Charged Black Holes in a Rotating Gross-Perry-Sorkin Monopole Background

Understand

We present a new class of stationary charged black hole solutions to five-dimensional Einstein-Maxwell-Chern-Simons theories.

• We construct the solutions by utilizing so called the squashing transformation.
• At infinity, our solutions behave as a four-dimensional flat spacetime plus a `circle' and hence describe a Kaluza-Klein black hole.
• More precisely, our solutions can be viewed as a charged rotating black hole in a rotating Gross-Perry-Sorkin monopole background with the black hole rotation induced from the background rotation.