| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1848976 | Physics Letters B | 2015 | 7 Pages |
Abstract
In the presence of a complex scalar field scalar–tensor theory allows for scalarized rotating hairy black holes. We exhibit the domain of existence for these scalarized black holes, which is bounded by scalarized rotating boson stars and hairy black holes of General Relativity. We discuss the global properties of these solutions. Like their counterparts in general relativity, their angular momentum may exceed the Kerr bound, and their ergosurfaces may consist of a sphere and a ring, i.e., form an ergo-Saturn.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Burkhard Kleihaus, Jutta Kunz, Stoytcho Yazadjiev,