| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9861319 | Physics Letters B | 2005 | 9 Pages |
Abstract
We consider charged rotating black holes in 5-dimensional Einstein-Maxwell theory. These black holes are asymptotically flat, they possess a regular horizon of spherical topology and two independent angular momenta associated with two distinct planes of rotation. We discuss their global and horizon properties, and derive a generalized Smarr formula. We construct these black holes numerically, focusing on black holes with a single angular momentum, and with two equal-magnitude angular momenta.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Jutta Kunz, Francisco Navarro-Lérida, Anna Katinka Petersen,