Blackfolds, Plane Waves and Minimal Surfaces Jay Armas1;2 and Matthias Blau2 1 Physique Th´eoriqueet Math´ematique Universit´eLibre de Bruxelles and International Solvay Institutes ULB-Campus Plaine CP231, B-1050 Brussels, Belgium 2 Albert Einstein Center for Fundamental Physics, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
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[email protected] Abstract Minimal surfaces in Euclidean space provide examples of possible non-compact horizon ge- ometries and topologies in asymptotically flat space-time. On the other hand, the existence of limiting surfaces in the space-time provides a simple mechanism for making these configura- tions compact. Limiting surfaces appear naturally in a given space-time by making minimal surfaces rotate but they are also inherent to plane wave or de Sitter space-times in which case minimal surfaces can be static and compact. We use the blackfold approach in order to scan for possible black hole horizon geometries and topologies in asymptotically flat, plane wave and de Sitter space-times. In the process we uncover several new configurations, such as black arXiv:1503.08834v2 [hep-th] 6 Aug 2015 helicoids and catenoids, some of which have an asymptotically flat counterpart. In particular, we find that the ultraspinning regime of singly-spinning Myers-Perry black holes, described in terms of the simplest minimal surface (the plane), can be obtained as a limit of a black helicoid, suggesting that these two families of black holes are connected. We also show that minimal surfaces embedded in spheres rather than Euclidean space can be used to construct static compact horizons in asymptotically de Sitter space-times.