Higher-Dimensional Rotating Black Holes
Presenting author: Eli¨ka Klozová
The most general higher-dimensional rotating black hole is described by the Kerr-NUT-(A)dS metric. It includes rotational and NUT parameters as well as the cosmological constant, and can describe various geometries (maximally symmetric spaces, Euclidean instanton, black hole solutions). It also admits explicit and hidden symmetries associated with the principal closed conformal Killing-Yano tensor. In this talk I would like to present some basic properties of this metric.