Charged Rotating Black Holes in Five Dimensional U(1)^3 Gauged N=2 Supergravity

TL;DR

This paper derives a comprehensive family of non-extremal rotating black hole solutions with three charges in five-dimensional gauged supergravity, unifying many previously known solutions and extending the understanding of black hole configurations in this theory.

Contribution

It provides the first general solution for non-extremal 3-charge rotating black holes in five-dimensional U(1)^3 gauged supergravity with equal rotation parameters.

Findings

Includes all known extremal solutions as special cases.

Reduces to non-extremal solutions of pure supergravity when charges are equal.

Generalizes the solution space for charged rotating black holes in this theory.

Abstract

We obtain the general solution for non-extremal 3-charge dilatonic rotating black holes in the U(1)^3 gauged five-dimensional N=2 supergravity coupled to two vector multiplets, in the case where the two rotation parameters are set equal. These solutions encompass all the previously-known extremal solutions, and, by setting the three charges equal, the recently-obtained non-extremal solutions of N=2 gauged five-dimensional pure supergravity.