of the charged black hole bomb system ⋮ Evidence for the existence of a novel class of supersymmetric black holes with AdS 5 ×S 5 asymptotics ⋮ Dynamical boson stars ⋮ Dynamical boson stars ⋮ Hunting for fermionic instabilities in charged AdS black holes ⋮ Inside an asymptotically flat hairy black hole ⋮ Holographic dual of hot Polchinski-Strassler quark-gluon plasma ⋮ Charged black hole bombs in a Minkowski cavity ⋮ AdS nonlinear instability: breaking spherical and axial symmetries ⋮ Stationary black holes: uniqueness and beyond ⋮ Classification of near-horizon geometries of extremal black holes
Cites Work
- Unnamed Item
- Rotating boson stars in \(2+1\) dimensions
- The general Kerr-de Sitter metrics in all dimensions
- Boson stars with negative cosmological constant
- Small hairy black holes in global AdS spacetime
- Small hairy black holes in \(\mathrm{AdS}_{5} {\times} S^{5}\)
- A higher dimensional stationary rotating black hole must be axisymmetric
- An instability of higher-dimensional rotating black holes
- Symmetries of higher dimensional black holes
- Superradiance and Instability of Black Holes
- Gravity and hydrodynamics: lectures on the fluid-gravity correspondence
- Do collapsed boson stars result in new types of black holes?
- The first law of thermodynamics for Kerr–anti-de Sitter black holes
- Asymptotically anti-de Sitter spacetimes: conserved quantities
This page was built for publication: Black holes with only one Killing field
