Interior of Nonuniform Black Strings
arXiv:0710.1726 · doi:10.1016/j.physletb.2008.05.025
Abstract
We consider nonuniform black strings inside their event horizon. We present numerical evidence, that the singularity touches the horizon as the horizon topology changing transition is reached.
4 pages, 5 figues
References in corpus (17)
- Black Strings and p-Branes are Unstable
- Static Axisymmetric Vacuum Solutions and Non-Uniform Black Strings
- Instability of Ultra-Spinning Black Holes
- On non-uniform black branes
- Fate of the Black String Instability
- The Phase Structure of Higher-Dimensional Black Rings and Black Holes
- The Phase Transition between Caged Black Holes and Black Strings - A Review
- Instabilities of Black Strings and Branes
- A critical dimension in the black-string phase transition
- Topology change in General Relativity and the black-hole black-string transition
- Connecting black holes and black strings
- Properties of Kaluza-Klein black holes
- From Black Strings to Black Holes
- New nonuniform black string solutions
- Evidence that highly non-uniform black strings have a conical waist
- Interior of Distorted Black Holes
- Rotating nonuniform black string solutions
Cited by in corpus (8)
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- Black Holes in Higher-Dimensional Gravity
- Looking at the Gregory-Laflamme instability through quasi-normal modes
- Bumpy black holes
- Harrison transformation and charged black objects in Kaluza-Klein theory
- Distorted 5-dimensional vacuum black hole
- Rotating Black Holes in Higher Dimensions