Black String Flow
arXiv:1307.2276 · doi:10.1007/JHEP09(2013)068
Abstract
We give an exact description of the steady flow of a black string into a planar horizon. The event horizon is out of equilibrium and provides a simple, exact instance of a `flowing black funnel' in any dimension D>=5. It is also an approximation to a smooth intersection between a black string and a black hole, in the limit in which the black hole is much larger than the black string thickness. The construction extends easily to more general flows, in particular charged flows.
16 pages, 3 figures
References in corpus (8)
- A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric
- Black Strings, Low Viscosity Fluids, and Violation of Cosmic Censorship
- The large D limit of General Relativity
- Symmetries of Higher Dimensional Black Holes
- AdS flowing black funnels: Stationary AdS black holes with non-Killing horizons and heat transport in the dual CFT
- Stationary holographic plasma quenches and numerical methods for non-Killing horizons
- Thermodynamics of the hot BIon
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Cited by in corpus (17)
- Numerical Methods for Finding Stationary Gravitational Solutions
- The holographic dual of a Riemann problem in a large number of dimensions
- Holographic thermal field theory on curved spacetimes
- Holographic duals of evaporating black holes
- Exact Event Horizon of a Black Hole Merger
- Black Droplets
- Steady States of Holographic Interfaces
- Phases of Holographic Hawking Radiation on spatially compact spacetimes
- Overcoming obstacles in nonequilibrium holography
- Dissonant Black Droplets and Black Funnels
- The large D effective theory of black strings in AdS
- To go or not to go with the flow: Hawking radiation at strong coupling
- Kerr Black string flow
- The Flowing BIon
- Black Tunnels and Hammocks
- Towards Fluid Instabilities of Stationary Non-Killing Horizons
- Far-from-equilibrium energy flow and entanglement entropy