New Geometries for Black Hole Horizons
arXiv:1504.01393 · doi:10.1007/JHEP07(2015)048
Abstract
We construct several classes of worldvolume effective actions for black holes by integrating out spatial sections of the worldvolume geometry of asymptotically flat black branes. This provides a generalisation of the blackfold approach for higher-dimensional black holes and yields a map between different effective theories, which we exploit by obtaining new hydrodynamic and elastic transport coefficients via simple integrations. Using Euclidean minimal surfaces in order to decouple the fluid dynamics on different sections of the worldvolume, we obtain local effective theories for ultraspinning Myers-Perry branes and helicoidal black branes, described in terms of a stress-energy tensor, particle currents and non-trivial boost vectors. We then study in detail and present novel compact and non-compact geometries for black hole horizons in higher-dimensional asymptotically flat space-time. These include doubly-spinning black rings, black helicoids and helicoidal -branes as well as helicoidal black rings and helicoidal black tori in .
v2: 37pp, 5figures, typos fixed, matches published version
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- Gravitational Tension, Spacetime Pressure and Black Hole Volume
- Blackfolds, Plane Waves and Minimal Surfaces
- Instabilities of Thin Black Rings: Closing the Gap
- Probing the near-horizon geometry of black rings
- New asymptotically (Anti)-de Sitter black holes in (super)gravity
- Towards higher dimensional black rings