Five-Dimensional Charged Rotating Black Holes
Jutta Kunz, Francisco Navarro-Lerida, and Anna Katinka Petersen
TL;DR
This paper studies five-dimensional charged rotating black holes in Einstein-Maxwell theory, analyzing their properties, deriving formulas, and numerically constructing solutions with different angular momentum configurations.
Contribution
It provides a detailed analysis and numerical construction of 5D charged rotating black holes with various angular momentum configurations, extending understanding of higher-dimensional black hole solutions.
Findings
Black holes have spherical horizon topology and two independent angular momenta.
Derived a generalized Smarr formula for these black holes.
Numerically constructed solutions with single and equal-magnitude angular momenta.
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, focussing on black holes with a single angular momentum, and with two equal-magnitude angular momenta.
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